<?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.2013.48A001</article-id><article-id pub-id-type="publisher-id">JMP-36066</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>
 
 
  Scaling and Orbits for an Isotropic Metric
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>oseph</surname><given-names>D. Rudmin</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>College of Integrated Science and Engineering, James Madison University, Harrisonburg, USA</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>rudminjd@jmu.edu</email></corresp></author-notes><pub-date pub-type="epub"><day>20</day><month>08</month><year>2013</year></pub-date><volume>04</volume><issue>08</issue><fpage>1</fpage><lpage>6</lpage><history><date date-type="received"><day>May</day>	<month>26,</month>	<year>2013</year></date><date date-type="rev-recd"><day>June</day>	<month>3,</month>	<year>2013</year>	</date><date date-type="accepted"><day>July</day>	<month>25,</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>
 
 
   Conventional interpretation of the Einstein Equation has inconsistencies and contradictions, such as gravitational fields without energy, objects crossing event-horizons, objects exceeding the speed of light, and inconsistency in scaling the speed of light and its factors. An isotropic metric resolves such problems by attributing energy to the gravitational field, in the Einstein Equation. This paper discusses symmetries of an isotropic metric, including scaling of physical quantities, the Lorentz transformation, covariant derivatives, and stress-energy tensors, and transitivity of this scaling between inertial reference frames. Force, charge, Planck’s constant, and the fine structure constant remain invariant under isotropic gravitational scaling. Gravitational scattering, orbital period, and precession distinguish between isotropic and Schwarzschild metrics. An isotropic metric accommodates quantum mechanics and improves models of black-holes.
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</p></abstract><kwd-group><kwd>Gravitation; Scaling; Orbits; Black Hole Physics; Celestial Mechanics; Relativistic Processes</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>The present interpretation of the Einstein Equation <img src="1-7501391\4b2325f2-4fd7-48c2-9bf1-5787da9d1cef.jpg" /> in general relativity has troubling inconsistencies and contradictions, such as violation of semiclassical locality, quantum unitarity, time reversibility, and energy conservation [<xref ref-type="bibr" rid="scirp.36066-ref1">1</xref>]. For example, when an object crosses a Swarzschild black-hole’s event-horizon, it attains the speed of light, giving the object unbounded energy for nearby observers. Apparently, conservation of energy must be grossly violated, at least for local observers near the event-horizon. Since the Einstein Equation explicitly conserves energy, then the Einstein Equation must not work for local observers. Conventionally, one assumes that the Einstein Equation works only for distant observers, but by their location within the massive cosmos, all physical observers are local observers. So, the present interpretation of the Einstein Equation does not work for any physical observer. Moreover, a rotating black-hole can have a naked singularity, resulting in contradictions of time-travel [<xref ref-type="bibr" rid="scirp.36066-ref2">2</xref>]. Since the conventional model of a black-hole predicts objects to enter a region where the model no longer makes sense, then something must be lacking from the model.