<?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">JHEPGC</journal-id><journal-title-group><journal-title>Journal of High Energy Physics, Gravitation and Cosmology</journal-title></journal-title-group><issn pub-type="epub">2380-4327</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/jhepgc.2018.43026</article-id><article-id pub-id-type="publisher-id">JHEPGC-85832</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>
 
 
  How a Minimum Time Step and Formation of Initial Causal Structure in Space-Time May Void the Penrose Singularity Theorem, as in Hawkings and Ellis’s 1973 Write-Ups
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Andrew</surname><given-names>Walcott Beckwith</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>Physics Department, Chongqing University, Chongqing, China</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>rwill9955b@gmail.com</email></corresp></author-notes><pub-date pub-type="epub"><day>28</day><month>06</month><year>2018</year></pub-date><volume>04</volume><issue>03</issue><fpage>485</fpage><lpage>491</lpage><history><date date-type="received"><day>7,</day>	<month>May</month>	<year>2018</year></date><date date-type="rev-recd"><day>3,</day>	<month>July</month>	<year>2018</year>	</date><date date-type="accepted"><day>6,</day>	<month>July</month>	<year>2018</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><html>
 <head></head>
 
  Using a root finder procedure to obtain 
  <img src="Edit_d37aed4e-c2d1-4208-969f-cc34371dd259.bmp" alt="" /> we use an inflaton value due to use of a scale factor 
  <img src="Edit_672248ae-857a-4d3c-8b19-f7579842596c.bmp" alt="" /> if we furthermore use 
  <img src="Edit_55b67a17-5303-4f85-8a14-a34839daca33.bmp" alt="" /> . From use of the inflaton, we initiate a procedure for a minimum scale factor, which would entail the 
  <img src="Edit_187a7045-4ff7-4212-adc3-e9619bd0b55e.bmp" alt="" /> , for a sufficiently well placed frequency ω. If the Non Linear Electrodynamics procedure of Camara et al. of General relativity was used, plus the modified Heisenberg Uncertainty principle, of Beckwith, and others,
  <em> i.e <img src="Edit_10b5ac05-3227-4990-8d40-99833837cfc8.bmp" alt="" />.</em> we come due to a sufficiently high frequency a case for which 
  <img src="Edit_9de51016-5018-4381-9374-3a5d90385fc1.bmp" alt="" /> implies a violation of the Penrose singularity theorem, 
  <em>i.e</em> . this is in lieu of  
  <img src="Edit_722d0a5e-a867-4fd7-8e2e-3d060b8758eb.bmp" alt="" />. If this is not true,
  <em> i.e.</em> that the initial 
  <img src="Edit_744fb141-bb8c-4e27-8486-32af956bf71a.bmp" alt="" /> , then we will likely avoid 
  <img src="Edit_ba57651e-7d4b-488e-ab91-3e4ed33e2452.bmp" alt="" /> for reasons brought up in this manuscript.
 
</html></p></abstract><kwd-group><kwd>Inflaton Physics</kwd><kwd> Causal Structure</kwd><kwd> Non Linear Electrodynamics</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Framing the Initial Inquiry</title><p>Here, the idea would be, to make the following equivalence, namely look at, [<xref ref-type="bibr" rid="scirp.85832-ref1">1</xref>] as well as our own derivation</p><p>[ [ Λ Max r 4 8 π G ] ⋅ ( 4 / 3 ) ⋅ [ 2 π 2 g ∗ 45 ] 1 / 3 ] 3 / 4 ~ S initial (1)</p><p>We furthermore, make the assumption of a minimum radius of [<xref ref-type="bibr" rid="scirp.85832-ref2">2</xref>] [<xref ref-type="bibr" rid="scirp.85832-ref3">3</xref>]</p><p>R initial ~ 1 # l N g &lt; l Planck (2)</p><p>We will initially be assuming that the cosmological constant remains at a constant value, as it is today, and does not change over time (which is the situation given in [<xref ref-type="bibr" rid="scirp.85832-ref4">4</xref>] ) as given by Park et al., where the initial value of the cosmological constant could be much higher initially.