<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article  PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd"><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article"><front><journal-meta><journal-id journal-id-type="publisher-id">JMP</journal-id><journal-title-group><journal-title>Journal of Modern Physics</journal-title></journal-title-group><issn pub-type="epub">2153-1196</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/jmp.2013.410174</article-id><article-id pub-id-type="publisher-id">JMP-38879</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Physics&amp;Mathematics</subject></subj-group></article-categories><title-group><article-title>
 
 
  Is the Space-Time a Superconductor?
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>enceslao</surname><given-names>Santiago-Germán</given-names></name><xref ref-type="aff" rid="aff1"><sub>1</sub></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib></contrib-group><aff id="aff1"><label>1</label><addr-line>Manuel Sandoval Vallarta Institute for Theoretical Physics, Chetumal, México</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>wsan1905@gmail.com</email></corresp></author-notes><pub-date pub-type="epub"><day>17</day><month>10</month><year>2013</year></pub-date><volume>04</volume><issue>10</issue><fpage>1447</fpage><lpage>1467</lpage><history><date date-type="received"><day>July</day>	<month>1,</month>	<year>2013</year></date><date date-type="rev-recd"><day>August</day>	<month>3,</month>	<year>2013</year>	</date><date date-type="accepted"><day>September</day>	<month>4,</month>	<year>2013</year></date></history><permissions><copyright-statement>&#169; Copyright  2014 by authors and Scientific Research Publishing Inc. </copyright-statement><copyright-year>2014</copyright-year><license><license-p>This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/</license-p></license></permissions><abstract><p>
 
 
   At the fundamental level, the 4-dimensional space-time of our direct experience might not be a continuum and discrete quantum entities might “collectively” rule its dynamics. Henceforth, it seems natural to think that in the “low-energy” regime some of its distinctive quantum attributes could, in principle, manifest themselves even at macroscopically large scales. Indeed, when confronted with Nature, classical gravitational dynamics of spinning astrophysical bodies is known to lead to paradoxes: to untangle them, dark matter or modifications to the classical law of gravity are openly considered. In this article, the hypothesis of a fluctuating space-time acquiring “at large distances” the properties of a Bose-Einstein condensate is pushed forward: firstly, it is shown that a natural outcome of this picture is the production of monopoles, dyons, and vortex lines of “quantized” gravitomagnetic—or gyrogravitational—flux along the transition phase; the minimal supported “charge” (and multiples of it) being directly linked with a nonzero (minimal) vacuum energy. Thus, a world of vibrating, spinning, interacting strings whose only elements in their construction are our topological concepts of space and time is envisioned, and they are proposed as tracers of the superfluid features of the space-time: the archetypal embodiment of these physical processes being set by the “gravitational roton”, an analogue of Landau’s classic higher-energy excitation used to explain the superfluid properties of helium II. The far and the near field asymptotics of string line solutions are presented and used to deduce their pair-interaction energy. Remarkably, it is found that two stationary, axis-aligned, quantum space-time vortices with the same sense of spin not only exhibit zones of repulsion but also of attraction, depending on their relative geodetic distance. 
 
</p></abstract><kwd-group><kwd>Modified Gravity; Superconductivity; Kinematics; Dynamics; Rotation</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Spiral patterns extending over a large portion of the stelar disk of many galaxies are seen everywhere in the cosmos. Thus, it may seem as if these majestic structures were stable features over a time of many orbital periods. Yet, current theory has a hard time to come up with a convincing explanation of their origin and stability. From the “coffee-cup” theory suggested by von Weizsaecker [<xref ref-type="bibr" rid="scirp.38879-ref1">1</xref>] to the spiral density wave theory of B. Lindblad [<xref ref-type="bibr" rid="scirp.38879-ref2">2</xref>], C.C. Lin, and F. Shu [3,4], it is fair to say, this basic problem of formation and stability of spiral galaxies is still not fully understood. In this article, this very crucial question is reversed, by imagining the sort of features a space-time needs to fulfill in order to explain this apparent stability as a pure gravitational phenomena, without invoking-a priori-the need of cold dark matter. More precisely, V. Rubin’s discovery (of an almost constant velocity flow of cool hydrogen clouds outside the bright parts of large spiral galaxies) is pictured here as an indication that the geometry along these special regions is rather uniform, the test orbiting bodies receive the same code of instructions, and the unexplained stiffness in the geometry is primarily due-according to the launched hypothesis-to a second order phase transition where the space-time acquires, at low curvatures, the properties of a superfluid. Basically, Weizsaecker’s “coffee-cup” analogy [<xref ref-type="bibr" rid="scirp.38879-ref1">1</xref>] is replaced by a “superfluid-cup” one, where phonons and rotons can flow, see <xref ref-type="fig" rid="fig1">Figure 1</xref>.</p><p>Can the geodesic motion of a radial alignment of test particles resist the winding process when the space-time is a superfluid [5,6]? How, in the first place, do quantum vortices behave if the space-time is a superfluid? In this article a research program is commenced by examining fully this second opening issue.</p><p>It should be stressed that the catalog of spiral galaxies is indeed vast: the so called grand design spirals have a well defined two-arm structure, but some others present multiple arms not necessarily symmetrical spaced, while there are others-referred to as flocculent spirals-showing sporadic spiral arm segments [<xref ref-type="bibr" rid="scirp.38879-ref5">5</xref>]; spiral patterns of a very</p><p>bizarre shape also show up in Nature: for instance, the spiral galaxy NGC4622 not only posses inner spiral arms that are trailing but also has a pair of outer arms that are leading, contrary to most expectations [<xref ref-type="bibr" rid="scirp.38879-ref7">7</xref>]. The oddest thing of all is that according to standard theory, if the material originally making up a spiral arm remains in the arm; then, the differential rotation of the galaxy will wind up the arm in a time short compare with the age of the galaxy. But most spiral arms (often logarithmic in nature) are far from being too tightly wound, with a pitch angle absolute value ranging from <img src="10-7501443\fe93dbba-9f41-41e9-b865-83cecd29bb45.jpg" /> to <img src="10-7501443\b3993592-c07e-43ec-bbf9-627d867745dc.jpg" /> [8-10]. How can this be?</p><p>This acute observation creates a fundamental challenge to theories on the origin of the spiral structure and it is referred to as “the winding dilemma” [<xref ref-type="bibr" rid="scirp.38879-ref11">11</xref>]. A description of this winding process, when there is an annular disk of material with a constant pattern speed-thus fulfilling the flat rotation curve criterion-is given in <xref ref-type="fig" rid="fig1">Figure 1</xref>.</p><p>At first sight, these bearings seem no different if one assumes that the orbiting objects are governed by Kepler’s laws of planetary motion or if they move with an approximately constant pattern speed; that is why, in the 1960s, an hypothesis was advanced: where the spiral features were assumed not only to be long lasting, but also that they were the result of a quasi-stationary density wave that rotated rigidly, at a slow paced rate, through the galactic disk-meaning in particular that stars should stream in and out of the spiral arms as they orbit the galaxy. This theory, however, has not been satisfactorily confirmed as even the question of longevity of the spiral arms, whether they are short-live transient patters (perhaps breaking apart and reforming periodically) or not has not yet been settled [12,13]. In Binney &amp; Tremaine comprehensive treatise on galaxy formation this peculiar situation is depicted as follows [<xref ref-type="bibr" rid="scirp.38879-ref5">5</xref>]:</p><p>“The common thread of several of these mechanism is that because of the swing amplifier, galactic disk respond with remarkable vigor to a wide variety of perturbations, whether these be tidal forces, gravitational instability of some local pattern of gas or stars, or fresh leading density waves. In some cases there is clear evidence that Lindblad’s original conception of the spiral arm as a density wave is correct. However, there is little or no direct evidence for the hypothesis that the spiral pattern is stationary (i.e. that it looks the same in 10<sup>9</sup> yr or so).”</p><p>Intriguingly, if the density wave theory were correct, a spatial ordering of different stages of star formation would be expected in the arms of galaxies: with very young objects on the leading edges of the arm (where star birth would be triggered by a compression wave) and the oldest ones on the trailing edge. However, research involving computer algorithms to examine twelve nearby spiral galaxies of different variety: such as the ‘whirlpool galaxy’ M51a, M63, M66, M74, and M95-an interacting, a flocculent, an arm-distorted, a grand design, and a barred spiral respectively-did not find such an ordering, leading to the conclusion that spiral density waves in their simplest form are not an important aspect of explaining spirals in large disk galaxies [<xref ref-type="bibr" rid="scirp.38879-ref14">14</xref>].</p><p>The purpose of this article is two fold:</p><p>Firstly: to get a deeper understanding of the physics of rotating astrophysical bodies in models where the spacetime exhibits non trivial macroscopic quantum effects.</p><p>Secondly: to deduce, in some quantitative way, part of the relevant signatures (topological traces) which might help to reveal whether or not such exotic behaviour is present in our universe.</p><p>Contents: the plan of the paper is as follows. The Euler-Lagrange equations for a quantum gravitational action are solve for vortexes and monopoles, in Section 4 and 6 respectively, exhibiting in full the superfluid properties of the space-time. The spin interaction of an array of axis-aligned quantum vortices is analysed in Section 5. Next, in Section 6.1, Dirac’s quantization condition is applied to quantize the size of the cosmological constant, which in the superconducting theory of gravitation plays a role analogous to an electric charge. Finally, the basic results are discussed and summarised in Section 9, where future directions for research are indicated.</p></sec><sec id="s2"><title>2. Space-Time as a Charged Superfluid</title><p>In the late 1930s, W. H. Kessom, P. Kapitza, J. F. Allen and A. D. Misener, initiated a series of low-temperature experiments that led to the discovery of superfluidity [15,16], a quantum many-body effect responsible of very striking properties in a superfluid, such as: an infinity heat conductivity, i.e. the boiling abruptly stops, a zero viscosity (superleaking with zero resistance), the fountain and mechanocaloric effects, to cite some appearing below a certain critical temperature (the <img src="10-7501443\b7bc5945-be41-4a02-bfb9-27bdb8f20f37.jpg" />- point for He II) and strictly at speeds under some critical velocity <img src="10-7501443\7b2e28c3-7302-4f89-9281-3c12217dac34.jpg" /></p><p>Is the space-time at galactic scales acting as a superfluid?</p><p>According to the prevailing view, at extragalactic scales the expanding universe is best think of as consisting of two parts: one luminous (obeying Newtonian mechanics in the limit of slowly moving bodies and large distances) and the other dark, or to use perhaps a better word: invisible (which is several times more abundant than the first one, and from which the formation and stability of the large scale structure of the universe presumably rests upon). For this second component, the quality of being invisible (or dark) is bring at front since it is only through its gravitational interaction with other bodies that this hypothetical form of matter (so far) has been accounted for.</p><p>In our view, the whole mystery of cold dark matter, and thus, the appearance of a two-fluid like model to describe the universe, where one component is behaving normally, while the other posses very odd properties, is a symptom of a bigger crisis than the one usually cured by just adding a new type of particle:</p><p>It is the failure of a proper understanding of how the quanta of mass-energy “there” rules inertia “here”. Indeed much is gained by flipping from the dark matter perspective into the realm of quantum gravitational phenomena, since there is now-as D. Hilbert could have put it, “a guide post on the mazy paths of hidden truths” for quantizing the gravitational field. “Quantum gravity is a very tough problem”-warned W. Pauli to B. S. De-Witt [17,18]. How are we going to unify “the strange world” of Max Born’s probability wave amplitudes <img src="10-7501443\c33d8895-bcc0-4621-8a6a-35e58c97aba0.jpg" />‘s with the peculiarities of the Einstein’s four-dimensional curved space-time continuum ?</p><p>Perhaps, as the dark mater conundrum seems to imply, we have various clues already:</p><p>There is an electrically neutral, QCD colourless, quasisubstance with local (or non-local) mass that is in a cold, stable (or long-lived) unexcited state far away of any strong field; it flows freely (without resistance) but only at non relativistic speeds-as if there were a limiting velocity that it cannot surpass, it has a negligible nongravitational interaction with ordinary baryonic matter or itself.</p><p>What could it be? To cope with the subtleties imposed by the above scenario let us turn to mathematics since as Max Born put it [<xref ref-type="bibr" rid="scirp.38879-ref19">19</xref>]: “When in conflict, mathematics— as often happens—is cleverer than interpretative thought.”</p></sec><sec id="s3"><title>3. Quantum Mathematical Model</title><p>In 1956 W. Pauli remarked [<xref ref-type="bibr" rid="scirp.38879-ref20">20</xref>]:</p><p>“The question of whether Kaluza’s formalism has any future in physics is thus leading to the more general unsolved main problem of accomplishing a synthesis between the general theory of relativity and quantum mechanics.”