</p><p>Since the Einstein Equation is designed to conserve energy, the failure to conserve energy must involve application of the equation, such as the failure to account for the energy density of the gravitational field. When one assembles electric charges on a sphere, one applies a force through a distance on the charges, and thus puts energy into the electric field. For gravity, ordinary mass plays the role of charge. When one assembles a sphere of mass, energy is released. So, a gravitational field should have negative energy density. The Einstein Equation equates<img src="1-7501391\8c151efd-7180-4536-98ea-a256cde650e7.jpg" />, which is a contraction of the curvature tensor for space-time, to<img src="1-7501391\4c2196da-f207-4c13-a429-0910adc1d6a8.jpg" />, which is the local energy and momentum density. The fact that the conventional Schwarzschild metric for a black-hole is derived by solving the differential equations for <img src="1-7501391\bd976951-dfad-40ea-98cf-80870f30f5bd.jpg" /> for all regions around the singularity, implies that the gravitational fields have no energy nor momentum.</p><p>The resulting Schwarzschild metric for a black-hole is anisotropic: While objects in the gravitational well look shorter in a radial direction, their azimuthal dimensions remain unaffected, as viewed by a remote observer. Then, the speed of light is also anisotropic, and one cannot consistently scale mass and energy, and complications arise in reconciling gravity with quantum mechanics. These contradictions and inconsistencies should inspire us to consider a different metric.</p></sec><sec id="s2"><title>2. Isotropic Metric</title><p>An isotropic metric with the scaling for time reciprocal that for space, yields a distance differential<img src="1-7501391\1bd8b2d0-fb6c-4136-a89d-c34f7d01226d.jpg" />, in terms of a distant observer’s coordinates<img src="1-7501391\98e25e0a-6859-423b-af92-1a64ce8613ee.jpg" />:</p><disp-formula id="scirp.36066-formula11803"><label>(1.1)</label><graphic position="anchor" xlink:href="1-7501391\91101a78-2dbe-4c8a-af2a-c0180945cac4.jpg"  xlink:type="simple"/></disp-formula><p>The speed of light as seen from a distance, <img src="1-7501391\10252c39-fdb4-4ed1-adc9-4f293f53ff53.jpg" />, in terms of that locally, <img src="1-7501391\bb6e0a31-4cf1-4746-a464-2bdcc4e6348c.jpg" />, is <img src="1-7501391\70f1d0f5-3235-4f50-a8b9-fb7f2290b918.jpg" />, which means that since<img src="1-7501391\6ca3dfde-3fbf-4b85-b23d-ba4c6f6f57f4.jpg" />, light in a gravitational well moves more slowly. As a result, a gravitational field deflects light. Therefore, this metric is not “conformally flat”. Because the metric is isotropic, objects no longer cross eventhorizons. For example, one can see that in the orbit Equation (1.44) below, for a spherically symmetric potential, <img src="1-7501391\acb9ee1d-b0f3-436d-86ba-0324dfbb3d02.jpg" />is bounded.</p><p>In matrix form for spherical coordinates, this isotropic metric is</p><disp-formula id="scirp.36066-formula11804"><label>(1.2)</label><graphic position="anchor" xlink:href="1-7501391\2d8fcd33-a3af-4e92-84a8-66ece5252241.jpg"  xlink:type="simple"/></disp-formula><p>so that the length differential</p><disp-formula id="scirp.36066-formula11805"><label>(1.3)</label><graphic position="anchor" xlink:href="1-7501391\33052c18-6d6a-4648-9cfb-2d90739b7cf1.jpg"  xlink:type="simple"/></disp-formula><p>is that in Equation (1.1). The <img src="1-7501391\769d8272-3a83-488f-9e2d-1b7fd19f4ee5.jpg" /> term of the Einstein Tensor equals the total energy density. For an isotropic metric, it has two terms, one that has the form of a charge density, and the other that has the form of an energy density of a field [<xref ref-type="bibr" rid="scirp.36066-ref3">3</xref>]:</p><disp-formula id="scirp.36066-formula11806"><label>(1.4)</label><graphic position="anchor" xlink:href="1-7501391\21c32f7d-3915-42fe-a168-23616ee91442.