</p><p>This Equation (1) will be put as the minimum value of r, where we have in this situation [<xref ref-type="bibr" rid="scirp.85832-ref5">5</xref>] [<xref ref-type="bibr" rid="scirp.85832-ref6">6</xref>]</p><p># bits ~ [ E ℏ ⋅ l c ] 3 / 4 ≈ [ M c 2 ℏ ⋅ l c ] 3 / 4 (3)</p><p>And if M is the total space-time energy mass, for initial condition [<xref ref-type="bibr" rid="scirp.85832-ref5">5</xref>] [<xref ref-type="bibr" rid="scirp.85832-ref6">6</xref>] where</p><p>S initial ~ n graviton ~ initial   graviton   count (4)</p><p>M then will be defined by the mass of a massive graviton [<xref ref-type="bibr" rid="scirp.85832-ref7">7</xref>] , times, the graviton count, as given in (4) and the modified uncertainty principle, [<xref ref-type="bibr" rid="scirp.85832-ref3">3</xref>] and the Camarra et al. defined Hubble parameter, given in [<xref ref-type="bibr" rid="scirp.85832-ref2">2</xref>]</p><p>Δ E ~ [ ℏ / Δ t ⋅ ( δ g t t ~ a min 2 ⋅ ϕ initial ) ] | Pre-Planckian           ~ H ( Hubble ) ~ 4 π G B 2 3 c 2 μ 0 ⋅ ( 1 − 8 μ 0 ω B 2 ) + Λ c 2 3           ~ 4 π G B 2 3 c 2 μ 0 ⋅ ( 1 − 8 μ 0 ω B 2 ) + Λ Today c 2 3 (5)</p><p>This will lead to</p><p>a min ~ &#177; # ⋅ ( 1 + i ) 2 (6)</p><p>whereas if Λ ≫ Λ Today , Equation (6) likely will not hold, and we also state that Equation (6) is a violation of the Penrose singularity theorem as written up in [<xref ref-type="bibr" rid="scirp.85832-ref8">8</xref>] , whereas we also have that we are using the Padmanbhan results as given in [<xref ref-type="bibr" rid="scirp.85832-ref9">9</xref>] [<xref ref-type="bibr" rid="scirp.85832-ref10">10</xref>] [<xref ref-type="bibr" rid="scirp.85832-ref11">11</xref>] to the effect that we are employing</p><p>a ~ a initial t γ ϕ = γ 4 π G ln [ 8 π V 0 G γ ( 3 γ − 1 ) ⋅ t ] (7)</p><p>While adhering to a potential in line with</p><p>V = V 0 exp [ { − 16 π G γ } ⋅ ϕ ( t ) ] (8)</p><p>We next then go to the results given in [<xref ref-type="bibr" rid="scirp.85832-ref9">9</xref>] , which is a publication in JHEPGC by the author, in 2017.</p></sec><sec id="s2"><title>2. Examination of the Minimum Time Step, in Pre-Planckian Space-Time as a Root of a Polynomial Equation</title><p>We initiate our work, citing [<xref ref-type="bibr" rid="scirp.85832-ref9">9</xref>] to the effect that we have a polynomial equation for the formation of a root finding procedure for Δ t , namely if</p><p>Δ t ⋅ | ( 8 π G V 0 γ ⋅ ( 3 γ − 1 ) ⋅ Δ t − 1 ) − ( 8 π G V 0 γ ⋅ ( 3 γ − 1 ) ⋅ Δ t − 1 ) 2 2 + ( 8 π G V 0 γ ⋅ ( 3 γ − 1 ) ⋅ Δ t − 1 ) 3 3 − ⋯ | ≈ ( γ π G ) − 1 48 π ℏ a min 2 ⋅ Λ (9)</p><p>From here, we then cited, in [<xref ref-type="bibr" rid="scirp.85832-ref9">9</xref>] , using [<xref ref-type="bibr" rid="scirp.85832-ref6">6</xref>] a criteria as to formation of entropy, i.e. If Λ is an invariant cosmological “constant” and if Equation (10) holds, we can use the existence of nonzero initial entropy as the formation point of an arrow of time.</p><p>S Λ | Arrow-of-time = π ⋅ ( R c | initial ~ c ⋅ Δ t l Planck ) 2 ≠ 0 (10)</p><p>This leads to the following, namely in [<xref ref-type="bibr" rid="scirp.85832-ref9">9</xref>] we make our treatment of the existence of causal structure, as given by writing its emergence as contingent upon having</p><p>( R c | initial ~ c ⋅ Δ t l Planck ) ~ ϑ ( 1 ) (11)</p><p>The rest of this article will be contingent upon making the following assumptions. FTR</p><p>That we will drop most of the terms in the expansion of Equation (9) and instead of a huge infinite expansion of terms, pick instead using</p><p>Δ t ⋅ ( 8 π G V 0 γ ⋅ ( 3 γ − 1 ) ⋅ Δ t − 1 ) ≈ ( γ π G ) − 1 48 π ℏ a min 2 ⋅ Λ (12)</p><p>This is assuming here that the terms in ( 8 π G V 0 γ ⋅ ( 3 γ − 1 ) ⋅ Δ t − 1 ) are extremely</p><p>small, which permits us to come up with a quadratic expression of the term Δ t which is of course useful as to what we do next, i.e.