</p><p>A deep connection between Einstein’s law of gravity (with a nonzero cosmological constant) and quantum physical phenomena better associated to the theory of superconductivity was explored in [<xref ref-type="bibr" rid="scirp.38879-ref6">6</xref>], where the KaluzaKlein idea of splitting the space-time metric as:</p><disp-formula id="scirp.38879-formula20367"><label>(1)</label><graphic position="anchor" xlink:href="10-7501443\1192e70e-25ed-42ca-8ecd-a15061e5b7bf.jpg"  xlink:type="simple"/></disp-formula><p>and thus:</p><disp-formula id="scirp.38879-formula20368"><label>(2)</label><graphic position="anchor" xlink:href="10-7501443\24d64eba-8bf6-4575-aed8-76caf247c554.jpg"  xlink:type="simple"/></disp-formula><p>was adapted to offer a phenomenological, GinzburgLandau model of a 4-dimensional “quantum space-time”. <img src="10-7501443\b272c0b9-19d2-4a6c-a3a6-236975679e5a.jpg" />is the gravitomagnetic vector potential, <img src="10-7501443\3e0ab0a0-1e49-408e-8544-77d613f9596c.jpg" />is a scalar field, and <img src="10-7501443\b3918e22-bc4f-442e-8b9a-873d01eddb0c.jpg" /> is referred to as the 3-space base metric. The novelty of this approach is that although all the metric components are held real, <img src="10-7501443\5c29c63e-c44b-4816-8333-3d59b3c8ca05.jpg" />is set to be a complex scalar field:</p><disp-formula id="scirp.38879-formula20369"><label>(3)</label><graphic position="anchor" xlink:href="10-7501443\913d1717-cf1d-4bed-b0db-bb95e0b85394.jpg"  xlink:type="simple"/></disp-formula><p>characterising the onset of order of a phase transition affecting the intrinsic features of the space-time itself, which-at galactic scales, it is imagined developing the properties of a highly coherent quantum system in parallelism with superfluids, lasers, and superconductors. <img src="10-7501443\ca09f85b-d56c-4b13-8ef8-cded921f4a4d.jpg" />in other words, is a measure of symmetry violation. <img src="10-7501443\8fd9a61b-4471-45a0-b9a8-e1d6c9d22862.jpg" />will play the role of a Goldstone boson field.</p><p>Every direct comparison between this and the (traditional) ADM setting should always kept in mind the dual transformation:</p><disp-formula id="scirp.38879-formula20370"><label>(4)</label><graphic position="anchor" xlink:href="10-7501443\38b64cdb-2268-4c87-85df-d43bd5a97979.jpg"  xlink:type="simple"/></disp-formula><p>More comments on this very issue are given in [<xref ref-type="bibr" rid="scirp.38879-ref6">6</xref>].</p><p>In this article, Greek and Latin indices are employed to mark 4-dimensional and 3-dimensional tensors respectively (<img src="10-7501443\2d93ed71-70c1-4d18-882f-88ddb0313999.jpg" />;<img src="10-7501443\873002ce-520f-49c0-b5d0-16756a9e8445.jpg" />), as it is done in (2) and (4).</p><p>Key points of this bold proposal are briefly described next, leaving the details to the original article, where the theory was first developed [<xref ref-type="bibr" rid="scirp.38879-ref6">6</xref>]. First pay attention that by virtue of the complex nature of <img src="10-7501443\3b55bedc-af45-47f4-b984-795e91002956.jpg" /> the scheme by H. Weyl [21-24] to unite general relativity with electromagnetism can be adapted to treat the gravitomagnetic field <img src="10-7501443\12226775-7bf2-4bc7-9e45-a7aea039c1af.jpg" /> so that in theory, the primeval gauge transformations set by:</p><disp-formula id="scirp.38879-formula20371"><label>(5)</label><graphic position="anchor" xlink:href="10-7501443\2178591b-d75d-4e8c-85f0-a01662535075.jpg"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.38879-formula20372"><label>(6)</label><graphic position="anchor" xlink:href="10-7501443\a0f6c9b7-50a9-4658-8692-5330407e8969.jpg"  xlink:type="simple"/></disp-formula><p>become a symmetry of the physical gravitating system. Weyl’s original view of a 4-dimensional conformally invariant universe (described by a conformally invariant action where only purely real exponents get involved in the gauge transformation laws) was abandoned as a model for the actual state of the universe: for as much as the prediction that physical observables, such as the lengths and times of measuring rods and clocks, would depend of their prehistory, which would in turn introduce spectral blur effects which simply do not show up in reality [20,24]. Yet, gauge invariance (which has been very successful as guidance principle for formulating the electroweak and the strong nuclear interactions) can be incorporated into gravitation in another way [<xref ref-type="bibr" rid="scirp.38879-ref6">6</xref>] which seems more in unison with the principles of quantum mechanics.</p><p>As it is argue in pages to come, an utterly natural, Ginzburg-Landau-action principle for gravitation is:</p><disp-formula id="scirp.38879-formula20373"><label>(7)</label><graphic position="anchor" xlink:href="10-7501443\53a80d65-bb4e-4b54-9193-56ae128a8006.jpg"  xlink:type="simple"/></disp-formula><p>where the third term plainly depends on the Ricci scalar of the 3-space, base metric <img src="10-7501443\5ea62546-7c36-43b4-86df-a7b2406b184c.jpg" /> By keeping <img src="10-7501443\6dbdce13-4e42-4b9a-adb0-2964f80ce76f.jpg" /> fixed, the <img src="10-7501443\0d95074e-378a-4395-be66-490c3d22faaa.jpg" />-term becomes a constant multiplying the physical four-volume. Thus, <img src="10-7501443\1e565c0f-b9a1-49be-b108-76a74c6353dd.jpg" />can be identified with a vacuum energy, and <img src="10-7501443\4025e155-b672-4b38-b0e2-755aa14a9f88.jpg" /> must be proportional to the only constant present in the classical Einstein’s field equations which surely, is completely determined by the microphysics of the gravitating system, expressly, Einstein’s (1917) cosmological constant. The gravitomagnetic field-stress tensor is given by <img src="10-7501443\5ab26026-adea-48e1-aa69-5785b021c8b2.jpg" /> and attention should be brought to the curious sign in front of the <img src="10-7501443\a76c93b6-a369-4ff7-95e3-71351d67ad48.jpg" />-term (whose origin is traced back to the temporal nature of the fourth dimension).</p><p>Equation (7) is expected to be valid in stationary situations, where the temporal variations of the gravitomagnetic vector potential <img src="10-7501443\d2c11975-eb14-45ea-91f7-3d916fa78605.jpg" /> and the base metric <img src="10-7501443\667c8683-9531-4e44-8f13-bc3c818533d7.jpg" /> can be neglected [<xref ref-type="bibr" rid="scirp.38879-ref6">6</xref>]. It is exactly in this case when the parallelism between gravitation and a metallic super conductor looks more straightforward, after all, stationary space-times with horizons follow mechanical rules resembling the laws of thermodynamics [<xref ref-type="bibr" rid="scirp.38879-ref25">25</xref>]. In light of this, it can be stated that the infrared quantum macroscopic effects inherent to gravity seem best fitted by a word introduced by Kamerlingh Onnes in 1911, namely “superconductivity”.</p><p>Significant aspects of this action are immediately assessed by taking a look to the condensation energy: having both a sixth and inverse-square power terms, and depicted in <xref ref-type="fig" rid="fig2">Figure 2</xref>. Its shape is dictated by the Einstein-Hilbert action itself. Indeed, by varying <img src="10-7501443\2df0e275-44c4-4017-be27-98a534bd563f.jpg" /> and <img src="10-7501443\929fb1ef-98a9-43c5-8165-4d2bb2f159db.jpg" /> the least action principle (7) leads respectively to the energy and momentum constraint equations of Einstein’s theory of gravity, as it was developed by A. Lichnerowicz, J. W. York, and Y. Choquet-Bruhat in the 40s and 80s [26,27].</p><p>The mere existence of a phase in the ubiquitous complex gravitational potential introduced in (3) and (7) has the most amazing implications [<xref ref-type="bibr" rid="scirp.38879-ref6">6</xref>]:</p><p>Firstly: it allows the generation of supercurrents:</p><disp-formula id="scirp.38879-formula20374"><label>(8)</label><graphic position="anchor" xlink:href="10-7501443\23f854ba-8fae-4413-a0f5-8ab13eec8d19.jpg"  xlink:type="simple"/></disp-formula><p>transporting vacuum energy while deforming the gravitomagnetic (or gyrogravitational) lines of force. Be aware that closed strings are natural carriers of vacuum energy.</p><p>Secondly: second-order phase transitions controlled by</p><p>the curving of space can set in, subtlety raising the mass of the gravitomagnetic vector potential <img src="10-7501443\df498d7b-1295-4c6a-8ac9-a64b231c1c57.jpg" /> due to its interaction with an all-pervading gravitational degree of freedom [<xref ref-type="bibr" rid="scirp.38879-ref6">6</xref>]: expressly, the modulus of the complex potential<img src="10-7501443\5ad704cf-3969-4725-a9af-91839d879afe.jpg" />.</p><p>Thirdly: when a spinning point-like mass in empty space gets surrounded by supercurrents, the net effect is the generation of space-time superconducting zones, in which the associated rotation curves display non Keplerian features such as the ones exhibited in large spiral galaxies. Such rotations curves can be regarded as arising from the spontaneous breaking of <img src="10-7501443\ec96a60f-7c5f-4d97-a978-52e4d58a64e8.jpg" />-symmetry induced by the condensation of a Goldstone field coordinate <img src="10-7501443\3973a8d5-cc1a-4bb9-b86d-2253f03decc6.jpg" /> to an azimuthal angular value; thus, defining a preferred orbital direction of reference [see [<xref ref-type="bibr" rid="scirp.38879-ref6">6</xref>]].</p><p>Finally: at short distances, covering only a sufficiently small open neighbourhood of the space-time, when <img src="10-7501443\18d9eb37-83b3-4539-8ecf-53e9835a9e13.jpg" /> (and henceforth<img src="10-7501443\e2fcafe4-d44e-4f05-94eb-fa26e4e2836d.jpg" />) has not too much relevance, the predictions of Einstein’s theory of gravity are recovered. The same is truth if <img src="10-7501443\2c22e9df-6f95-4376-befb-0ab453ebbfe4.jpg" /> vanishes identically.</p><p>How does this work? Well, the string and monopole cases are provided below.</p><p>Notation and nomenclature—it is convenient to denote by <img src="10-7501443\14add8db-a165-4d78-aa5c-43b313775528.jpg" /> the value taken by the modulus of the complex field <img src="10-7501443\88fb27b1-b1bb-40e1-b658-6f192a24d917.jpg" /> under the peculiar situation when: <img src="10-7501443\dd74757c-d46f-4d43-b3b8-3e9261d56062.jpg" />at the minimum of the condensation potential. The identity:</p><disp-formula id="scirp.38879-formula20375"><label>(9)</label><graphic position="anchor" xlink:href="10-7501443\55519067-e279-47f1-9cfd-9b147af0ba6b.jpg"  xlink:type="simple"/></disp-formula><p>is then a direct consequence of this definition, see <xref ref-type="fig" rid="fig2">Figure 2</xref>. Direct inspection to (7) suggest that <img src="10-7501443\79ae0707-d6c7-4059-9bdc-35de22a6ab1e.jpg" /> is physically related to a measurable mass [<xref ref-type="bibr" rid="scirp.38879-ref6">6</xref>].</p><p>Write next</p><disp-formula id="scirp.38879-formula20376"><label>(10)</label><graphic position="anchor" xlink:href="10-7501443\270f94a0-24bf-4f54-8dc0-6566e059dfac.jpg"  xlink:type="simple"/></disp-formula><p>and set</p><disp-formula id="scirp.38879-formula20377"><label>(11)</label><graphic position="anchor" xlink:href="10-7501443\3dcfbc0f-c528-4dd0-b4e8-1fb3b391288f.jpg"  xlink:type="simple"/></disp-formula><p>also demanding that</p><disp-formula id="scirp.38879-formula20378"><label>(12)</label><graphic position="anchor" xlink:href="10-7501443\4352e17f-b731-468c-adb7-64f93753a281.jpg"  xlink:type="simple"/></disp-formula><p><img src="10-7501443\994fe41c-7cc3-418e-b6d5-d7ac88624efd.jpg" />is called the “London parameter” (or the penetration depth) and <img src="10-7501443\7114bc67-9895-4830-8320-1bf30a5ec688.jpg" /> is referred to as the “correlation length”.</p><p>The physical significance of all these expressions will be worked out with examples later.</p><p>Equations (11) and (12) give a dimensionless GinzburgLandau (G-L) parameter:</p><disp-formula id="scirp.38879-formula20379"><label>(13)</label><graphic position="anchor" xlink:href="10-7501443\fe8a1960-f203-4c4a-b92f-01bba082459d.jpg"  xlink:type="simple"/></disp-formula><p>equal to three halves, in line with type II super-conductivity. The (G-L) parameter, however, changes its value if one allows the <img src="10-7501443\0fc9bb37-dfe0-419e-961c-9dae81f207a4.jpg" />-term to be multiplied by a different coefficient than 12. This arbitrariness is discussed in more detail in [<xref ref-type="bibr" rid="scirp.38879-ref6">6</xref>]. A space-time fulfilling a principle of least action of the form given by (7) will be said to be a charged, space-time superfluid.</p><p>Space-time defects (mathematical preliminaries): Let the initial-data hypersurface <img src="10-7501443\d1a27ebe-3c31-4c0d-88db-60f14220e035.jpg" /> be a Riemannian space of constant sectional curvature; that is to say:</p><disp-formula id="scirp.38879-formula20380"><label>(14)</label><graphic position="anchor" xlink:href="10-7501443\8454cd56-3a42-4534-b6e4-3a98e649451f.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="10-7501443\46ddcc7a-8745-4282-b277-480be4948a82.jpg" /> is a given constant. Then, according to the theorem of H. Hopf and W. Killing [28,29], locally that space is isometric to one of the following models: a 3-sphere<img src="10-7501443\5157e434-1860-4fb3-95f9-7b236b8b8eae.jpg" />, a 3-Euclidean space<img src="10-7501443\07180965-1295-4b0c-bc09-0456b62c0515.jpg" />, or an hyperbolic 3-space<img src="10-7501443\fa60c39e-4b20-4ecf-9c53-5c37d56e16b1.jpg" />, with the same Ricci-scalar curvature <img src="10-7501443\93239aea-8de7-4064-b05a-42f79750c78e.jpg" /> Setting <img src="10-7501443\f69483f9-ae3c-4247-9f42-fbecfa3d62e6.jpg" /> as <img src="10-7501443\27d92467-c628-49d4-8637-fc576c60d7c0.jpg" /> appropriated line elements for the neighbourhood containing a given point <img src="10-7501443\d455a075-0179-43b6-ad73-241b5e5a9571.jpg" /> as origin are:</p><disp-formula id="scirp.38879-formula20381"><label>(15)</label><graphic position="anchor" xlink:href="10-7501443\544930fc-a897-4eef-9f10-9a00fa219ad5.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.38879-formula20382"><label>(16)</label><graphic position="anchor" xlink:href="10-7501443\228782f8-f6b9-4e68-97be-a8f7b795da70.jpg"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.38879-formula20383"><label>(17)</label><graphic position="anchor" xlink:href="10-7501443\e62d87d6-f719-47d9-8946-fe6041d48e1c.jpg"  xlink:type="simple"/></disp-formula><p>in the spherical, Euclidean, and hyperbolic instances respectively. By (17), the associated Laplace-Beltrami operator <img src="10-7501443\89f1add8-b43b-4065-826b-7bcbba28e92c.jpg" /> can be written as:</p><disp-formula id="scirp.38879-formula20384"><label>(18)</label><graphic position="anchor" xlink:href="10-7501443\4b10c691-e8f2-4200-9037-21da35c56b6f.jpg"  xlink:type="simple"/></disp-formula><p>Defining <img src="10-7501443\f3a7145a-cfb9-4485-9ab8-bd8bed376561.jpg" /> gives:</p><p><img src="10-7501443\d3fb6ba7-d648-41f6-a38c-1fde417cfabf.jpg" /></p><p><img src="10-7501443\0bfbb841-b4b9-48d5-9829-58d98219a96d.jpg" /></p><p>Since</p><p><img src="10-7501443\86aa91a0-ecf4-49aa-8d56-1ed0aacbeca2.jpg" /></p><p>the following identity must be satisfied:</p><disp-formula id="scirp.38879-formula20385"><label>(19)</label><graphic position="anchor" xlink:href="10-7501443\4932e8c9-2bc8-4dd6-8a8a-323828dd34ed.jpg"  xlink:type="simple"/></disp-formula><p>likewise,</p><disp-formula id="scirp.38879-formula20386"><label>(20)</label><graphic position="anchor" xlink:href="10-7501443\70eeb782-0607-40e3-8523-df7e48effc05.jpg"  xlink:type="simple"/></disp-formula><p>The nomenclature introduced in this passage as well as the pair set by (19) and (20), find an immediate application in the analysis of topological space-time defects, coming next.