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="1-7501391\6748312f-e4b4-4d53-9f01-48b87e1a9ef4.jpg" /> is the gravitational potential in terms of scale factor<img src="1-7501391\b4742913-19fc-4a07-8042-612e8369a766.jpg" />. One should ascribe the energy density of ordinary matter to the first term of the Einstein Tensor, and the energy density of the gravitational field to the second term. In the course of deriving this form, one finds that the metric scales momentum-energy like it scales space-time. Mass differential</p><disp-formula id="scirp.36066-formula11807"><label>(1.5)</label><graphic position="anchor" xlink:href="1-7501391\7cf7c325-8616-41e2-9a3c-b25aa35dfaeb.jpg"  xlink:type="simple"/></disp-formula><p>corresponds to distance differential <img src="1-7501391\2bbd9a9d-5ad7-4f90-9551-3a2dab327489.jpg" /> in Equation (1.1) above.</p><p>Explicit inclusion of factors of c helps to verify scaling factors of g in these equations. Unlike the isotropic metric in Equation (1.1), isotropic metrics rejected in the past were conformally flat. They also did not include the corresponding relation (1.5) for momentum and energy, nor the energy of gravitational fields in the Einstein Tensor (1.4). While the same isotropic metric by Yilmaz [<xref ref-type="bibr" rid="scirp.36066-ref4">4</xref>] has an implicit globally preferred reference frame due to flawed assumptions ancillary to the form of the metric, the gravitational fields for the metric here have rest frames that vary from point to point, as shown in Equation (1.21) below. Such rest frames are consistent with frame-dragging. The “Parameterized Post-Newtonian” (PPN) parameters for equation (0.1) as defined on pp. 1084-1085 of Gravitation [<xref ref-type="bibr" rid="scirp.36066-ref5">5</xref>] are:<img src="1-7501391\817e186a-a783-4ce4-8a23-1e9e3c3468de.jpg" />.<img src="1-7501391\a5510008-b716-404f-8fdd-c5aea4a3c94b.jpg" />, <img src="1-7501391\54395051-b1fc-4b46-a742-abdf0694433e.jpg" />, <img src="1-7501391\764b2900-a0db-4293-addc-d45af272e4ec.jpg" />, <img src="1-7501391\74663aaa-f09a-491e-a86d-c8c58f179398.jpg" />, <img src="1-7501391\473a3a2b-a6fb-4d4a-b89e-682518e2da4d.jpg" />, <img src="1-7501391\8abfb22c-9097-4544-bf50-f67ec91aaeb9.jpg" />, <img src="1-7501391\284fc7e3-f03d-4fbb-8db3-1fa2d31108cf.jpg" />, <img src="1-7501391\d75f1f49-940e-4875-affa-1cc179a84f07.jpg" />, <img src="1-7501391\afcaa0f7-5cd0-4211-a5f1-6a4073ffbf2e.jpg" />, <img src="1-7501391\b80d25b8-ecbf-45da-98ee-9f2de96234b5.jpg" />, <img src="1-7501391\443b8664-5267-418d-9ebc-810d96892267.jpg" />,<img src="1-7501391\62a3649e-83f3-4b99-a962-975aad5c6287.jpg" />. The nonzero value for <img src="1-7501391\9801a905-197b-426e-a401-b0bcc54955d6.jpg" /> is consistent with the existence of rest frames, although there is no globally preferred frame.</p><p>For a point source without rotation, metric scaling [<xref ref-type="bibr" rid="scirp.36066-ref3">3</xref>]</p><disp-formula id="scirp.36066-formula11808"><label>(1.6)</label><graphic position="anchor" xlink:href="1-7501391\c6bc1ada-a377-487a-939a-98bd20d082e3.jpg"  xlink:type="simple"/></disp-formula><p>Since this scaling appears in the metric as <img src="1-7501391\1b80c2d9-5216-4308-b777-d9d72c46bd3c.jpg" />, it is the same as Schwarzschild metric <img src="1-7501391\ed4b0795-35a4-4adf-a6df-e3a5033343e1.jpg" /> to first order in the gravitational constant<img src="1-7501391\6357e4cb-6a66-4920-a22c-8a0f0b87add2.jpg" />, but differs greatly in the strong field limit. For example, the event-horizon is at <img src="1-7501391\7c8240de-181c-4921-997c-a1737f04c9d3.jpg" /> for an isotropic metric. So, one must look at strong gravitational fields to distinguish between them.</p></sec><sec id="s3"><title>3. Scaling of Physical Quantities</title><p>It would help to consider scaling of physical quantities, to avoid blunders in gravitational scaling, and to identify those quantities that are invariant. Suppose a local observer in a gravitational field measures the distance between events, and a remote observer external to the gravitational field measures the distance between the same two events. In local coordinates,</p><disp-formula id="scirp.36066-formula11809"><label>(1.7)</label><graphic position="anchor" xlink:href="1-7501391\dac071e6-c20f-4fe2-b47f-25ead7ed8ca6.jpg"  xlink:type="simple"/></disp-formula><p>while in remote coordinates,</p><disp-formula