</p><p>If we make use of the Peebles relationship [<xref ref-type="bibr" rid="scirp.85832-ref12">12</xref>] of what would be occurring just before and at the start of expansion of the universe, i.e. the causal structure as given by [<xref ref-type="bibr" rid="scirp.85832-ref9">9</xref>] as, using the Keiffer result of [<xref ref-type="bibr" rid="scirp.85832-ref13">13</xref>] so as to get</p><disp-formula id="scirp.85832-formula1"><label>(13)</label><graphic position="anchor" xlink:href="//html.scirp.org/file/3-2180222x2.png"  xlink:type="simple"/></disp-formula></sec><sec id="s3"><title>3. Consequences, in Terms of the Minimum Scale Factor</title><p>We then use the Peebles result [<xref ref-type="bibr" rid="scirp.85832-ref12">12</xref>] for the strain of space-time at the START of expansion result of</p><p>Δ E ~ [ ℏ / Δ t ⋅ ( δ g t t ~ a min 2 ⋅ ϕ initial ) ] | Pre-Planckian             ~ H ( Hubble ) ~ 4 π G B 2 3 c 2 μ 0 ⋅ ( 1 − 8 μ 0 ω B 2 ) + Λ c 2 3             ~ 4 π G B 2 3 c 2 μ 0 ⋅ ( 1 − 8 μ 0 ω B 2 ) + Λ Today c 2 3 (14)</p><p>The key result is that we have a quadratic expression for the Δ t term, as indicated by (12) with the result that there is a solvable expression in terms of Δ t , so that then, we can take the square of the terms of Equation (14) with using the expression of Equation (7) above, in order to obtain after using an expansion of Ln x, (if 0 &lt; x &lt; 2) from [<xref ref-type="bibr" rid="scirp.85832-ref14">14</xref>] to get, then, after algebra</p><p>γ 4 π G ( 8 π G V 0 γ ⋅ ( 3 γ − 1 ) ⋅ Δ t − 1 ) 2 ~ ℏ 2 a min 4 ⋅ ( Δ t ) 2 ⋅ ( 4 π G B 2 3 c 2 μ 0 ⋅ ( 1 − 8 μ 0 ω B 2 ) + Λ Today c 2 3 ) (15)</p><p>This is also reflecting the ideas given in reference [<xref ref-type="bibr" rid="scirp.85832-ref15">15</xref>] which has similar ideas which are similar to our Equation (15) above.</p></sec><sec id="s4"><title>4. Conclusion, Two Parts</title><sec id="s4_1"><title>4.1. So What If the Denominator of Equation (15) Is Less Than Zero?</title><p>If that happens, due to a very high frequency value for gravitational waves, and a small cosmological constant, we then have</p><p>a min 4 &lt; 0 ⇒ a min ~ &#177; # ⋅ ( 1 + i ) 2 (16)</p><p>Note here that when this happens, we have two equally admissible solutions for the scale factor, minimum, and the consequences; if # is a real number, then we have a contradiction with what is called Theorem 3, Hawking (1967) as cited on page 271, of [<xref ref-type="bibr" rid="scirp.85832-ref8">8</xref>] we have that</p><p>Theorem 3: If R a b K a K b ≥ 0 for every non space-like Vector K</p><p>1) The strong casuality condition holds on ( M ˜ , g ) ,</p><p>2) There is some past-directed unit timelike vector W at a point p, and a positive constant b, such that if V is the Unit tangent factor to the past directed timelike geodesic through p, then on each geodesic the expansion θ ≡ V ; a a of these geodesics becomes less than −3c/p, within a distance b/c from p, where c = − W a V a , i.e. then there is a past incomplete non space-like geodesic through p.</p><p>One does not have a curve violating the causality conditions as given as an assertion by Hawkings and Ellis, 1973. i.e. there is, if this occurs at the causal boundary, instead, a bifurcation point at the surface of the causal set, with real and imaginary components, but the incompleteness of the non space geodesic through a point p, if it is on the surface of the causal surface, as defined by Equation (13) is not due to a point p-. It is well known that certain Kerr black hole models, as in page 465 of Ohanian and Ruffini [<xref ref-type="bibr" rid="scirp.85832-ref14">14</xref>] involve the use of g t t ~ 0 for their horizon surfaces and the definition of a plate disc singularity surface but we are instead employing, δ g t t ~ a min 2 ⋅ ϕ initial .