</p></sec><sec id="s4"><title>4. String Solution</title><p>The most basic features of the line defects predicted by the quantum rule set down by (7) are determined by the set of equations:</p><disp-formula id="scirp.38879-formula20387"><label>(21)</label><graphic position="anchor" xlink:href="10-7501443\344bea36-e09a-422f-a85a-a91cddeff93d.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.38879-formula20388"><label>(22)</label><graphic position="anchor" xlink:href="10-7501443\d03c959f-406c-4bfd-b481-c97d44d6a8aa.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="10-7501443\0da37125-4f6f-4daa-8ae1-395ad28a24ad.jpg" /> is a scalar field; <img src="10-7501443\07a208e3-5f58-47cb-bb16-de0b8eaa78d9.jpg" /><img src="10-7501443\37073131-8353-443e-a39f-b7dc9b3dc4fe.jpg" />and <img src="10-7501443\345c0b6d-c073-44d1-83b8-e54e84bbee83.jpg" /> are given by (9), (10), (11), and (12) respectively; <img src="10-7501443\45d57b1c-65b9-40ec-939c-71ce11364303.jpg" />is referred to as the gravitomagnetic field and it is given by <img src="10-7501443\1d0c68cc-af83-400f-ab25-224eaf23bdca.jpg" /></p><p>This can be found as follows. As in the previous paragraph, let <img src="10-7501443\76ffbbee-0ca8-49f7-9a91-97cc5a59fe7c.jpg" /> be a Riemannian space of constant sectional curvature. Let <img src="10-7501443\84625602-f4ec-46ef-abc7-3ae090539195.jpg" /> i.e. allow the curvature radius of the universe be large enough. Then, by (20), at leading order it must be true that</p><p><img src="10-7501443\4d85eaa6-219c-4eac-9754-b38fcc66a306.jpg" /></p><p>and similarly with other expressions having the divergence, the gradient, and so on-as it is intuitive from (15) and (17). Thus, it is seen that there exists a convenient way to promote various calculations in flat space to curve space. Following this simplifying lead, make the subsequent choices. Employing cylindrical coordinates, write <img src="10-7501443\c7e8d9c4-4ac3-40cb-81db-e42344515c9c.jpg" /> as <img src="10-7501443\5fb5f8e4-6944-4507-9ba5-2710d529a8bf.jpg" /> Then, in the corresponding orthonormal frame, the gradient of <img src="10-7501443\4147926b-7c40-49fe-9aa9-4ea2f6aaa8ff.jpg" /> and the curl of <img src="10-7501443\e0663886-3934-40bf-b35d-cd93b307aa33.jpg" /> (or any other vector field) have respectively the form:</p><disp-formula id="scirp.38879-formula20389"><label>(23)</label><graphic position="anchor" xlink:href="10-7501443\95090d1c-aae2-4e86-8f4b-726fd56fa5c1.jpg"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.38879-formula20390"><label>(24)</label><graphic position="anchor" xlink:href="10-7501443\df06920f-c6d6-4296-8757-7fa36d14cc1c.jpg"  xlink:type="simple"/></disp-formula><p>Assuming that not far away from the axis of symmetry, here symbolized by the z-axis, the “probability-like” current density:</p><disp-formula id="scirp.38879-formula20391"><label>(25)</label><graphic position="anchor" xlink:href="10-7501443\27bd45f5-6b74-46bd-9506-6a01d7f40fe1.jpg"  xlink:type="simple"/></disp-formula><p>girdles always in the azimuthal direction, and moreover, that its magnitude at any given point <img src="10-7501443\922ee67b-917a-46e2-8ca1-aad9a4064c80.jpg" /> proximate to the centre line only depends on its geodesic distance to such line, let <img src="10-7501443\48660eeb-aaf5-4421-bf9e-bb88e3a3be08.jpg" /> take the form:</p><disp-formula id="scirp.38879-formula20392"><label>(26)</label><graphic position="anchor" xlink:href="10-7501443\784a9c13-d6bb-41b0-aa5e-98e3556b1c6d.jpg"  xlink:type="simple"/></disp-formula><p>These restrictions immediately imply:</p><disp-formula id="scirp.38879-formula20393"><label>(27)</label><graphic position="anchor" xlink:href="10-7501443\64668ca6-4eac-427a-a54b-9e5e8dfce9e7.jpg"  xlink:type="simple"/></disp-formula><p>and henceforth:</p><disp-formula id="scirp.38879-formula20394"><label>(28)</label><graphic position="anchor" xlink:href="10-7501443\d9d98071-7cf2-4159-b235-5f38a9525846.jpg"  xlink:type="simple"/></disp-formula><p>Additionally, if only the radial part of the modulus field <img src="10-7501443\8b336efb-39bb-42ff-adf1-bdec875527ff.jpg" /> is considered [see (3)], Combining (10) and (11) with the Euler-Lagrange equation:</p><disp-formula id="scirp.38879-formula20395"><label>(29)</label><graphic position="anchor" xlink:href="10-7501443\7f4784fe-a76a-42f3-8305-9b531e189a97.jpg"  xlink:type="simple"/></disp-formula><p>resulting from the variation <img src="10-7501443\6f6b9eeb-46b5-43db-a59d-7801cfac9961.jpg" /> in the action principle set by (7), a differential relationship between the two unknown functions: <img src="10-7501443\03baded9-26dc-403c-94eb-85e063005959.jpg" />and <img src="10-7501443\e28c89df-f61f-4cba-a790-8d1f5e329604.jpg" /> follows immediately:</p><disp-formula id="scirp.38879-formula20396"><label>(30)</label><graphic position="anchor" xlink:href="10-7501443\92b4dc54-626c-4618-b560-a73e562bdd26.jpg"  xlink:type="simple"/></disp-formula><p>By letting further, the order parameter <img src="10-7501443\91198bf1-8df2-4f0e-8287-1a7144a1a107.jpg" /> to be a function of <img src="10-7501443\f6f654bc-341f-4df4-97b5-a5757c93e94d.jpg" /> only, the Lichnerowicz equation, obtained by the <img src="10-7501443\17a5a114-0cae-4ca0-82f7-04b000ceb995.jpg" />-variation of the Ginzburg-Landau action set by (7), becomes at leading order [using (12) and (20)]:</p><disp-formula id="scirp.38879-formula20397"><label>(31)</label><graphic position="anchor" xlink:href="10-7501443\e9d91b91-a5c9-4f84-9ad5-ee6636f812e7.jpg"  xlink:type="simple"/></disp-formula><p>completing the system, where the relation: <img src="10-7501443\31c00ab1-9b90-477a-a78e-8f79e46e2acf.jpg" />entailing the gravitomagnetic field <img src="10-7501443\92810bdb-b276-435f-819d-ddb49807f1e0.jpg" /> has been used.</p><sec id="s4_1"><title>4.1. Asymptotic Analysis near the String Axis</title><p>The action principle set by (7) implies the following:</p><p>Firstly: the vortex-gravitomagnetic flux is quantized.</p><p>Secondly: the minimal flux <img src="10-7501443\d87112ae-9f9a-4276-904c-ca92bd4fdf6f.jpg" /> is achieved by some regular <img src="10-7501443\659eaaae-ca9c-4fe1-84be-eeb135a80678.jpg" />-vortex profile. Thirdly: the order <img src="10-7501443\374d90ee-f1a6-41cc-93cb-ce7e9c084997.jpg" />- parameter for such a vortex of minimal vorticity vanishes in a linear fashion, along cylindrical ring-like structures of nonzero finite radius. Fourhtly: near the vortex core, the asymptotic metrical aspects of the quantum, regular vortex of minimal vorticity are determined (say at the initial time<img src="10-7501443\735ad073-68eb-46b7-95b9-f101822531b6.jpg" />) by</p><p><img src="10-7501443\d04af68b-ad35-4087-8311-dc5a62af7dba.jpg" /></p><p><img src="10-7501443\1b88003a-45bf-409b-9a81-6c6f391481a5.jpg" />is here the intensity of the gravitomagnetic field along the flux tube and it is assumed to be nonzero. Finally but not least-by (58), a natural way to express the fitting “charge” <img src="10-7501443\fb7d34d6-f11a-4f2e-9fa8-107e37f870ce.jpg" />is in the form <img src="10-7501443\fde219ae-0f7b-4598-9f26-999b2bd17ca1.jpg" /> where <img src="10-7501443\9efe1e8d-1264-48fb-8254-62a969b94411.jpg" /> is Planck’s constant <img src="10-7501443\606f64d4-7e58-4cf7-9f4c-faf66147e527.jpg" /> joule-seconds, meaning that <img src="10-7501443\25709f72-50d8-4a75-9bd2-6c2da31086ba.jpg" /> can be regarded as introducing an <img src="10-7501443\3ac4d5a9-ff86-4a6c-8207-44f86ce5ea3f.jpg" /> factor into the main gravitational equations.</p><p>Proof: For the sake of argument, ignore first the A-ρ coupling in (21). Then, at sufficiently close distance from the axis of symmetry, when</p><p><img src="10-7501443\6dbc92ef-0b6c-4292-842b-f88a869675a4.jpg" /></p><p>and <img src="10-7501443\15261595-4963-42b8-8829-214bb1ce4a47.jpg" /> (21) implies:</p><disp-formula id="scirp.38879-formula20398"><label>(32)</label><graphic position="anchor" xlink:href="10-7501443\3aa0f388-eb79-4885-a36a-277b076ac284.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="10-7501443\2b9c36f1-86af-4229-afe9-6cc9fc3e11b2.jpg" /> and <img src="10-7501443\98f45c54-22d5-457f-9126-caf7bc72b14c.jpg" /> are integration constants. Inserting (32) into (27) shows that the <img src="10-7501443\bebb1d52-589f-4b18-be17-b304a27af4dc.jpg" />-constant physically gives the intensity of the gravitomagnetic field <img src="10-7501443\e9c05ea6-67c5-4084-8f0b-58d002e19a74.jpg" /> along the <img src="10-7501443\b227b9e7-4202-40fe-8333-85cf114dc752.jpg" />-axis, i.e.</p><disp-formula id="scirp.38879-formula20399"><label>(33)</label><graphic position="anchor" xlink:href="10-7501443\cda62f4e-4d2a-4eef-a48c-7ccdde69a35a.jpg"  xlink:type="simple"/></disp-formula><p>Setting</p><disp-formula id="scirp.38879-formula20400"><label>(34)</label><graphic position="anchor" xlink:href="10-7501443\7361dca7-e8ca-464d-886e-e7bbeaa39425.jpg"  xlink:type="simple"/></disp-formula><p>(22) reads, in the limit imposed by (32), as</p><disp-formula id="scirp.38879-formula20401"><label>(35)</label><graphic position="anchor" xlink:href="10-7501443\d3755f0b-44e4-49f5-802e-218744f226ba.jpg"  xlink:type="simple"/></disp-formula><p>Equation (35) is reminiscent of the Bessel differential equation; however, it contains the non-linear <img src="10-7501443\f228e94a-2bed-40ae-a64b-57984c380b53.jpg" />-factor, multiplying <img src="10-7501443\5988592f-ca3c-4f35-84ce-4648eac93d15.jpg" /> and spoiling an all-encompassing similarity. To solve (35), follow these simple steps:</p><p>Firstly: verify the expression below is an exact, regular solution.</p><disp-formula id="scirp.38879-formula20402"><label>(36)</label><graphic position="anchor" xlink:href="10-7501443\c1c027d5-0460-4e46-b3cc-5bdc62c6fafa.jpg"  xlink:type="simple"/></disp-formula><p>Secondly: spot that clearly another regular asymptotic answer is given by:</p><disp-formula id="scirp.38879-formula20403"><label>(37)</label><graphic position="anchor" xlink:href="10-7501443\3465e8c2-beb6-487a-ae78-13adcaff7f95.jpg"  xlink:type="simple"/></disp-formula><p>whenever <img src="10-7501443\a0f4d72d-46d1-477b-8985-ee5f4f81ae46.jpg" /> What about the distinctive <img src="10-7501443\a5d72d0b-d598-44e2-a074-e9f3c8e3849f.jpg" /> value? Well, several transformations simplify the problem.</p><p>Last step: as suggested by (36) and (37), pick</p><disp-formula id="scirp.38879-formula20404"><label>(38)</label><graphic position="anchor" xlink:href="10-7501443\e8011d9d-4802-4e66-b458-8af4d7c62f69.jpg"  xlink:type="simple"/></disp-formula><p>and set <img src="10-7501443\267b7213-4ecd-421a-8b20-f62ffcf859c8.jpg" /> Then, (35) reduces to</p><disp-formula id="scirp.38879-formula20405"><label>(39)</label><graphic position="anchor" xlink:href="10-7501443\76e461f6-c0ac-407f-a3d8-5e11315cad05.jpg"  xlink:type="simple"/></disp-formula><p>which is symmetric under the specular transformation: <img src="10-7501443\f3de8144-641c-4a29-9e6c-241ba84efa1b.jpg" />By the change of variables: <img src="10-7501443\4543e436-10ee-47ff-81be-529342552b4a.jpg" />it transforms into</p><disp-formula id="scirp.38879-formula20406"><label>(40)</label><graphic position="anchor" xlink:href="10-7501443\6a78f262-236b-467f-8233-a7abf23558ae.jpg"  xlink:type="simple"/></disp-formula><p>complying with the canonical form of the so-called Emdem-Fowler (E-F) equation:</p><disp-formula id="scirp.38879-formula20407"><label>(41)</label><graphic position="anchor" xlink:href="10-7501443\a673d050-a4b7-42d0-9908-f8eafaba59cf.jpg"  xlink:type="simple"/></disp-formula><p>If <img src="10-7501443\0fabc889-e82e-440a-98c8-5ad002440769.jpg" /> the E-F equation has the exact solution:</p><disp-formula id="scirp.38879-formula20408"><label>(42)</label><graphic position="anchor" xlink:href="10-7501443\85a9d333-3efb-48d3-86dc-005cb5ed244a.jpg"  xlink:type="simple"/></disp-formula><p>as it is readily verified. Unfortunately <img src="10-7501443\9ad4ea33-3d92-4afe-b3bb-ac06fc2e38a8.jpg" /> and <img src="10-7501443\50b48ad6-dc1f-4d41-b4ab-aaf26bb3c52b.jpg" /> thus no formal solution can be extracted from this previous knowledge, as the coefficient multiplying <img src="10-7501443\4231ba37-6008-4a50-a2a9-d83a6057cf1d.jpg" /> diverges. To advance further, introduce the change of variable <img src="10-7501443\0855733b-6730-4c74-ad25-8c1be3178a3a.jpg" /> then, (40) becomes instead:</p><disp-formula id="scirp.38879-formula20409"><label>(43)</label><graphic position="anchor" xlink:href="10-7501443\5151633d-cfcf-4dcd-ae10-d361e8e0ad10.jpg"  xlink:type="simple"/></disp-formula><p>which has coefficients which do not depend explicitly on the independent <img src="10-7501443\7c07e1dc-7a53-436a-8a1c-e897cad9a0d0.jpg" />-variable. A standard trick is then to pick <img src="10-7501443\50d74473-ccae-480f-83cb-2811b184b883.jpg" /> hence <img src="10-7501443\225869d5-b0be-4b26-9bf9-ef8d6e5cf83f.jpg" /> and (43) simplifies to:</p><disp-formula id="scirp.38879-formula20410"><label>(44)</label><graphic position="anchor" xlink:href="10-7501443\647b583e-31eb-4f23-8742-2aa0700f2b29.jpg"  xlink:type="simple"/></disp-formula><p>which is intended to be solved for <img src="10-7501443\3a8127e7-cfd0-4f36-99d7-24b43c351960.jpg" /> Thus, proceeding in the reverse order, <img src="10-7501443\026b57e8-e0ec-4204-af8c-5437a4c0fa91.jpg" />is obtained by inverting (if possible)</p><disp-formula id="scirp.38879-formula20411"><label>(45)</label><graphic position="anchor" xlink:href="10-7501443\e31f54fb-8b3c-4a09-9980-052f623ced93.jpg"  xlink:type="simple"/></disp-formula><p>The general features of the solutions, <img src="10-7501443\df7e9f9b-0477-4ddd-8f99-11de9eff2e85.jpg" />of (44) are depicted in the phase diagram: <img src="10-7501443\c6cb3d6e-8047-4553-b883-1225af21c0b0.jpg" />versus <img src="10-7501443\55761d6d-71e6-4061-a712-d000eee6f369.jpg" /> in <xref ref-type="fig" rid="fig3">Figure 3</xref>. The vertical axis not only gives a measure of the magnitude of <img src="10-7501443\a7628c38-906d-459f-8aff-292c2559a19f.jpg" /> but also of <img src="10-7501443\85ced9ef-db5c-4317-a046-7e89bb91d1cb.jpg" /> as can be seen by the chain of relations <img src="10-7501443\40df4de7-52d9-4698-9a60-4a9757ee8e7d.jpg" /> Thus, the locus of points of the form <img src="10-7501443\64909253-3460-4d1e-9c05-d54cb2ab8a8d.jpg" /> where, as a function of<img src="10-7501443\ca85e6f1-cd72-4bbf-a370-894993e6417f.jpg" />, <img src="10-7501443\dd661125-145c-4580-a7f8-a6c84beabb34.jpg" />is an extremum are mapped into the horizontal axis <img src="10-7501443\9deb4939-16aa-4676-8199-32776a09a6ae.jpg" /> of <xref ref-type="fig" rid="fig3">Figure 3</xref>; the points set by <img src="10-7501443\32b7e0a7-171b-4167-aea0-964fb12ab5e8.jpg" /> where, as a function of <img src="10-7501443\ff161e61-f962-4bfb-9de6-bf40f8f4a6cf.jpg" /> <img