</p><p>i.e. precisely because we have avoided using g t t ~ 0 as was done in the Kerr black holes, as given in [<xref ref-type="bibr" rid="scirp.85832-ref14">14</xref>] but instead have the δ g t t ~ a min 2 ⋅ ϕ initial plus the situation we wish to avoid, that of instead looking at</p><p>a min 4 &lt; 0 ⇒ a min ~ &#177; # ⋅ ( 1 + i ) 2 , that a causal surface, would be formed on a</p><p>sphere of space time which would in itself violate the 3<sup>rd</sup> Penrose theorem.</p></sec><sec id="s4_2"><title>4.2. So What Happens If Λ i n i t i a l ≫ Λ T o d a y ?</title><p>The second case to consider would be if we have, instead of today’s version of the cosmological constant, a large valued initial cosmological constant, in which then</p><p>γ 4 π G ( 8 π G V 0 γ ⋅ ( 3 γ − 1 ) ⋅ Δ t − 1 ) 2 ~ ℏ 2 a min 4 ⋅ ( Δ t ) 2 ⋅ ( Λ initial c 2 3 ) &amp;     Λ initial ≫ Λ Today (17)</p><p>We argue that then, there is no reason for assigning a singularity, but it would in line with [<xref ref-type="bibr" rid="scirp.85832-ref4">4</xref>] , i.e. assigning an almost infinite value for the initial cosmological constant.</p><p>Different variants of the above can be imagined, and of course one should be considering [<xref ref-type="bibr" rid="scirp.85832-ref16">16</xref>] in the reformulation of the Causal structure boundary idea. In addition the points brought up as to [<xref ref-type="bibr" rid="scirp.85832-ref17">17</xref>] to [<xref ref-type="bibr" rid="scirp.85832-ref21">21</xref>] of the nonlinear electrodynamics cosmology should be utilized as a refinement as to the Hubble parameter as outlined in Equation (5) above.</p></sec><sec id="s4_3"><title>4.3. Otonion Geometry and Non-Commutativity as a Future Project to Be Combined with Our Present Inquiry?</title><p>We should close with one reference as to the Octonionic geometry program as follows. We may be seeing instead of just our roof finder iterations, as outlined above, an exploration into non commutative geometry. This is what I am referring to, and it is from [<xref ref-type="bibr" rid="scirp.85832-ref22">22</xref>] .</p><p>From [<xref ref-type="bibr" rid="scirp.85832-ref22">22</xref>]</p><p>Quote:</p><p>i.e.</p><p>The change in geometry is occurring when we have first a pre quantum space time state, in which, in commutation relations [<xref ref-type="bibr" rid="scirp.85832-ref23">23</xref>] (Crowell, 2005) in the pre Octonion space time regime no approach to QM commutations is possible as seen by.</p><p>[ x j , p j ] ≠ − β ⋅ ( l Planck / l ) ⋅ ℏ T i j k x k     and   does   not → i ℏ δ i , j (18)</p><p>Equation (18) is such that even if one is in flat Euclidian space, and i = j, then</p><p>[ x j , p j ] ≠ i ⋅ ℏ (19)</p><p>In the situation when we approach quantum “octonion gravity applicable” geometry, Equation (18) becomes</p><p>[ x j , p j ] = − β ⋅ ( l Planck / l ) ⋅ ℏ T i j k x k → Approaching-flat-space i ℏ δ i , j (20)</p><p>End of quote</p><p>We assert that the issues as of Equation (18) to Equation (20) if done in higher dimensional analogues, taking into account non commutative initial geometry as outlined in [<xref ref-type="bibr" rid="scirp.85832-ref23">23</xref>] in time, if twinned directly with an analysis of Equation (15) to Equation (17) may in time help us delineate the future of space time research in the early universe.</p></sec></sec><sec id="s5"><title>Acknowledgements</title><p>This work is supported in part by National Nature Science Foundation of China grant No. 11375279.