src="10-7501443\ee9aaf0b-bdcb-4472-8f34-8254428c992d.jpg" /> is an extremum falls over the dotted curve <img src="10-7501443\9d556c75-4b8c-4262-a763-23f2b25278f5.jpg" /> labeled by the <img src="10-7501443\6d59b088-ba06-4983-a4a1-b77a8556f276.jpg" /> latin symbol in <xref ref-type="fig" rid="fig3">Figure 3</xref> Use next (44) to obtain</p><disp-formula id="scirp.38879-formula20412"><label>(46)</label><graphic position="anchor" xlink:href="10-7501443\9fd4c949-aed4-42a7-866f-fdcbf4644d49.jpg"  xlink:type="simple"/></disp-formula><p>The superior (and by the same note, inferior) branch of the “inflexion curve”:</p><disp-formula id="scirp.38879-formula20413"><label>(47)</label><graphic position="anchor" xlink:href="10-7501443\86cbdf8c-9ca8-40b9-9bb1-6820dc402d91.jpg"  xlink:type="simple"/></disp-formula><p>drew from (46) by the condition <img src="10-7501443\e4e103ee-9a80-41d5-8837-6ae093d2b965.jpg" /> is labeled <img src="10-7501443\c413fba8-31ec-4b9d-86b9-a1b87578c93e.jpg" /> (jointly<img src="10-7501443\9eeb5aec-bb32-42a1-895d-c97011986965.jpg" />) in <xref ref-type="fig" rid="fig3">Figure 3</xref>. The solutions <img src="10-7501443\a53268ed-4d9c-45c7-88aa-9b857ee68572.jpg" /> can be separated into two distinct classes, referred to as type I and type II for definiteness. A representative of each class has been found numerically and depicted in the same figure: type-I solutions do not cross the <img src="10-7501443\e0d36c16-9364-4fde-836a-f7899350d0e4.jpg" /> <img src="10-7501443\10fcbd82-ff04-4782-a994-421ad0a18d62.jpg" />-axis,</p><p>type-II make that cross. Let <img src="10-7501443\1e2a78d8-735d-49f5-8d4d-a94f9f50a545.jpg" /> be a type-I solution, clearly <img src="10-7501443\b9fe6685-cfb1-4d5a-8165-f7d69a1ac566.jpg" /> is bounded from below by some positive constant, lets say<img src="10-7501443\47eb0a4a-1cd2-41cf-8eec-025681320efb.jpg" />. By (44), as <img src="10-7501443\a7d78e4e-77a8-4171-ad06-0cfcb65fe92c.jpg" /> approach infinity, <img src="10-7501443\bc3bca86-57e9-4f99-927a-4d35a0170847.jpg" />tends to 1. This means that <img src="10-7501443\550f9599-2641-4dab-a45d-4d6847e486ce.jpg" /> takes the asymptotic form</p><p><img src="10-7501443\d929f180-dbe2-4034-ba40-07071ffb681e.jpg" />as<img src="10-7501443\7aff3085-a31c-46ef-81df-111810bf04c2.jpg" />where <img src="10-7501443\f10dad32-f688-404f-ba93-1f9cc9531790.jpg" /> is a point in <img src="10-7501443\19e73d41-09ec-4adb-8e0b-15153a0d84a3.jpg" /> Therefore, according to (45) one has</p><disp-formula id="scirp.38879-formula20414"><label>(48)</label><graphic position="anchor" xlink:href="10-7501443\8f16909b-4b70-489a-a928-c960b0b9df43.jpg"  xlink:type="simple"/></disp-formula><p>as <img src="10-7501443\baa85f16-ce31-491d-b85d-83224dfb1d5d.jpg" /> Meaning, by inverting the relation, that</p><disp-formula id="scirp.38879-formula20415"><label>(49)</label><graphic position="anchor" xlink:href="10-7501443\12611f73-417c-4e5b-ba43-e6ff1f91901b.jpg"  xlink:type="simple"/></disp-formula><p>The important point to make is that this is not a regular solution, since</p><p><img src="10-7501443\038d5ba4-bc7a-4329-ac1d-fc546066b717.jpg" /></p><p>is obviously different from zero. Turning now to type-II solutions, consider the situation when one has both: <img src="10-7501443\83242df3-8773-4882-8c18-485224db55ce.jpg" />and <img src="10-7501443\348512e9-2af3-4f19-a014-f25be268c846.jpg" /></p><p>Applying l’H&#244;pital’s rule to (44), it is established that in this regime:</p><disp-formula id="scirp.38879-formula20416"><label>(50)</label><graphic position="anchor" xlink:href="10-7501443\ce09ac58-ee95-4e09-ba51-de0e80d64159.jpg"  xlink:type="simple"/></disp-formula><p>which gives</p><disp-formula id="scirp.38879-formula20417"><label>(51)</label><graphic position="anchor" xlink:href="10-7501443\cf81f2d5-7e1b-4414-b833-7eca33ffe001.jpg"  xlink:type="simple"/></disp-formula><p>Thus <img src="10-7501443\bd28df7b-0aee-4586-abb9-13c6f6386ed7.jpg" /> and henceforth</p><p><img src="10-7501443\72bb7482-967c-4f46-bb6d-21c2b64c5471.jpg" /></p><p>Inserting such an expression in (45), the following asymptotic formulae for the <img src="10-7501443\2a835665-8e3f-4b08-a414-b1057c42fd1d.jpg" />-field are obtained, from which some characteristics observed on <xref ref-type="fig" rid="fig4">Figure 4</xref> are deduced:</p><p><img src="10-7501443\95997e86-bb04-45b6-9ad3-330704aeea9d.jpg" /><img src="10-7501443\7d0664da-a25b-4a9b-8d27-a47a553d130f.jpg" /> (52)</p><disp-formula id="scirp.38879-formula20418"><label>(53)</label><graphic position="anchor" xlink:href="10-7501443\12e22d30-18e2-4d18-9290-d86cbb4d6b14.jpg"  xlink:type="simple"/></disp-formula><p>Let</p><p><img src="10-7501443\77264b8b-4cbf-4c99-8e74-120bf5133096.jpg" /></p><p>and insert the (53) result into (21), it gives a linear non homogeneous equation whose general solution for <img src="10-7501443\5b4687ef-6968-481e-8a3d-a91b34c53189.jpg" /> is the sum of a particular solution, say <img src="10-7501443\676cdb96-52c5-41e6-934e-8bf214866b1f.jpg" /> to the solution of the homogeneous problem given by (32) again, choosing a particular solution satisfying the initial conditions: <img src="10-7501443\a6a5de29-a444-4b52-ad07-bf00b0c660e9.jpg" />at <img src="10-7501443\b1cae0ca-877f-424b-8273-c429613f3e44.jpg" /> (where <img src="10-7501443\9433d399-dcba-4ea5-9a0b-57ac18382bf5.jpg" /> is the value of the coordinate radius at some point of the permitted interval), it is seen then that the non particular solution can only bring quadratic <img src="10-7501443\1355af39-c116-4c78-a054-72c35766e89c.jpg" />-corrections to the previous answer. The <img src="10-7501443\3f56350f-f16b-4a7b-9589-ded59dab5d9e.jpg" /> term in (32) still dominates the limiting behaviour at small radii. Thus, if</p><disp-formula id="scirp.38879-formula20419"><label>(54)</label><graphic position="anchor" xlink:href="10-7501443\af677bab-eba7-4a5e-9ea9-53362462c65c.jpg"  xlink:type="simple"/></disp-formula><p>it is consistent to set</p><disp-formula id="scirp.38879-formula20420"><label>(55)</label><graphic position="anchor" xlink:href="10-7501443\9eb4f501-59da-4a05-b052-af58da62fbdd.jpg"  xlink:type="simple"/></disp-formula><p>and also</p><disp-formula id="scirp.38879-formula20421"><label>(56)</label><graphic position="anchor" xlink:href="10-7501443\b3933eb8-8ae4-4090-9bd1-8e827fad0353.jpg"  xlink:type="simple"/></disp-formula><p>Yet, the Friedmann-Lema&#238;tre-Robertson-Walker-like scale factor introduced in the Kaluza-Klein-like metric (1), that is to say, the <img src="10-7501443\66490b01-f643-4396-92a1-211e36dea5ec.jpg" /> piece, must be a single-valued function. Not having any restriction on the polar angle <img src="10-7501443\3fd0abb1-9270-4c32-9cb7-f94a742d898d.jpg" /> it must be true, if <img src="10-7501443\9855c565-94f0-4283-ac74-eda8d2bb32cc.jpg" /> that</p><disp-formula id="scirp.38879-formula20422"><label>(57)</label><graphic position="anchor" xlink:href="10-7501443\526ff7f8-ce62-4bcc-9587-a7651d4e55b5.jpg"  xlink:type="simple"/></disp-formula><p>implying in turn a quantum law over the allowed values for the gravitomagnetic flux, namely</p><disp-formula id="scirp.38879-formula20423"><label>(58)</label><graphic position="anchor" xlink:href="10-7501443\e8bcab32-6913-4e46-b882-9ecd1b587d0c.jpg"  xlink:type="simple"/></disp-formula><p>in the understanding that <img src="10-7501443\f7b70b94-694f-4f4a-9601-e31d1c11f0e0.jpg" /> is a planar, smooth, closed curve of winding number one, surrounding the axis of symmetry; each point of <img src="10-7501443\ee0b9689-1441-4163-8630-dd0e2a0ba9a8.jpg" /> it is assumed also, falls deep inside a large enough zone where the space-time becomes superconducting, and thus where <img src="10-7501443\bf660fff-edfa-45fd-a801-330b87189841.jpg" /> vanishes identically. This type of flux quantization has exactly the same form than in metallic superconductors, where the carriers of electric current consist of pairs of electrons. A pair of charged quantum fields <img src="10-7501443\5c8ff8cd-704d-4be8-9a27-329c957e4c6d.jpg" /> actually a field coupled to itself, appears instead in the line element (1) from which the action principle (7) is based on. Here, the fitting charge, however, is in essence pure vacuum energy.</p><p>The law of gravitation (7) outlines the Bose-Einstein condensation of wave-particle pairs and it bring us closer to some of the most fundamental queries posed by Newton about the origin gravity [30,31]:</p><p>“I have not been able to discover the cause of those properties of gravity from phenomena, and I frame no hypotheses; for whatever is not deduced from the phenomena is to be called a hypothesis, and hypotheses, whether metaphysical or physical, whether of occult qualities or mechanical, have no place in experimental philosophy.”—Principia 2nd edition.</p><p>“Is not this &#198;thereal Medium much rarer within the dense Bodies of the Sun, Stars, Planets and Comets, than in empty celestial Spaces between them? And in passing from them to great distances, doth it not grow denser and denser perpetually, and thereby cause gravity of those great Bodies toward one another, and of their parts towards the Bodies; every Body endeavouring to go from the denser parts of the Medium towards the rarer?” — Opticks Query 21.</p><p>In what proportion is the intensity of what we call Gravity affected by an increase in mass of the gyromagnetic field which, by a Higgs-like mechanism, gets transformed as we move further and further away from macroscopic dense Bodies like the Sun, Stars, Planets and Comets? Is the local spherical radius on the verge of becoming rather uniform so that orbiting test bodies like Stars at different radii move through paths of almost equal length? And how this rigidity (or uniformity) of the space distorts a beam of light when it departs from a point where gravity is normal, then—as it travels—the gyrogravitational field becomes massive, to finally end at another point where the spacetime is not superconducting? Is this a step forward towards a consisitent solution to the stabilization problem of spiral galaxies?</p></sec><sec id="s4_2"><title>4.2. Far Away Asymptotics</title><p>A regular, infinite, string line, obeys the asymptotic formulae provided below if the conditions <img src="10-7501443\4c8f5ce7-a33e-48b3-9aa6-f9fb0fd48b57.jpg" /> and <img src="10-7501443\1c38e697-8132-4c97-aabd-415cb7d50e49.jpg" /> are met:</p><disp-formula id="scirp.38879-formula20424"><label>(59)</label><graphic position="anchor" xlink:href="10-7501443\1bac722a-4f31-4101-afc0-5192cef29e84.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.38879-formula20425"><label>(60)</label><graphic position="anchor" xlink:href="10-7501443\3f3c0199-e81d-4068-8047-f2cd47c66d2e.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="10-7501443\643c5ef6-8934-4748-ac73-b28443b44cc6.jpg" /> is the Macdonald function, decaying with distance at leading order as</p><p><img src="10-7501443\b386cf0d-d84a-4ab2-b95d-c43a373b325d.jpg" /></p><p>To look for the asymptotic distance decay of the gravitational <img src="10-7501443\f3a2db45-5743-4585-8740-d7ef882ea181.jpg" />-potential, turn back to the basic system of cylindrically symmetric equations:</p><p><img src="10-7501443\5f29e566-ba37-428f-bd40-5d60295a9144.jpg" />(61)</p><disp-formula id="scirp.38879-formula20426"><label>(62)</label><graphic position="anchor" xlink:href="10-7501443\c339dfe2-0262-4161-96b5-67a32d0c5b0c.jpg"  xlink:type="simple"/></disp-formula><p>As the gravitomagnetic vector potential becomes pure gauge, as the space-time becomes superconducting, the <img src="10-7501443\ab9c02c5-50aa-44d6-918e-478463a35efa.jpg" />-field becomes, to a high degree of accuracy, given by an asymptotic expansion of the form:</p><disp-formula id="scirp.38879-formula20427"><label>(63)</label><graphic position="anchor" xlink:href="10-7501443\a9e74a62-cc04-4a8d-9b86-3c946f538b6d.jpg"  xlink:type="simple"/></disp-formula><p>the system (61) and (62), in the limit<img src="10-7501443\82b3923a-bc5c-4c15-b2e3-5f1449e11c92.jpg" />, <img src="10-7501443\814d6d33-4fd2-4ec9-80be-3f47f07879d7.jpg" />simplifies to:</p><disp-formula id="scirp.38879-formula20428"><label>(64)</label><graphic position="anchor" xlink:href="10-7501443\7f275b3e-929d-4329-b159-65a35137ecf8.jpg"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.38879-formula20429"><label>(65)</label><graphic position="anchor" xlink:href="10-7501443\f5e88f8e-14f2-4387-b1f7-03028fe3d14d.jpg"  xlink:type="simple"/></disp-formula><p>Put attention that the <img src="10-7501443\a2e2ca18-35d0-4461-ac83-77e202b2d9e0.jpg" /> coupling implied by (61) is relevant only at second order and be alert on the dissimilarity in sign between the coefficient accompanying our correlation length <img src="10-7501443\b9a848f2-d94c-4585-8faa-7ebef4ffa9f6.jpg" /> and the one encountered in standard superconductivity: our sign, one may say, is anomalous. Nevertheless, this does not seem to represent a severe problem; on the contrary, it is necessary to display some of the features observed for the shape of the galactic rotation curves, as it is argued in [<xref ref-type="bibr" rid="scirp.38879-ref6">6</xref>]. (64) is just the modified Bessel equation:</p><disp-formula id="scirp.38879-formula20430"><label>(66)</label><graphic position="anchor" xlink:href="10-7501443\388ed399-ee53-4058-830e-ecab5b8828ad.jpg"  xlink:type="simple"/></disp-formula><p>and it has as one of its solutions: the Macdonald function <img src="10-7501443\a15d1dd8-b85d-4600-8b63-34b40d5cc5c8.jpg" /> decaying exponentially to zero according to the asymptotic representation [<xref ref-type="bibr" rid="scirp.38879-ref32">32</xref>]:</p><disp-formula id="scirp.38879-formula20431"><label>(67)</label><graphic position="anchor" xlink:href="10-7501443\d160c3bc-bd69-4ff9-bc32-6270b9f265fc.jpg"  xlink:type="simple"/></disp-formula><p>One discards the other independent solution, the hyperbolic Bessel function of the first kind <img src="10-7501443\5ae186de-7a58-4125-9d81-2f116f8f9774.jpg" /> since it grows exponentially with <img src="10-7501443\5c88869f-9afd-4570-80c2-3d3547182238.jpg" /> giving an apposite effect not in line with (63), unless <img src="10-7501443\bfed5eca-9c52-43b6-8fd3-53c811f166db.jpg" /> be unbounded. In the next section a rough estimate of the vortex-vortex interaction energy is obtained with the help of some identities satisfied by the Macdonald function, which for convenience’s sake are listed here: namely, its divergent behaviour at the origin:</p><p><img src="10-7501443\ee37d42a-8b0b-45af-b1de-26f6adf9283a.jpg" /></p><disp-formula id="scirp.38879-formula20432"><label>(68)</label><graphic position="anchor" xlink:href="10-7501443\e9f12f78-552a-47ee-8048-65f2c3dd3107.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="10-7501443\f768f9c6-4647-45ff-a428-21cbc56192fe.jpg" /> is the Euler-Mascaroni constant, approximately given by</p><p><img src="10-7501443\1799cb46-1a40-466b-b093-ee7f76d6fe5f.jpg" /></p><p>and the differential identities:</p><disp-formula id="scirp.38879-formula20433"><label>(69)</label><graphic position="anchor" xlink:href="10-7501443\527edb19-8758-4013-93d1-f9e9ee6c0ed5.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.38879-formula20434"><label>(70)</label><graphic position="anchor" xlink:href="10-7501443\f4bd7226-cde7-4f4f-b260-30f1038ff65b.jpg"  xlink:type="simple"/></disp-formula><p>In the same train of thought, (65) is just the Bessel o.d.e:</p><disp-formula id="scirp.38879-formula20435"><label>(71)</label><graphic position="anchor" xlink:href="10-7501443\b9cd6b34-ea84-452c-9444-995aec14f5b0.jpg"  xlink:type="simple"/></disp-formula><p>which has as solutions the cylindrical harmonics <img src="10-7501443\b5be9d4a-9b20-4bae-8c24-ada50f009b2f.jpg" /> and <img src="10-7501443\5044a4bf-1d35-49ed-89d5-c4195b883f79.jpg" /> An asymptotic representation of them for large real arguments is given respectively by</p><disp-formula id="scirp.38879-formula20436"><label>(72)</label><graphic position="anchor" xlink:href="10-7501443\d86a6892-117c-4b37-aa28-006347c5f685.jpg"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.38879-formula20437"><label>(73)</label><graphic position="anchor" xlink:href="10-7501443\f8255e90-4fb8-4495-bad9-42bc68a0762c.jpg"  xlink:type="simple"/></disp-formula><p>if <img src="10-7501443\c1cff514-768b-479b-beb6-ca871daa2609.jpg" /> Their distance decay is thus oscillatory and modulated, in part by the two-dimensional nature of the problem, by an inverse square root power of the separation distance from the source. Nonetheless at short radii:</p><disp-formula id="scirp.38879-formula20438"><label>(74)</label><graphic position="anchor" xlink:href="10-7501443\496abb3a-31a5-402d-a5cb-3996d7515995.jpg"  xlink:type="simple"/></disp-formula><p>holds.</p><p>Now, consider the Green’s identity:</p><disp-formula id="scirp.38879-formula20439"><label>(75)</label><graphic position="anchor" xlink:href="10-7501443\e5941a73-55ec-49b1-87e9-ac90b5398848.jpg"  xlink:type="simple"/></disp-formula><p>over the contour <img src="10-7501443\0d5743d5-6401-4b24-9770-067259ecce1d.jpg" /> depicted in <xref ref-type="fig" rid="fig5">Figure 5</xref>, letting <img src="10-7501443\80f77c06-241e-4c88-92f4-013988c32d0c.jpg" /> be a regular function on<img src="10-7501443\47680678-5700-43d5-965d-a073ea9ade9a.jpg" />—we already know, by (68), that <img src="10-7501443\7fb2c596-fa3c-49bc-b856-6cda0ff3573a.jpg" /> is indeed regular there. Adding and subtracting <img src="10-7501443\c558f86c-d7ce-4b01-8996-5506e45bae89.jpg" /> to the integrand on left hand side of (75), and using (66), we get:</p><disp-formula id="scirp.38879-formula20440"><label>(76)</label><graphic position="anchor" xlink:href="10-7501443\d46dc8a5-92d3-4801-afc9-0d441e938787.jpg"  xlink:type="simple"/></disp-formula><p>But the right-hand side of (75) is the sum of two contour integrals: one along the circle of very large radius <img src="10-7501443\fd9e9e37-9ecf-44b7-9756-cd0acec7b8d2.jpg" /> where the asymptotic representation of (67) applies, and the other along the circle of small radius <img src="10-7501443\70af5c33-13b6-48d2-b694-756caca3b04a.jpg" /> where (68) holds asymptotically. Therefore, taking the limit <img src="10-7501443\1ae20e3c-3cf9-48d3-8ef7-59be9ec9d0a4.jpg" /> gives</p><disp-formula id="scirp.38879-formula20441"><label>(77)</label><graphic position="anchor" xlink:href="10-7501443\563f1163-ebc8-4695-928f-96e65cca23a4.jpg"  xlink:type="simple"/></disp-formula><p>on the assumption that not only</p><p><img src="10-7501443\be74b07e-09e1-4453-ad6e-b068265a743e.jpg" /></p><p>is bounded from above <img src="10-7501443\a7b81bdd-ee63-4b85-8b4b-5415d7e06d16.jpg" /> outside a disk <img src="10-7501443\2637c4cc-f125-4dbf-93c3-15f6b226dfa1.jpg" /> of sufficiently large radius, but also that</p><disp-formula id="scirp.38879-formula20442"><label>(78)</label><graphic position="anchor" xlink:href="10-7501443\96fa3e43-967c-4abe-b7b6-2b736eecfe0e.jpg"  xlink:type="simple"/></disp-formula><p>Following Laurent Schwartz’s theory of distributions, a linear map</p><p><img src="10-7501443\e10a1d18-87d1-41ae-99cd-0e5f44d1f911.jpg" /></p><p>from a proper space of test functions <img src="10-7501443\6e94dfd3-7b9c-42b2-a63d-a9a56ae0dd19.jpg" /> to the reals can then be defined with the help of (77), symbolically written as:</p><disp-formula id="scirp.38879-formula20443"><label>(79)</label><graphic position="anchor" xlink:href="10-7501443\5b02a28e-4c75-4298-8b07-c0057b5cd109.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="10-7501443\4ffcfb73-5c36-4d97-a714-880a54d58cd8.jpg" /> is Dirac’s delta distribution with support at the polar origin. Likewise (73) and (74) leads to</p><disp-formula id="scirp.38879-formula20444"><label>(80)</label><graphic position="anchor" xlink:href="10-7501443\5a1355ff-c953-41bd-a037-3d80a0cf5cbe.jpg"  xlink:type="simple"/></disp-formula><p>Be aware, however, that as the natural space of test functions <img src="10-7501443\d015faa7-a8be-4b86-b065-89d31d45eefc.jpg" /> should be in tune with the vanishing hypothesis of boundary terms in the far field regime, in more diverse applications, stronger assumptions than the ones required for making sense of (79) must apply (if needed, a change of measure under which the given integrals are carried out, say by adding proper weighting factors becomes a natural way to follow). Proceeding on such grounds it must be true, by (66) and (67), that</p><disp-formula id="scirp.38879-formula20445"><label>(81)</label><graphic position="anchor" xlink:href="10-7501443\9144c25d-dc0e-4132-9eae-40745c6ef3bd.jpg"  xlink:type="simple"/></disp-formula><p>which by (27), (69), and (79), immediately gives</p><disp-formula id="scirp.38879-formula20446"><label>(82)</label><graphic position="anchor" xlink:href="10-7501443\fa2b5345-fe96-41f6-a814-21a5fe87182d.jpg"  xlink:type="simple"/></disp-formula><p>The minus sign appearing at the end of this expression is expected. Combining (72) and (73), we get</p><disp-formula id="scirp.38879-formula20447"><label>(83)</label><graphic position="anchor" xlink:href="10-7501443\9cd4efd1-4caa-4dd4-b886-6f4f3d6d0709.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="10-7501443\8cda7031-9016-4148-868a-1c59dddb0106.jpg" /> (determining the first order of the perturbation amplitude) and <img src="10-7501443\71ae1f60-5068-4ff6-9bb9-d9afe36e313e.jpg" /> (the angular phase) are integration constants. An immediate application of (59) and (60) is the estimation of the vortex-vortex and vortex-antivortex interaction energies.</p></sec></sec><sec id="s5"><title>5. Spin Interaction</title><p>Imagine a large pattern of quantum, space-time vortices: each vortex labelled by a unique number <img src="10-7501443\c29d8ef1-2563-4e4f-bd9c-079d761b0078.jpg" /> whose axes are all aligned, as depicted in <xref ref-type="fig" rid="fig6">Figure 6</xref>. Let the Lagrangian of the system be given by:</p><disp-formula id="scirp.38879-formula20448"><label>(84)</label><graphic position="anchor" xlink:href="10-7501443\2a51f498-16bf-4ef8-8d5f-0415e26a08f4.jpg"  xlink:type="simple"/></disp-formula><p><img src="10-7501443\196efb20-e7b0-4c3e-b76f-af4bd2448734.jpg" />denoting the free Lagrangian:<img src="10-7501443\6e3c83aa-e93c-422d-9821-a63db6854395.jpg" />, approximately given by a sum over disjoint regions of space <img src="10-7501443\127d427f-5485-4708-8be9-610a26e921bb.jpg" /> (hereafter referred to as terminals or ends) of compact support centred at each space-time quantum vortex: each vortex treated at leading order as if it were in complete isolation, plus a remainder; that is to say:</p><disp-formula id="scirp.38879-formula20449"><label>(85)</label><graphic position="anchor" xlink:href="10-7501443\b4ffdeaf-8f8e-4299-a862-5829d4e82147.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="10-7501443\8c18fa42-6108-40de-945c-387f1c868aa9.jpg" /> is given by (7). To a good degree of accuracy, two stationary, axis-aligned, quantum space-time vortices with the same sense of spin, interact with an interaction energy given by:</p><disp-formula id="scirp.38879-formula20450"><label>(86)</label><graphic position="anchor" xlink:href="10-7501443\2086af51-e797-4038-928f-0cd88c61858e.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="10-7501443\852b2e78-80bb-4cdf-85e8-ecc4db506640.jpg" /> is their relative geodetic distance (according to the rest frame of reference attached to the strings themselves) and <img src="10-7501443\e0c0b00e-e517-44a7-aa11-2b8bfcdee4e9.jpg" /> is a cylindrical harmonic which decays with distance as</p><p><img src="10-7501443\d5642905-1c90-4f95-b485-e966c993c577.jpg" /></p><p>To first order of approximation, the form of the extra piece in square brackets <img src="10-7501443\aac34b77-739d-41b0-99d7-6dc73cfe34a4.jpg" /> is dictated by the requirement that the perturbative motion, say of the umpteenth vortex of the pack, roughly described by the triplet</p><p><img src="10-7501443\457a17d2-6e42-4be2-a9c1-ae62bc0452b9.jpg" /></p><p>be given by the solution for an isolated vortex</p><p><img src="10-7501443\25250aef-a806-4076-9f09-abac98216395.jpg" /></p><p>plus a correction term <img src="10-7501443\68330f41-aa96-4268-9f07-8755233f6e6a.jpg" /> satisfying:</p><disp-formula id="scirp.38879-formula20451"><label>(87)</label><graphic position="anchor" xlink:href="10-7501443\99d1e3ae-866a-4c62-ae8e-dbec9b3ae41c.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.38879-formula20452"><label>(88)</label><graphic position="anchor" xlink:href="10-7501443\6b67ec97-3779-48db-b7d4-4daba8262cd7.jpg"  xlink:type="simple"/></disp-formula><p>where</p><p><img src="10-7501443\c2d5ca12-cc2e-4341-919d-c2a8c96bfeac.jpg" /></p><p>whereas <img src="10-7501443\c722a6d6-08c6-4bd2-ad34-e5768e29b514.jpg" /> and <img src="10-7501443\a8d8cd54-a7c9-4db8-84a9-bf6fb72cd06d.jpg" /> are source terms, one for each vortex of the bundle. Compare these equations with (64) and (65). The first entry in the superscript <img src="10-7501443\053fb573-4d51-44de-b435-1551253106c5.jpg" /> of <img src="10-7501443\1ee9e7fc-80cd-45fb-8858-4073e1d1c290.jpg" /> and <img src="10-7501443\0d1f441a-1403-4cc8-886a-4053131fb551.jpg" /> labels the vortex to which it is referred to, while the second entry (as well as the (0) in<img src="10-7501443\1cc4ef37-dc69-4ffb-8f0d-c98db1f50be0.jpg" />) establishes the degree of the perturbation.</p><p>In view of this, set</p><disp-formula id="scirp.38879-formula20453"><label>(89)</label><graphic position="anchor" xlink:href="10-7501443\4c5409a3-0e18-4ca7-ab69-c83f3b1b453a.jpg"  xlink:type="simple"/></disp-formula><p>where the sum spans over all the vortex singularities; the equations of motion then become:</p><disp-formula id="scirp.38879-formula20454"><label>(90)</label><graphic position="anchor" xlink:href="10-7501443\d695b583-8d5d-4ae1-b24f-d37b18f45d71.jpg"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.38879-formula20455"><label>(91)</label><graphic position="anchor" xlink:href="10-7501443\a52d6747-8e57-44d5-ab9c-9c678b211039.jpg"  xlink:type="simple"/></disp-formula><p>Next, assume that in the neighbourhood <img src="10-7501443\062476b1-29da-4064-bf3a-0599cc0f86d4.jpg" /> of the <img src="10-7501443\244fe196-7f89-47fa-bf24-1bccf96b01ee.jpg" />-th vortex of the sample, the asymptotic conditions:</p><disp-formula id="scirp.38879-formula20456"><label>(92)</label><graphic position="anchor" xlink:href="10-7501443\169f5cfb-cb12-4804-b2e4-808bea63ead9.jpg"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.38879-formula20457"><label>(93)</label><graphic position="anchor" xlink:href="10-7501443\73841779-8dda-4a8f-aa25-4ccadfbfc049.jpg"  xlink:type="simple"/></disp-formula><p>hold. Here <img src="10-7501443\63eb9271-1ca1-49e0-9f71-8487ff98c3f9.jpg" /> is the unit vector on the zero-order space-time background, surrounding the j-th vortex and pointing along the associated azimuthal direction. Solve then (90) and (91) perturbatively. At zero order, one gets the system of equations studied previously: (21) and (22). Up to second order terms one recovers the system given by (87) and (88), as requested. To compute the firstorder-correction terms of the <img src="10-7501443\380199c7-6aff-4112-8928-3101c27b8cf5.jpg" />-vortex solution, <img src="10-7501443\e70fb50f-1a4a-4ed7-a8af-0c5a9d307404.jpg" />and <img src="10-7501443\29ef365c-2754-43a2-a13d-0aaa44c7b908.jpg" /> suppose they are the direct result of an external field obtained by linear superposing each of the zeroorder fields, as seen from a long distance, of the remaining <img src="10-7501443\c4bb7485-433b-40c4-8437-2126702e716b.jpg" /> vortices; this can be done by setting:</p><disp-formula id="scirp.38879-formula20458"><label>(94)</label><graphic position="anchor" xlink:href="10-7501443\70648105-4f47-403e-88d9-fae13af016bd.jpg"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.38879-formula20459"><label>(95)</label><graphic position="anchor" xlink:href="10-7501443\e5f5ca43-e617-4083-bb62-9d034fa4fb62.jpg"  xlink:type="simple"/></disp-formula><p>since one must have both</p><p><img src="10-7501443\b21ace4f-43a9-416d-920b-f9fa1f629122.jpg" /></p><p>and (60) holding simultaneously, see (69), whereas the exact coefficients in front of the delta distribution and its distributional derivative are a direct consequence of (79) and (80). Henceforth, in the neighbourhood of the <img src="10-7501443\2cd6e4c6-89c7-424d-9433-3dae902a1246.jpg" />- vortex, the increment in energy <img src="10-7501443\cf8fe8ed-382d-4618-a557-22a7ef12f19d.jpg" /> due to the external field produced by an axis-aligned <img src="10-7501443\b0cbe44d-f0d3-4883-9b89-e82297b27479.jpg" />-vortex moving with the same sense of rotation is given by:</p><disp-formula id="scirp.38879-formula20460"><label>(96)</label><graphic position="anchor" xlink:href="10-7501443\dec5a229-ff5a-4244-a3fa-9ec22d93ec00.jpg"  xlink:type="simple"/></disp-formula><p>To a good degree of approximation <img src="10-7501443\2ca682ab-b412-4185-bef2-d427ce154c51.jpg" /> using</p><p><img src="10-7501443\0bc47d56-a5d2-4c71-a451-a3d97505a97e.jpg" /></p><p>and</p><p><img src="10-7501443\c6f310bc-7cc0-42ab-b910-30914c3af175.jpg" /></p><p>reduces to</p><disp-formula id="scirp.38879-formula20461"><label>(97)</label><graphic position="anchor" xlink:href="10-7501443\707229f7-ac70-4d00-bc74-567d984c5a7b.jpg"  xlink:type="simple"/></disp-formula><p>Here <img src="10-7501443\7c04ef68-39fe-4662-9947-3f7232e49e1b.jpg" /> gives the location of the <img src="10-7501443\7b695f3b-9a9f-4a0a-a558-54baa314d738.jpg" />-vortex; the denominator of the first term of (96) is evaluated using <img src="10-7501443\eeb4d33a-bd08-455d-8019-4ee9ccc46772.jpg" /> For small <img src="10-7501443\4f290b61-9188-4d49-9c83-2a35cff79cdb.jpg" /> the typical shape of this static potential is depicted in <xref ref-type="fig" rid="fig7">Figure 7</xref>; the first term, by (67), gives a repulsive contribution; the second term, in comparison with the first one, induces in virtue of (73) an attraction at some places, but gives a strong repulsion at others quarters, leading to an spectrum of local stationary minima roughly separated by a distance of order <img src="10-7501443\bab57981-843f-454a-82ae-9e88575d29ca.jpg" /> A variety of interesting solitonic phenomena may arise from (86), perhaps leading to voids where no vortices are</p><p>expected. Finally, the complete increment in energy, say <img src="10-7501443\83dde1ec-d624-4f1b-9f62-7d7aa9f7cb4a.jpg" /> associated with the external fields <img src="10-7501443\f82ae406-1721-4316-8b3a-3bcf3f77bf32.jpg" /> and <img src="10-7501443\7bbc41c0-1533-4874-97d5-cd3f49d69fa3.jpg" /> acting on the <img src="10-7501443\4551b969-cabd-4509-b02a-43d4daae3f49.jpg" />-vortex is obtained by summing over all the interacting energies, giving:</p><disp-formula id="scirp.38879-formula20462"><label>(98)</label><graphic position="anchor" xlink:href="10-7501443\0039b8d0-486d-4ef9-ac0a-c612972c6e01.jpg"  xlink:type="simple"/></disp-formula><p>In generic situations one may expect to lose some of the finer details resulting from second term of (86), leading to a net repulsive force.