</p></sec><sec id="s6"><title>Cite this paper</title><p>Beckwith, A.W. (2018) How a Minimum Time Step and Formation of Initial Causal Structure in Space-Time May Void the Penrose Singularity Theorem, as in Hawkings and Ellis’s 1973 Write-Ups. Journal of High Energy Physics, Gravitation and Cosmology, 4, 485-491. https://doi.org/10.4236/jhepgc.2018.43026</p></sec></body><back><ref-list><title>References</title><ref id="scirp.85832-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Kolb, E. and Turner, S. (1994) The Early Universe. Westview Press, Chicago.</mixed-citation></ref><ref id="scirp.85832-ref2"><label>2</label><mixed-citation publication-type="other" xlink:type="simple">Camara, C.S., de Garcia Maia, M.R., Carvalho, J.C. and Lima, J.A.S. (2004) Nonsingular FRW Cosmology and Non Linear Dynamics. Arxiv astroph/0402311 Version 1.</mixed-citation></ref><ref id="scirp.85832-ref3"><label>3</label><mixed-citation publication-type="other" xlink:type="simple">Beckwith, A. (2016) Gedanken Experiment for Refining the Unruh Metric Tensor Uncertainty Principle via Schwarzschild Geometry and Planckian Space-Time with Initial Nonzero Entropy and Applying the Riemannian-Penrose Inequality and Initial Kinetic Energy for a Lower Bound to Graviton Mass (Massive Gravity). Journal of High Energy Physics, Gravitation and Cosmology, 2, 106-124.  
&lt;br /&gt;https://doi.org/10.4236/jhepgc.2016.21012</mixed-citation></ref><ref id="scirp.85832-ref4"><label>4</label><mixed-citation publication-type="other" xlink:type="simple">Park, D., Kim, H. and Tamarayan, S. (2002) Nonvanishing Cosmological Constant of Flat Universe in Brane-World Scenario. Physics Letters B, 535, 5-10.  
&lt;br /&gt;https://doi.org/10.1016/S0370-2693(02)01729-X</mixed-citation></ref><ref id="scirp.85832-ref5"><label>5</label><mixed-citation publication-type="other" xlink:type="simple">Ng, Y.J. (2007) Holographic Foam, Dark Energy and Infinite Statistics. Physics Letters B, 657, 10-14. &lt;br /&gt;https://doi.org/10.1016/j.physletb.2007.09.052</mixed-citation></ref><ref id="scirp.85832-ref6"><label>6</label><mixed-citation publication-type="other" xlink:type="simple">Ng, Y.J. (2008) Spacetime Foam: From Entropy and Holography to Infinite Statistics and Nonlocality. Entropy, 10, 441-461. &lt;br /&gt;https://doi.org/10.3390/e10040441</mixed-citation></ref><ref id="scirp.85832-ref7"><label>7</label><mixed-citation publication-type="other" xlink:type="simple">Goldhaber, A. and Nieto, M. (2010) Photon and Graviton Mass Limits. Reviews of Modern Physics, 82, 939-979. &lt;br /&gt;https://doi.org/10.1103/RevModPhys.82.939</mixed-citation></ref><ref id="scirp.85832-ref8"><label>8</label><mixed-citation publication-type="other" xlink:type="simple">Hawkings, S.W. and Ellis, G.F.R. (1973) The Large Scale Structure of Space-Time. Cambridge Monographs on Mathematical Physics. Cambridge University Press, New York. &lt;br /&gt;https://doi.org/10.1017/CBO9780511524646  
&lt;br /&gt;https://drive.google.com/file/d/0B7Wa-F5dVHT7cVk2SHJBOHNHeGM/view</mixed-citation></ref><ref id="scirp.85832-ref9"><label>9</label><mixed-citation publication-type="other" xlink:type="simple">Beckwith, A.W. (2017) How a Minimum Time Step Leads to a Causal Structure Used to Form Initial Entropy Production and High Frequency Gravitons, with 7 Subsequent Open Questions. Journal of High Energy Physics, Gravitation and Cosmology, 3, 493-502. &lt;br /&gt;https://doi.org/10.4236/jhepgc.2017.33038</mixed-citation></ref><ref id="scirp.85832-ref10"><label>10</label><mixed-citation publication-type="other" xlink:type="simple">Padmanabhan, T. (2005) Understanding Our Universe; Current Status, and Open Issues. In: 100 Years of Relativity, Space-Time, Structure: Einstein and Beyond, World Scientific, P.T.E. LTD, Singapore, 175-204.  
&lt;br /&gt;https://doi.org/10.1142/9789812700988_0007</mixed-citation></ref><ref id="scirp.85832-ref11"><label>11</label><mixed-citation publication-type="other" xlink:type="simple">Padmanabhan, T. (2006) An Invitation to Astrophysics. World Scientific Series in Astronomy and Astrophysics: Volume 8. World Press Scientific, Singapore.</mixed-citation></ref><ref id="scirp.85832-ref12"><label>12</label><mixed-citation publication-type="other" xlink:type="simple">Peebles, P.J.E. (1993) Principles of Physical Cosmology. Princeton University Press, Princeton, New Jersey.</mixed-citation></ref><ref id="scirp.85832-ref13"><label>13</label><mixed-citation publication-type="book" xlink:type="simple">Keifer, C. (2012) Can the Arrow of Time Be Understood from Quantum Cosmology?. In: Mersini-Houghton, L and Vaas, R., Eds., The Arrows of Time, A Debate in Cosmology, Fundamental Theories in Physics, Volume 172, Springer Verlag, Heidelberg, 191-203.</mixed-citation></ref><ref id="scirp.85832-ref14"><label>14</label><mixed-citation publication-type="other" xlink:type="simple">Beyer, W. (1986) CRC Standard Mathematical Tables. 28th Edition, Massachusetts, Boston.</mixed-citation></ref><ref id="scirp.85832-ref15"><label>15</label><mixed-citation publication-type="other" xlink:type="simple">Ohanian, H. and Ruffini, R. (1994) Gravitation and Space-Time. 2nd Edition, WW. Norton, New York.</mixed-citation></ref><ref id="scirp.85832-ref16"><label>16</label><mixed-citation publication-type="other" xlink:type="simple">Dowker, F. (2005) Causal Sets and the Deep Structure of Space-Time. 
&lt;br /&gt;https://arxiv.org/abs/gr-qc/0508109</mixed-citation></ref><ref id="scirp.85832-ref17"><label>17</label><mixed-citation publication-type="other" xlink:type="simple">Rovelli, C. and Vidotto, F. (2015) Covariant Loop Quantum Gravity. Cambridge University Press, Cambridge.</mixed-citation></ref><ref id="scirp.85832-ref18"><label>18</label><mixed-citation publication-type="other" xlink:type="simple">Corda, C. and Mosquera Cuesta, H.J. (2011) INFLATON from R2 Gravity: A New Approach Using Nonlinear Electrodynamics. Astroparticle Physics, 34, 587-590.</mixed-citation></ref><ref id="scirp.85832-ref19"><label>19</label><mixed-citation publication-type="other" xlink:type="simple">De Lorenci, V.A., Klippert, R., Novello, M. and Salim, J.M. (2002) Nonlinear Electrodynamics and FRW Cosmology. Physical Review D, 65, Article ID: 063501.</mixed-citation></ref><ref id="scirp.85832-ref20"><label>20</label><mixed-citation publication-type="other" xlink:type="simple">Corda, C. and Mosquera Cuesta, H.J. (2010) Removing Black-Hole Singularities with Nonlinear Electrodynamics. Modern Physics Letters A, 25, 2423-2429.  
&lt;br /&gt;https://arxiv.org/abs/0905.3298  
&lt;br /&gt;https://doi.org/10.1142/S0217732310033633</mixed-citation></ref><ref id="scirp.85832-ref21"><label>21</label><mixed-citation publication-type="other" xlink:type="simple">Penrose, R. (1965) Gravitational Collapse and Space-Time Singularities. Physical Review Letters, 14, 57-59. &lt;br /&gt;https://doi.org/10.1103/PhysRevLett.14.57</mixed-citation></ref><ref id="scirp.85832-ref22"><label>22</label><mixed-citation publication-type="other" xlink:type="simple">Beckwith, A.W. (2017) Reconsidering “Does the Sum Rule Hold at the Big Bang?” with Pre Planckian HUP, and Division Algebras. Journal of High Energy Physics, Gravitation and Cosmology, 3, 539-557.</mixed-citation></ref><ref id="scirp.85832-ref23"><label>23</label><mixed-citation publication-type="other" xlink:type="simple">Crowell, L. (2005) Quantum Fluctuations of Spacetime. World Press Scientific, Singapore. &lt;br /&gt;https://doi.org/10.1142/5952</mixed-citation></ref></ref-list></back></article>