</p></sec><sec id="s6"><title>6. Monopole Solution</title><p>Ever since its inception in 1861, Maxwell’s equations raised a mystery that is still with us. While they seem to emphasize a complete symmetry between the phenomena of electricity and magnetism, only in the vacuum the alleged harmony is known to exist: as particles carrying a single magnetic charge (the magnetic analogue of the electron) so far have not been found [<xref ref-type="bibr" rid="scirp.38879-ref33">33</xref>]. Yet Poincar&#233;, J. J. Thomson, O. Heavyside, and P. Curie contemplated the idea of an exact symmetry at least once [<xref ref-type="bibr" rid="scirp.38879-ref34">34</xref>]. In the years of 1931 and 1948, a consistent quantum theory of magnetic monopoles was put forward by Dirac [35,36], who arrived to a very significant conclusion; namely, that if monopoles (or just one monopole) exist, this would amount of an explanation of why electricity is quantized and given in exact multiples of some smallest charge. Dirac’s own initial conviction on the existence of the monopole is succinctly expressed in this famous 1931 statement ([<xref ref-type="bibr" rid="scirp.38879-ref35">35</xref>], p. 71): “Under these circumstance one would be surprised if Nature had made no used of it.”</p><p>Contrariwise, Bohr was and remained very skeptical of this whole affair [<xref ref-type="bibr" rid="scirp.38879-ref34">34</xref>]. The monopole theory in fact did not seem to generate much interest until 1974, when it was discovered, by Gerard ‘t Hooft and Alexander M.</p><p>Polyakov [37,38] independently, that monopoles are an inevitably prediction of certain Grand Unified Theories (GUT’s) which rely on the spontaneous breakdown of symmetry. Namely, those in which the electromagnetic group <img src="10-7501443\3b8739c7-c54f-493f-84f2-ca2a91156562.jpg" /> is taken to be a subgroup of a larger group with a compact covering group, like <img src="10-7501443\496a8a04-5595-43b6-9d2a-ca9bb4b5adb7.jpg" /> which contains the standard model:</p><disp-formula id="scirp.38879-formula20463"><label>(99)</label><graphic position="anchor" xlink:href="10-7501443\904fe264-30ba-476e-b616-326e756d9cf4.jpg"  xlink:type="simple"/></disp-formula><p>The GUT monopoles are exceedingly massive, with a mass, say<img src="10-7501443\7ad2d435-42d0-47a1-8ff6-b0959b8cc911.jpg" />, larger by an inverse square gauge coupling constant than a typical vector boson mass:</p><p><img src="10-7501443\bccc0bff-0134-46cf-a1cb-6d170442d977.jpg" />, <img src="10-7501443\005f4bbc-0cbf-4ec2-9b86-718b12131b43.jpg" /></p><p>They would act as catalysers for the proton decay predicted by grand unified theories [39,40], and would be produced in copious number at the very early stages of the universe. Being highly stable particles, the GUT monopoles would survive as relics to the present epoch. But in order to not enter into conflict with what is observed, it would be necessary that their density be diluted considerable by some unknown mechanism (say inflation) during the cosmic evolution [<xref ref-type="bibr" rid="scirp.38879-ref41">41</xref>]. It is also known that in the so-called Prasad-Sommerfield limit some of these non abelian monopoles can be converted by their mutual interaction into dyons [42,43]: hypothetical particles carrying both electric and magnetic type charges that were first proposed in 1969 by J. Schwinger.</p><p>Be that as it may, even if no monopole has been found yet, it brings considerable insight regarding the foundations of physics.</p><p>The action principle (7) not only leads to the existence of a gyrogravitational Meissner-Ochsenfeld effect, one of the most fundamental properties expected to arise for a model where the space-time acts like a superconducting body, but also indicates that the cosmological constant, first introduced to gravitation by Einstein in 1917, is not only quantized but also that its square root is given in exact multiples of some smallest value.</p><p>To see if this is true, adopt an orthonormal, spherical, coordinate grid of reference outlined by the triplet <img src="10-7501443\d212162e-36d4-429d-b7fb-719049ed1048.jpg" /> defined by radial, zenith-angular, and azimuthal-angular variables respectively. The gradient of <img src="10-7501443\4809b142-83d9-456b-ae20-dc12e321f780.jpg" /> in the corresponding orthonormal frame, is given then by</p><p><img src="10-7501443\fa837b41-2993-49d1-a059-d34e5a8820d9.jpg" /></p><p>while the curl of any vector field, say <img src="10-7501443\78ff793d-83cd-4969-9f36-9cbb284b7786.jpg" /> for definiteness, assumes the form:</p><disp-formula id="scirp.38879-formula20464"><label>(100)</label><graphic position="anchor" xlink:href="10-7501443\a7a7cc11-3ec5-4187-bb01-5b0feed483ab.jpg"  xlink:type="simple"/></disp-formula><p>Suppose only one component (the azimuthal one ) of the density current (25) is nonzero, and moreover, that it does not depend on the azimuthal <img src="10-7501443\98db80d2-d222-4602-a4eb-b3bb23d5e837.jpg" />-variable; the problem reduces then to the evaluation of an scalar potential:</p><disp-formula id="scirp.38879-formula20465"><label>(101)</label><graphic position="anchor" xlink:href="10-7501443\c9127dcd-1bd6-4386-83ed-c7086cb544fa.jpg"  xlink:type="simple"/></disp-formula><p>taking values on the real line and having poles or singularities, so that the divergence of the gravitomagnetic field be different from zero, as depicted in <xref ref-type="fig" rid="fig8">Figure 8</xref>. By (100) and the working hypothesis</p><disp-formula id="scirp.38879-formula20466"><label>(102)</label><graphic position="anchor" xlink:href="10-7501443\dcf1ac44-0377-4e5b-a38d-9e27e62936ef.jpg"  xlink:type="simple"/></disp-formula><p>it is deduced that:</p><disp-formula id="scirp.38879-formula20467"><label>(103)</label><graphic position="anchor" xlink:href="10-7501443\9fbfaf04-2dc3-4a3e-a3a6-7c287379a7f9.jpg"  xlink:type="simple"/></disp-formula><p>Consequently, the curl of the gravitomagnetic field is</p><disp-formula id="scirp.38879-formula20468"><label>(104)</label><graphic position="anchor" xlink:href="10-7501443\ab26b1e1-57d5-4634-a6ea-db1a38db6930.jpg"  xlink:type="simple"/></disp-formula><p>and (29) immediately reduces to:</p><disp-formula id="scirp.38879-formula20469"><label>(105)</label><graphic position="anchor" xlink:href="10-7501443\d04592fc-4db2-4bdc-8fe8-d94580030a0c.jpg"  xlink:type="simple"/></disp-formula><p>Assuming:</p><disp-formula id="scirp.38879-formula20470"><label>(106)</label><graphic position="anchor" xlink:href="10-7501443\e8e50979-a47d-4b4d-af54-583cfb2efcdf.jpg"  xlink:type="simple"/></disp-formula><p>apply the method of separation of variables by letting the <img src="10-7501443\ad96dbcd-61c5-4ccf-a471-37fc55b3fa44.jpg" />-function to be given in terms of radial and angular eigenfunctions, <img src="10-7501443\1d1991be-e491-43c7-8b9e-dd3f7f37cb1f.jpg" />and <img src="10-7501443\7e5ba9d3-1ec2-4877-91d2-705ce7e1999e.jpg" /> satisfying respectively:</p><p><img src="10-7501443\2e9552e8-0009-47a9-bf16-88fc2d40e11b.jpg" />(107)</p><p>and</p><p><img src="10-7501443\fa74923a-f263-4b6b-adfb-10e3f2681f8e.jpg" />(108)</p><p>For now let <img src="10-7501443\ea6e2349-bf47-4137-9cb5-f7d71917b49d.jpg" /> be a function of <img src="10-7501443\bf6a69a8-1b95-4227-9498-c00cd97d0387.jpg" /> only. Then, by setting <img src="10-7501443\4b1731b4-4263-49d1-97e7-41dbf7dc9862.jpg" /> and making the change of variable: <img src="10-7501443\58e7dcf5-878a-4428-8806-2fa7606b7e7e.jpg" />(108) in turn translates into the form:</p><disp-formula id="scirp.38879-formula20471"><label>(109)</label><graphic position="anchor" xlink:href="10-7501443\44829ec6-a36a-4624-8961-180f72d09051.jpg"  xlink:type="simple"/></disp-formula><p>Thus, if <img src="10-7501443\656743be-6c06-4e4d-9e4a-ae9bf158adff.jpg" /> is the polynomial series</p><disp-formula id="scirp.38879-formula20472"><label>(110)</label><graphic position="anchor" xlink:href="10-7501443\648d4eda-f45a-4d23-89fb-f79a7f248f9b.jpg"  xlink:type="simple"/></disp-formula><p>its coefficients <img src="10-7501443\7755f0e1-5898-4797-8ec0-583e1aade065.jpg" /> must satisfied the recurrence relation:</p><disp-formula id="scirp.38879-formula20473"><label>(111)</label><graphic position="anchor" xlink:href="10-7501443\d95b969b-1391-422c-8edb-f81b4cdd0e9a.jpg"  xlink:type="simple"/></disp-formula><p>furthermore, since</p><disp-formula id="scirp.38879-formula20474"><label>(112)</label><graphic position="anchor" xlink:href="10-7501443\2d08ee86-c670-4c74-90cc-3b54cad26b2f.jpg"  xlink:type="simple"/></disp-formula><p>it is deduced that <img src="10-7501443\f6745b37-a5bf-43e8-a185-7b0462db92d1.jpg" /> has a finite number of terms whenever <img src="10-7501443\6b4586b9-ead5-4365-bec3-adb3cbf3fd46.jpg" /> becomes an integer. The<img src="10-7501443\f215eca2-7d24-40a6-9e80-e1df4d5617df.jpg" />’s are in fact a limiting case of the so called Jacobi polynomials, denoted by <img src="10-7501443\b95b83c7-4415-4daf-aaf0-ac9f00e3c2e9.jpg" /> where one assumes that <img src="10-7501443\8b75ddbd-eda3-4161-a4b3-9237d21099a4.jpg" /> and <img src="10-7501443\fce1ed91-d1fd-4962-bd6d-6bab21790675.jpg" /> are bigger than minus one, that is:</p><disp-formula id="scirp.38879-formula20475"><label>(113)</label><graphic position="anchor" xlink:href="10-7501443\383a27e3-ddaa-4808-8fc3-4f7e9d6efaf6.jpg"  xlink:type="simple"/></disp-formula><p>The<img src="10-7501443\df44f6a6-aa82-46c7-a1ba-c4531935557d.jpg" />’s fulfils the Rodrigue’s formula:</p><disp-formula id="scirp.38879-formula20476"><label>(114)</label><graphic position="anchor" xlink:href="10-7501443\eb077031-592b-45d3-9999-578d89b507c7.jpg"  xlink:type="simple"/></disp-formula><p>They are connected with the Gegenbauer polynomials also through the relation:</p><disp-formula id="scirp.38879-formula20477"><label>(115)</label><graphic position="anchor" xlink:href="10-7501443\28ceb029-538a-476e-9c70-e401666c5e36.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.38879-formula20478"><label>(116)</label><graphic position="anchor" xlink:href="10-7501443\7e6e84c3-82dd-4db4-a8b1-40c096f70435.jpg"  xlink:type="simple"/></disp-formula><p>A small set of angular functions <img src="10-7501443\b93fb8cf-824d-4311-ace1-b72d1fd5fb7b.jpg" /> obtained by the repeated application of the recurrence relation (111) or directly through the Rodrigue’s formula (114), is given bellow:</p><disp-formula id="scirp.38879-formula20479"><label>(117)</label><graphic position="anchor" xlink:href="10-7501443\a38efb2b-fa5b-439b-92d8-e943816ea59a.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.38879-formula20480"><label>(118)</label><graphic position="anchor" xlink:href="10-7501443\355ac528-e207-47fc-865f-482bf491c605.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.38879-formula20481"><label>(119)</label><graphic position="anchor" xlink:href="10-7501443\a0d10dc1-ebd5-482d-820f-bac98d2bf21a.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.38879-formula20482"><label>(120)</label><graphic position="anchor" xlink:href="10-7501443\23311f3f-5165-4389-a60b-7e4fe50afe04.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.38879-formula20483"><label>(121)</label><graphic position="anchor" xlink:href="10-7501443\09b903ae-08e7-4b9b-866f-703366ae6a67.jpg"  xlink:type="simple"/></disp-formula><p><img src="10-7501443\79be1f24-d287-460a-8787-e884ade6a0a1.jpg" />(122)</p><p><img src="10-7501443\99c91fcb-42cf-4304-881f-4c353516b973.jpg" />(123)</p><p>and so on. The zero eigenvalue is degenerate and an arbitrary linear combination of the corresponding eigenfunctions is presented in (117). In general, they not lead to (weighted) squared integrable functions, inasmuch as the integral:</p><disp-formula id="scirp.38879-formula20484"><label>(124)</label><graphic position="anchor" xlink:href="10-7501443\7bbc7ed8-3855-489c-836d-65e7d3d7890c.jpg"  xlink:type="simple"/></disp-formula><p>is divergent for the <img src="10-7501443\d6c3a1bc-3c5a-43e0-8815-4ba830f77ba0.jpg" /> and <img src="10-7501443\ec901db8-4b17-4905-81b9-9986aac22a91.jpg" /> cases. The rest, however, satisfy the identity</p><p><img src="10-7501443\cb320dde-b1f8-4d74-93f2-7fdeeda1a882.jpg" />(125)</p><p>having finite limits at the north and south poles. In fact,</p><p><img src="10-7501443\7d95e7da-2c94-4af1-a0ba-6b28ef5d048a.jpg" /></p><p>if <img src="10-7501443\f945f7ff-0226-45a6-8a22-71a76e1d4654.jpg" /> By an appropriated choice of parameters (117) can be made regular, either at the north or the south pole, but not both! Regularity at the north pole (when<img src="10-7501443\c34bc739-4872-4309-b645-ee9c748a5ea3.jpg" />) implies</p><p><img src="10-7501443\403dc93b-c8c6-4382-acfd-0ddb5ec6c811.jpg" /></p><p>whereas regularity at the south pole (when<img src="10-7501443\654fe51a-9bda-447b-ab90-d57712b63176.jpg" />) requires</p><p><img src="10-7501443\16fa2cd0-ba66-47f1-b331-93f6265e3a27.jpg" /></p><p>Turn next to the radial part. <img src="10-7501443\f17a1e92-55a6-4082-a7bc-f794f8e4cecd.jpg" />is a solution of the linear differential equation:</p><disp-formula id="scirp.38879-formula20485"><label>(126)</label><graphic position="anchor" xlink:href="10-7501443\36bb93a7-7afc-4ff1-868a-7349a11be8f8.jpg"  xlink:type="simple"/></disp-formula><p>Two special limits call for inquiry, namely, the behaviour of the <img src="10-7501443\48273fc4-d8b1-4338-8c3d-46899adc9220.jpg" />-field at near and far distances from the source. Suppose firstly that, at spatial infinity, <img src="10-7501443\70b8bd37-157a-4230-a35b-f03cd880500a.jpg" />tends to <img src="10-7501443\e56cf3e1-0c63-4b7d-82c2-54d414b4eb78.jpg" /> Then, (126) reduces to the modified, spherical Bessel equation, which besides being linear and homogeneous: at infinity has as regular solutions the modified spherical Bessel functions of the third kind, often denoted as <img src="10-7501443\41f34c65-b86a-4e0a-be01-15d8727be77f.jpg" /> A few of them are listed below:</p><disp-formula id="scirp.38879-formula20486"><label>(127)</label><graphic position="anchor" xlink:href="10-7501443\8eb5e36b-3cf4-4222-8781-38f723754956.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.38879-formula20487"><label>(128)</label><graphic position="anchor" xlink:href="10-7501443\86b68b1a-8f3a-4e98-adc8-e709c9af9328.jpg"  xlink:type="simple"/></disp-formula><p><img src="10-7501443\e7cf20c1-f192-400c-898d-733f998e2849.jpg" /><img src="10-7501443\9bbf6213-b0fe-441d-af63-888c04d2495a.jpg" /> (129)</p><disp-formula id="scirp.38879-formula20488"><label>(130)</label><graphic position="anchor" xlink:href="10-7501443\b639164f-015c-4707-af31-9fe4811192b2.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.38879-formula20489"><label>(131)</label><graphic position="anchor" xlink:href="10-7501443\31ff4fe5-d165-4bed-b627-e1ee487402ef.jpg"  xlink:type="simple"/></disp-formula><p>The differential identity</p><disp-formula id="scirp.38879-formula20490"><label>(132)</label><graphic position="anchor" xlink:href="10-7501443\75a55583-9e15-473d-8a0c-e8340fc5ccdc.jpg"  xlink:type="simple"/></disp-formula><p>generates the rest. The exponential decay with distance shown in equations (127)-(131) and inferred from (132) is nothing more than the mathematically embodiment of the gyrogravitational Meissner effect.</p><p>On the other hand, in the vicinity of the source-where the relation <img src="10-7501443\3b05ace5-074c-4177-870b-5065be3f7b58.jpg" /> is expected—the term in (126) depending on such a parameter can be neglected, and moreover, if <img src="10-7501443\0f6d7e47-2b73-420a-afab-09222929b304.jpg" /> has a minimum at some spherical core but it does not vanish there, the r.h.s. of (126) can also be ignored up to terms of quadratic order. The radial function, under these assumptions, must take the form:</p><disp-formula id="scirp.38879-formula20491"><label>(133)</label><graphic position="anchor" xlink:href="10-7501443\2d6781c3-161c-4320-8ab1-098632fd8b44.jpg"  xlink:type="simple"/></disp-formula><p>Then, it is seen immediately, by restricting attention to the degenerate case: <img src="10-7501443\f79bbc86-d30f-474b-9cee-6b3307c4f075.jpg" /><img src="10-7501443\ae1cdfbe-3995-4381-82aa-b0f5b1b28d0b.jpg" />that if <img src="10-7501443\5b363d9b-7c6b-44f2-87c4-8d7a8dec588d.jpg" /> the combination of the radial and angular dependence leads, in the neighbourhood of the centre of symmetry, the following asymptotic behaviour for the vector potential <img src="10-7501443\83af3876-a68e-48bc-93c7-b24d43966cde.jpg" /></p><disp-formula id="scirp.38879-formula20492"><label>(134)</label><graphic position="anchor" xlink:href="10-7501443\c6e1a4fb-cc08-4491-b2a3-d7e95886f915.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.38879-formula20493"><label>(135)</label><graphic position="anchor" xlink:href="10-7501443\71b586f4-459a-4f44-84c6-235b75c96509.jpg"  xlink:type="simple"/></disp-formula><p>The first (the second) expression of the pair allows for a gravitomagnetic vector potential that is well defined at north (south) latitudes but not in the semi <img src="10-7501443\31bf53eb-8300-4ff4-9bd9-dc45575ca858.jpg" />-axis:</p><p><img src="10-7501443\d3abb5e7-b544-47c1-83d2-4aef0f5a4e83.jpg" /></p><p>referred to as the “Dirac string”. As it has been depicted in <xref ref-type="fig" rid="fig8">Figure 8</xref>. By direct comparison with (100), it is seen immediately that both <img src="10-7501443\f8bf0f3e-f14c-48d2-95e6-953e6f57a708.jpg" /> and <img src="10-7501443\7fc7b239-6896-4c14-b5aa-0b844ee818b7.jpg" /> lead to the same Hedgehog-like gravitomagnetic field:</p><disp-formula id="scirp.38879-formula20494"><label>(136)</label><graphic position="anchor" xlink:href="10-7501443\2943e63c-546f-4e4c-b62d-6758c5e8e2f4.jpg"  xlink:type="simple"/></disp-formula><p>whose exact form implies that <img src="10-7501443\8a15cbf2-d43d-4cb9-be06-3b05281db024.jpg" /> is the gravitational analogue of the “magnetic charge”. Thus, the gravitomagnetic field of (136) admits a description in terms of two different gravitomagnetic vector potentials <img src="10-7501443\d3424995-509e-48e3-82d4-c86a1dde3780.jpg" /> and <img src="10-7501443\bad4fc52-2b98-47a0-b062-fc3ad98bc65f.jpg" /> each of which is not singular (except at the origin) when they are assigned to a chart dividing the north and south hemispheres respectively. Using the former construction, Stokes theorem, and (136), it is readily verified that the total flux around the centre of symmetry <img src="10-7501443\d0e957d6-9abd-4f24-8ffa-d54d001f880e.jpg" /> of such a field is given by</p><disp-formula id="scirp.38879-formula20495"><label>(137)</label><graphic position="anchor" xlink:href="10-7501443\8dbef3c2-cc05-412f-83ca-b5cbb2f2644f.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="10-7501443\9e962131-ca2e-44ee-a824-ecef03424087.jpg" /> is a sphere of radius <img src="10-7501443\a68b442b-5da4-453d-8f8d-3a68d2ef84a3.jpg" /> with centre at the origin and <img src="10-7501443\8ae819d4-8eeb-4363-be11-0f5db47c160d.jpg" /> is its equator, as defined by the north and south poles; <img src="10-7501443\d256aeee-4117-4df0-97c7-02fdfdb6592b.jpg" />is a unit normal to <img src="10-7501443\2b94eceb-f099-4e60-b90c-c4e712422d40.jpg" /> pointing outwards, and <img src="10-7501443\3efa4d95-c66b-4289-8b1d-eb60355a8ad7.jpg" /> is the unit tangent vector to <img src="10-7501443\0310cbee-8be8-489d-96d7-9502cd38db0c.jpg" /> obtained by the corkscrew’s rule. Moreover, the fulfilment of the mathematical expression:</p><disp-formula id="scirp.38879-formula20496"><label>(138)</label><graphic position="anchor" xlink:href="10-7501443\f3a02ed0-2127-4643-991e-a78d1a4c6ad7.jpg"  xlink:type="simple"/></disp-formula><p>also establishes in differential form the existence of gravitomagnetic monopoles whenever <img src="10-7501443\69f455ad-68dc-4073-a180-3753ece4f133.jpg" /></p><sec id="s6_1"><title>6.1. <img src="10-7501443\9a79561a-3173-42f4-9b23-5d42b146cdc0.jpg" />and Dirac’s Quantization Condition</title><p>Gauge invariance, implicit for instance in (136), implies that the gravitomagnetic vector potentials <img src="10-7501443\dd6ebd18-2f0b-4788-97af-c2d75f2b2d5f.jpg" /> and <img src="10-7501443\55cb748e-4194-40be-a1a8-f4d53caed47b.jpg" /> given by (134) and (135) respectively, must in fact be related by a nonsingular gauge transformation. In effect</p><disp-formula id="scirp.38879-formula20497"><label>(139)</label><graphic position="anchor" xlink:href="10-7501443\ffb98a3d-383b-4222-8cb5-677df78931e9.jpg"  xlink:type="simple"/></disp-formula><p>where φ is the Goldstone boson field introduced in (3). Hence</p><disp-formula id="scirp.38879-formula20498"><label>(140)</label><graphic position="anchor" xlink:href="10-7501443\39de2757-0da9-4491-b37b-82465dbea409.jpg"  xlink:type="simple"/></disp-formula><p>and consequently:</p><disp-formula id="scirp.38879-formula20499"><label>(141)</label><graphic position="anchor" xlink:href="10-7501443\73eb03c4-367b-4093-b6d3-27d9e61061ac.jpg"  xlink:type="simple"/></disp-formula><p>Moreover, by (2), which contains the combination <img src="10-7501443\677a9dd5-3718-4334-8c5f-2feedad57c46.jpg" /> it is inferred that the gravitational potential amplitude <img src="10-7501443\8f07035f-c362-48d9-ad30-d7a0c8031630.jpg" /> must be a single valued function, not changing by marching out, going around the origin one or more times, and arriving to the same spacio-temporal point of departure. Thus, if <img src="10-7501443\43287333-a263-4774-880c-d0aaa696e6f0.jpg" /></p><disp-formula id="scirp.38879-formula20500"><label>(142)</label><graphic position="anchor" xlink:href="10-7501443\62d4129f-7128-4189-9b3a-6abc61e67c2b.jpg"  xlink:type="simple"/></disp-formula><p>It is seen, therefore, that Dirac’s quantization condition, given in [<xref ref-type="bibr" rid="scirp.38879-ref35">35</xref>], means that the existence of just one gravitomagnetic monopole would imply that the cosmological constant is not only quantized but also that its square root is given in exact multiples of some smallest value!</p></sec><sec id="s6_2"><title>6.2. Macroscopic <img src="10-7501443\c7804316-9e4a-4d34-8ea3-24bd678a8eb6.jpg" /> for Monopoles</title><p>It is time to reflect on the underlying mathematical aspects of the companion, modulus field <img src="10-7501443\2add2823-74cd-473a-a134-2aa9b5ea38f6.jpg" /> technically a sort of symmetry violating dial satisfying a Lichnerowicz’s like equation [<xref ref-type="bibr" rid="scirp.38879-ref6">6</xref>]:</p><p><img src="10-7501443\9b67b565-9446-40b5-a52b-005a1d85cae2.jpg" /><img src="10-7501443\707f1bce-3116-4c4b-93a0-89dce838ce78.jpg" />(143)</p><p>To get the leading order terms, in the hedgehog-like setting, insert the monopolar equation (134) into (143). In the asymptotic limit <img src="10-7501443\88bc3912-60c5-483e-95f1-ea616d61608b.jpg" /> when <img src="10-7501443\3c4707cf-eaa4-43be-bb76-82e083d829ef.jpg" /> goes to <img src="10-7501443\93cba845-f30b-4e57-941c-8ee94c3b8821.jpg" /> the resulting equation becomes separable and a solution of the form:</p><disp-formula id="scirp.38879-formula20501"><label>(144)</label><graphic position="anchor" xlink:href="10-7501443\e0e295db-c0a3-4b79-b776-43afc5fba460.jpg"  xlink:type="simple"/></disp-formula><p>is feasible, where <img src="10-7501443\e8f7d87d-9492-411c-b2a9-5bd3d5953ed2.jpg" /> are constant coefficients. The azimuthal, the radial, and the zenith equations that follow straightforwardly from applying the method of separation of variables are:</p><disp-formula id="scirp.38879-formula20502"><label>(145)</label><graphic position="anchor" xlink:href="10-7501443\84b334e3-5286-48ce-9f9b-7e50db4756cb.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.38879-formula20503"><label>(146)</label><graphic position="anchor" xlink:href="10-7501443\a4840175-99fe-4747-b1ad-829ac6c63a97.jpg"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.38879-formula20504"><label>(147)</label><graphic position="anchor" xlink:href="10-7501443\9208e9be-7709-4808-9d8d-07af4453aedf.jpg"  xlink:type="simple"/></disp-formula><p>respectively.</p><p><img src="10-7501443\37ca2914-a0a4-4c4f-8512-bebc91802465.jpg" /></p><p>solve evidently (145). If the <img src="10-7501443\91f58f18-7bcf-4adc-b0e2-71424c3b17e8.jpg" />-term is ignored, (146) leads to</p><disp-formula id="scirp.38879-formula20505"><label>(148)</label><graphic position="anchor" xlink:href="10-7501443\acd96653-ec99-4b95-b67e-1a75f3e1ae67.jpg"  xlink:type="simple"/></disp-formula><p>compare with (59). To unravel the solutions of (147), set <img src="10-7501443\f8fa0390-fa4b-4738-93e9-8bace43a44cf.jpg" /> and<img src="10-7501443\78e7d061-b916-4c39-a8e0-a69529fbd413.jpg" />, it transforms then into:</p><disp-formula id="scirp.38879-formula20506"><label>(149)</label><graphic position="anchor" xlink:href="10-7501443\b7be07bb-9842-4db4-a783-a856689a2fbe.jpg"  xlink:type="simple"/></disp-formula><p>For <img src="10-7501443\80f67efc-4200-4fc7-a4be-6ca78904eac3.jpg" /> a solution to (149) can be found by applying the series expansion method. Putting thus</p><disp-formula id="scirp.38879-formula20507"><label>(150)</label><graphic position="anchor" xlink:href="10-7501443\9f232553-5010-4be3-abd7-3c8752507e5d.jpg"  xlink:type="simple"/></disp-formula><p>into (149) and defining, for notational convenience,</p><disp-formula id="scirp.38879-formula20508"><label>(151)</label><graphic position="anchor" xlink:href="10-7501443\345966c4-0272-4be0-ad90-ef7941659594.jpg"  xlink:type="simple"/></disp-formula><p>the recurrence relation:</p><disp-formula id="scirp.38879-formula20509"><label>(152)</label><graphic position="anchor" xlink:href="10-7501443\0c559e0d-db19-4ed9-a2c4-df8d2544131b.jpg"  xlink:type="simple"/></disp-formula><p>limited by the rule <img src="10-7501443\00b20e44-f275-4e6e-8ce4-b649260fae67.jpg" /> is obtained immediately; <img src="10-7501443\eaa2205a-94fb-428d-bd2c-5e26c9982c49.jpg" />and <img src="10-7501443\766d9e1e-2e2e-417c-b373-ce747a5bb0f5.jpg" /> however, are arbitrary given numbers. D’Alembert’s criterion and the inferable property <img src="10-7501443\8e992171-5875-4fb7-beb5-e33b1220a285.jpg" /> imply that the resulting series converges for <img src="10-7501443\f8648c67-df3f-49ec-b86d-4ca32a4b8716.jpg" /> since</p><disp-formula id="scirp.38879-formula20510"><label>(153)</label><graphic position="anchor" xlink:href="10-7501443\9b2e2e12-ef7b-432e-9e35-fad37bae2e35.jpg"  xlink:type="simple"/></disp-formula><p>Henceforth,</p><disp-formula id="scirp.38879-formula20511"><label>(154)</label><graphic position="anchor" xlink:href="10-7501443\9e99fbae-c55d-4efc-b58e-fffb3be2cd04.jpg"  xlink:type="simple"/></disp-formula><p>In this way, the departure to <img src="10-7501443\95d55e07-ef1a-487c-8efd-5f752bdbc536.jpg" /> is obtained.</p><p>As for the limit of <img src="10-7501443\2309bf85-3297-449a-8ddb-5cd092ac59f5.jpg" /> at small radii, the dominant contribution arises from the <img src="10-7501443\81c85e17-4764-471c-b0be-83a50e8f3d31.jpg" />-term. By (136), (143) reduces, in such a limit, to:</p><p><img src="10-7501443\9f7e177a-10eb-4408-974a-1076526aa1f4.jpg" /></p><p>where <img src="10-7501443\a6804875-317a-49df-ae3a-fbb768b3cd21.jpg" /> Using the change of variable: <img src="10-7501443\8d86310f-be50-419c-a23d-c43d947ea03d.jpg" />it is easily seen that when the integration constants <img src="10-7501443\98e52d6b-1832-44ff-aaa8-6b3770170003.jpg" /> and <img src="10-7501443\086bdd43-d795-4e61-9707-da3471004502.jpg" /> are nonzero, then</p><disp-formula id="scirp.38879-formula20512"><label>(155)</label><graphic position="anchor" xlink:href="10-7501443\f001890e-6250-4b79-a119-12a8bed89348.jpg"  xlink:type="simple"/></disp-formula><p>solves the problem, and thus, if <img src="10-7501443\9ad5524c-4b60-4147-803f-0a90325d9536.jpg" /></p><disp-formula id="scirp.38879-formula20513"><label>(156)</label><graphic position="anchor" xlink:href="10-7501443\d39aa9e3-f0e0-4d26-ad2e-d305dc13e9af.jpg"  xlink:type="simple"/></disp-formula></sec></sec><sec id="s7"><title>7. A Note on Dyons</title><p>From the multipolar expansion (106) of the <img src="10-7501443\34362aa8-4469-4411-9139-7f921f2b5ddc.jpg" />-scalar field-which it must not be forgotten, it was obtained under the assumption of an orthonormal, spherically symmetric grid, the gravitomagnetic form <img src="10-7501443\a28bc596-8965-406d-96db-cc62c732255f.jpg" /> can be extracted. By combining (118) and (129), it is seen immediately that the dipolar <img src="10-7501443\438eee61-4f2a-40dc-9e11-73e4e0482f64.jpg" /> contribution to the <img src="10-7501443\db698996-98ac-4292-aa46-5c42c2a54834.jpg" /> differential encompass, for instance, the following form:</p><disp-formula id="scirp.38879-formula20514"><label>(157)</label><graphic position="anchor" xlink:href="10-7501443\1164f4ca-b757-490c-87ab-3d7d27c3ab00.jpg"  xlink:type="simple"/></disp-formula><p>for <img src="10-7501443\23ec9d8a-5030-4395-b363-eb6e54874776.jpg" /> and<img src="10-7501443\0bccb4dd-b785-4578-b83f-c29f6b17969e.jpg" />. However, if <img src="10-7501443\536aeba3-2084-45a2-829a-cdb15f7c17ff.jpg" /> (118) and (133) implies (for<img src="10-7501443\45a6b3aa-c58b-4d67-80b2-30e5fbe6aa20.jpg" />) that:</p><disp-formula id="scirp.38879-formula20515"><label>(158)</label><graphic position="anchor" xlink:href="10-7501443\9e4a3614-ebbc-4a4e-92e2-d1796e8fb339.jpg"  xlink:type="simple"/></disp-formula><p>Both expressions, one when the space-time becomes superconducting and the other valid in the vicinity of the source, contain the</p><p><img src="10-7501443\cfa5edb3-c814-424c-a2ee-6bfe846202d5.jpg" /></p><p>piece of the Taub-NUT space: an exact, spatially homogeneous solution of the vacuum Einstein’s equations, first discovered in 1951 by A. H. Taub and extended analytically a little bit later by E. Newman, L. Tamburino, and T. Unti [44,45]. The Taub-NUT solution has topology <img src="10-7501443\b660af1d-3d62-49cf-93d4-161d0486e045.jpg" /> It determines the gravitational field produced by a gravitational dyon of mass <img src="10-7501443\23896851-2f94-4e71-8729-638cbd8e4314.jpg" /> and gravitating magnetic mass <img src="10-7501443\9c0f6dbb-0c76-4eb4-aefc-56b650c9a7d5.jpg" /> [<xref ref-type="bibr" rid="scirp.38879-ref46">46</xref>]. Its metric, in gravitomagnetic units and isotropic coordinates, can be written, if <img src="10-7501443\59ebbc1a-99bb-44cf-9863-08e889282b80.jpg" /> as:</p><disp-formula id="scirp.38879-formula20516"><label>(159)</label><graphic position="anchor" xlink:href="10-7501443\21b636ad-4edf-4b6e-ba85-0dbdae1bfdd3.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="10-7501443\19ededf1-f7ad-4ef8-adac-f72443295505.jpg" /> <img src="10-7501443\079a2753-7d51-4ab6-b3b5-cb893de2c57b.jpg" /> reduces to:</p><disp-formula id="scirp.38879-formula20517"><label>(160)</label><graphic position="anchor" xlink:href="10-7501443\14185248-1a9b-4bf0-9c6c-54b3917d43e6.jpg"  xlink:type="simple"/></disp-formula><p>Here <img src="10-7501443\9f0e21d8-1c96-4f7c-b0ec-2a19aba33106.jpg" /> and <img src="10-7501443\880eca61-815f-4c78-8893-c264096d067c.jpg" /> are Euler coordinates on <img src="10-7501443\4c18ff71-659e-4c24-8953-57d60e36a1d4.jpg" /> while <img src="10-7501443\e2e4beba-2e95-49e4-a29f-48600593c367.jpg" /> denotes the isotropic radial coordinate. Common points between (155) and (160) can be established at<img src="10-7501443\821bb368-f381-4a3f-9fc7-63c71b911789.jpg" />. The Taub-NUT space-time is better visualized by the product of the Hopf fibering</p><p><img src="10-7501443\ca9767f3-af48-4074-8810-446e7d797c3f.jpg" /></p><p>with the <img src="10-7501443\21309e73-921c-4956-aa46-c6a137ae9735.jpg" />-axis <img src="10-7501443\6fdfe85a-9a68-421d-8a65-191249328de0.jpg" /> <img src="10-7501443\52caf158-e71b-44a0-8eea-4df4763a2392.jpg" /> corresponds to an horizon and <img src="10-7501443\bb89a9cd-0b44-47ee-bba0-62fa3cb98944.jpg" /> to an irremovable curvature singularity [<xref ref-type="bibr" rid="scirp.38879-ref46">46</xref>]. In (159) <img src="10-7501443\9ef4049e-4208-4d78-b63f-bae3f85abd84.jpg" />however, any establishment of space-time superconducting requires <img src="10-7501443\2ec88a62-f089-4dd4-9575-bf6c5059cd10.jpg" /> <img src="10-7501443\e8f2ab78-b34f-4a1c-a7f4-70fcefd87e50.jpg" /> as depicted in <xref ref-type="fig" rid="fig2">Figure 2</xref>. Current observation limits <img src="10-7501443\eb4e546e-b49d-4e36-b241-a006e0e02c5c.jpg" /> to a rather small value.</p></sec><sec id="s8"><title>8. A Note on Topology Change</title><p>When <img src="10-7501443\2eebae1f-c307-4d0d-baa3-32927452e1ec.jpg" /> but <img src="10-7501443\ae082be9-a57d-4cf2-b113-e92eb1c535aa.jpg" /> does not vanish, (117) and (133) imply:</p><disp-formula id="scirp.38879-formula20518"><label>(161)</label><graphic position="anchor" xlink:href="10-7501443\592709cd-25f9-4159-9d1f-b98bfa4ad9b4.jpg"  xlink:type="simple"/></disp-formula><p>The <img src="10-7501443\98de733c-5204-4a10-8fd4-1192a6581bac.jpg" /> factor of (134) has utterly disappeared (similar comments apply for<img src="10-7501443\aa03c01d-874d-41bf-90d7-26503b5ddd00.jpg" />). In that case, by (100):</p><disp-formula id="scirp.38879-formula20519"><label>(162)</label><graphic position="anchor" xlink:href="10-7501443\b092597c-d9cf-425b-a79e-2408b232da23.jpg"  xlink:type="simple"/></disp-formula><p>implying at once:</p><disp-formula id="scirp.38879-formula20520"><label>(163)</label><graphic position="anchor" xlink:href="10-7501443\e81e05cd-6023-42dc-83f2-696b0d65c24f.jpg"  xlink:type="simple"/></disp-formula><p>Such gravitomagnetic field is singular along the nonpositive <img src="10-7501443\d25b9e31-ad97-40a5-b712-27612e961574.jpg" />-semi-axis and it can be interpreted as a tear or cut (labeled <img src="10-7501443\e22025f2-5d4c-42ce-9ab5-ec62c723f2f8.jpg" /> in <xref ref-type="fig" rid="fig9">Figure 9</xref>) in the very fabric of the space-time. The lines of force create a family of parabolic curves cutting orthogonally the equipotential surfaces: a coaxial set of paraboloids of revolution. In the figure, the gravitomagnetic-field intensity can be read off from the arrow’s length. Space-time ripping opens the possibility of topology change in quantum gravity.</p></sec><sec id="s9"><title>9. Remarks and Conclusions</title><p>The universe has at least several billions of galaxies. An</p><p>explanation of their origin and stability remains, however, uncertain. And it rises two of the most fundamental open problems in Physics, like one time ago were the structure and stability problems of the atom, that led to the quantum revolution. In the present state of knowledge, no man of our age, no inflationist, no dark matter theorist, can claim to know for sure the identity of the primeval mechanism giving rise to the rich galactic tapestry observed across the cosmos, or the way that the dismantling of the largest structures of the universe is avoided.</p><p>The lack of a fully satisfactory explanation to such basic issues, and the impression that perhaps inflation and dark matter (although actively pursued) are not enough, because there are still relevant missing pieces needed to achieve complete clarification, like the unification of quantum mechanics with the general theory of relativity, certainly calls for a revision of our most cherished ideas, concerning the nature of space, time, and matter. It is in this spirit, that we have set to explore the likeliness that “even at large scales” the space-time might exhibit some very striking properties of purely quantum origin, which might well have passed unnoticed, in favour of other powerful possibilities that have become very tight to our way of thinking, like the lightest supersymmetric particle idea which depends on the assumption of R-parity conserving supersymmetry.</p><p>The point of view adopted in this article is that at the core of the dark matter conundrum lies the problem of finding how to develop a consistent law of inertia for a discrete, quantum fluctuating, space-time background, and not necessarily the presence-in some exact proportion-of an entirely new class of particle per se, such as the neutralino or the invisible axion, that may or may not exist in the required amounts.</p><p>According to the Einstein-Hilbert action, asymptotic flatness seems like a very natural&#160; restriction to follow for the classical geometry due to an isolated, static, point-like source in empty space. However, at the fundamental level, the 4-dimensional space-time of our direct experience might not be a continuum [<xref ref-type="bibr" rid="scirp.38879-ref47">47</xref>] and discrete entities (“space-time atoms”) might rule its dynamics [48,49]. This possibility might be enough to radically change the picture provided by classical theory, and to put into question the “relevance” of the asymptotic flatness hypothesis: all the entities that we know about in Nature, at least the ones which are linked (in one away or the other) to indistinguishable particles, follow well defined statistical rules: Bose-Einstein or Fermi-Dirac statistics. Therefore, it seem natural to speculate that perhaps such “space-time atoms” could suffer from a similar identity crisis than the one known to exist in superfluids [6,50], specifically in a situation where phrases like: “low temperature” and “the lowest state of energy” apply. All these reasons, including the analogy of an stable atom surrounded by superconducting currents, but more strongly, the precise mathematical form, piece by piece, of the Einstein-Hilbert action led unavoidably to the exploration of the “space-time as a superconductor” paradigm [<xref ref-type="bibr" rid="scirp.38879-ref6">6</xref>]; an exercise that it is not only useful to provide a fertile arena for contrasting (and estimate) how classical ideas about the nature of the space-time can get altered when quantum affects are taken into account, but also to translate the main difficulties encountered in the dynamical study of galaxies in a completely new language, where different technical tools can be put in practice with the hope of getting better insights about how to handle the fundamental unsolved questions of their dynamics, such as the well known “winding dilemma”.</p><p>This article focuses primarily on finding out the distinctive, physical consequences of modifying, in precise accord to a gauge principle [see (5), (6), and (7)], the l.h.s. of Einstein’s field equations, by the addition of a phase factor to one of the gravitational potentials: Equations (2) and (3). The first thing that comes across is the similarity of such gravitational theory with the theory of superconductivity, which surely cannot be an accident.</p><p>It was highlighted that:</p><p>•&#160;&#160;&#160;&#160;&#160;&#160; Firstly: The cosmological constant (which in terms of Planck units is as small as<img src="10-7501443\eb6638ac-612a-4131-9a84-894b6d914a99.jpg" />) can be linked with the minimal gravitomagnetic (or gyrogravitational) flux supported by a spinning string [see (58) and (142)].</p><p>•&#160;&#160;&#160;&#160;&#160;&#160; Secondly: the appearance of supercurrents around rotating astrophysical bodies can modify the spacetime geometry in such a way that the aforementioned complex potential gets a modulus which remains very close to a characteristic value [e.g. (59), (144) and (148)], while the gravitomagnetic vector potential acquires mass causing an exponentially decay (with distance) of the gravitomagnetic field [e.g. (127)- (131)]; this picture, as discussed in [<xref ref-type="bibr" rid="scirp.38879-ref6">6</xref>], provides an alternative to the dark-matter-halo hypothesis, see <xref ref-type="fig" rid="fig9">Figure 9</xref>.</p><p>•&#160;&#160;&#160;&#160;&#160;&#160; Thirdly: vortex and monopole solutions can be found [Section 4 and Section 6] exhibiting in full the superfluid properties of the space-time; the critical point of the quantum phase transition, where the order <img src="10-7501443\5c7dbbbe-fca3-4994-9c59-d4fadb65b8ac.jpg" />- parameter vanishes, takes place at space-time singularities, see <xref ref-type="fig" rid="fig9">Figure 9</xref>.</p><p>•&#160;&#160;&#160;&#160;&#160;&#160; Fourthly: the close enough mathematical similitude that can be established with subatomic models where hadrons are viewed as being made up of quarks bound by dual strings [51,52], suggests the application of the scheme just presented to the study of open strings having gravitomagnetic monopoles at their ends, or where, spinning strings (open or closed)</p><p>break or join when they interact.</p><p>•&#160;&#160;&#160;&#160;&#160;&#160; Finally: but not least, two crucial differences when a comparison is made with the type of superconductivity found in metals like Nb is that, firstly, our theory is not renormalizable, and secondly, that two axis-aligned quantum vortices with the same sense of spin not only exhibit zones of repulsion but also of attraction, depending on their relative geodetic distance [see (86)]; this in itself is an invitation to reflect, in this new setting, on the spin-statistic theorem and supersymmetry.</p><p>It might seem fitting to recall (as a matter of reflexion or even as an historical panoramic view) Einstein’s own remarks, set in the 1920s, regarding the revolutionary impact brought in by the discovery of superconductivity [<xref ref-type="bibr" rid="scirp.38879-ref53">53</xref>]:</p><p>“The theoretical oriented scientist cannot be envied, because Nature, i.e. the experiment, is a relentless and not very friendly judge of his work. In the best case scenario it only says ‘maybe’ to a theory, but never ‘yes’ and in most cases ‘no’. If an experiment agrees with theory it means ‘perhaps’ for the later. If it does not agree it means ‘no.’ Almost any theory will experience a ‘no’ at one point in time-most theories very soon after they have been developed. In this paper we want to focus on the fate of theories concerning metallic conductivity.”</p><p>In summary, the list on the left assembles some of the features-topological traces if you will-that should be present in our universe if the space-time behaves, in some places and times, as a superconductor: obeying (say) an action principle like (7). According to the train of thought pushed forward: when this happens, the <img src="10-7501443\4985d768-19ad-4489-9631-b7784f8d32ac.jpg" /> space-time is quite capable of producing quantum vortices of (minimal) quantized gravitomagnetic flux <img src="10-7501443\ac59e673-c25f-4b1e-98a7-b260583d13e9.jpg" /> looping back on themselves to form rings, see <xref ref-type="fig" rid="fig6">Figure 6</xref>. At a first rough approximation, such entities should obey the Nambu-Goto action to take into account any relativistic Lorentz contraction of their vortex core, or better yet, a sort of Kalb-Ramond effective action to incorporate the topological coupling to the Goldstone boson field; what is more, by virtue of (86), they also self interact. All these features, together with the “hydrodynamical” Magnus effect, are expected to be crucial to correctly obtain their effective equation of motion: these distinctive “hula-hoop” structures not only are capable of reproducing spin-2 effects [<xref ref-type="bibr" rid="scirp.38879-ref52">52</xref>] but also are the natural analogue of the higher energy excitations referred to as “rotons” in helium II [54,55]. Such looped excitations, let’s call them gravitational rotons, can form supercurrents: which can persist for very long times, as Cooper pairs do in a superconducting wire, or photons do in a laser, or electrons in an atom, affecting the inertia of test orbiting bodies by a frame-dragging effect and producing places of uniformity in the spatial geometry [see <xref ref-type="fig" rid="fig4">Figure 4</xref> and Equations (59) and (148)].</p><p>Thus, a crucial question arises: Could these theoretical ideas: superfluidity of the space-time, supercurrents of gravitational rotons, quantization of vacuum energy, frame dragging, as well as a Higgs mechanism for gravity-located in the borderline typified by the shifty split between micro-macro, reversible-irreversible, and quatumclassical, bring us closer to identify the nature of cold dark matter?</p><p>Is the space-time a superconductor?</p><p>We do not know the answer yet, but surely Nature will tell us.</p></sec><sec id="s10"><title>REFERENCES</title></sec><sec id="s11"><title>NOTES</title></sec></body><back><ref-list><title>References</title><ref id="scirp.38879-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">F. 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