id="scirp.36066-formula11810"><label>(1.8)</label><graphic position="anchor" xlink:href="1-7501391\e34e6758-0ac0-4cbc-83c7-6a41039210eb.jpg"  xlink:type="simple"/></disp-formula><p>In terms of remote coordinates, <img src="1-7501391\715090cb-a140-4d1c-af89-086d634b6cec.jpg" />and <img src="1-7501391\76a7e18e-5348-472e-b419-6fe058b46958.jpg" />. These substitutions into Equation (1.7) give the distance differential (1.1) from which one may infer the metric tensor, and calculate the affine connection and Einstein Tensor. Substitution <img src="1-7501391\cedb5eca-16d7-473f-8e87-5cdcbfed8459.jpg" /> into Equation (1.1) yields<img src="1-7501391\43edb2f5-9c86-41af-a6dd-fbed414bfd50.jpg" />, which shows that scaling is transitive for successive reference frames:</p><disp-formula id="scirp.36066-formula11811"><label>(1.9)</label><graphic position="anchor" xlink:href="1-7501391\96a81608-281a-4a66-b95e-90a1fa6844e6.jpg"  xlink:type="simple"/></disp-formula><p>Scale factor <img src="1-7501391\4c11e918-1635-4205-b757-7ada9c12e4ac.jpg" /> grows to values greater than one, toward an attractive gravitational potential<img src="1-7501391\dd8e7d33-6e4f-48b1-a80a-8d1fa9f2bafd.jpg" />. So, <img src="1-7501391\3dc79066-a8d7-4125-9e51-f1498645c17a.jpg" />shows that, as seen by a remote observer, an object in a gravitational well is shorter. For time,<img src="1-7501391\514435d3-150f-4f50-8813-1c7035d331a5.jpg" />; energy,<img src="1-7501391\916efd14-6adc-4a9e-851b-44e73da1c3e2.jpg" />; momentum,<img src="1-7501391\0bcd80bc-d958-4919-8a8a-3d2e93637ae7.jpg" />; energy density<img src="1-7501391\102de5b2-6ead-48de-a957-1e32545b567d.jpg" />; and mass,<img src="1-7501391\e75f94e2-3605-4107-a55c-d3fa9397a158.jpg" />. Force and angular momentum are invariant. So, all observers agree on the value of<img src="1-7501391\d129edd6-eb47-44d0-a975-0995943a436d.jpg" />.</p><p>The gravitational constant scales as<img src="1-7501391\5b91b269-7689-43e4-beaa-f0430221c6a8.jpg" />. To change the scaling of a physical quantity, one can multiply by powers of<img src="1-7501391\67752cdb-6b4f-4451-843c-ca577f17a928.jpg" />. For example, the dimensionless quantity in<img src="1-7501391\597d3846-5601-4228-bbb4-590dae64a3c1.jpg" />,</p><disp-formula id="scirp.36066-formula11812"><label>(1.10)</label><graphic position="anchor" xlink:href="1-7501391\4aea4188-ed2c-404e-9c50-ee4639d5268c.jpg"  xlink:type="simple"/></disp-formula><p>is invariant under scaling. By redistributing powers of<img src="1-7501391\11d6fa6e-6b96-4e09-aa86-e062168bac9d.jpg" />, <img src="1-7501391\ef691879-7248-489a-8331-5aca6d981136.jpg" />is invariant under scaling, and <img src="1-7501391\aebec9fe-4d8a-494a-8396-6cc7f3af9096.jpg" /> scales like energy.</p><p>To preserve the symmetry of the Helmholtz-Maxwell Equations, the electric permittivity <img src="1-7501391\441518b4-ea03-42af-8f15-ea4e160ce402.jpg" /> and magnetic permeability <img src="1-7501391\edabef91-2c1d-48bd-9b3a-5cd52d46f0b6.jpg" /> scale the same way. Then</p><disp-formula id="scirp.36066-formula11813"><label>(1.11)</label><graphic position="anchor" xlink:href="1-7501391\f783ebe2-8cda-43c4-aa16-5749f788178a.jpg"  xlink:type="simple"/></disp-formula><p>shows <img src="1-7501391\b33b70fc-26e8-49ed-9cef-c359c695c1de.jpg" /> and<img src="1-7501391\56bd19e3-b90b-407f-9ad7-a37412a48d94.jpg" />. Energy density of an electromagnetic field,</p><disp-formula id="scirp.36066-formula11814"><label>(1.12)</label><graphic position="anchor" xlink:href="1-7501391\f348babc-6eae-4db2-8886-3cf9974c1b0d.jpg"  xlink:type="simple"/></disp-formula><p>shows that <img src="1-7501391\799a72d1-e7e6-4526-8522-8f66f4390081.jpg" /> and<img src="1-7501391\9f8d4b6d-7754-4549-a005-67bf71e92360.jpg" />. Also, <img src="1-7501391\9d3b370c-af66-482a-8de7-a4f5c343e086.jpg" />shows that electric charge<img src="1-7501391\04b60229-419d-45f4-9be3-87a351a2278b.jpg" />, and fine structure constant <img src="1-7501391\14cc30e7-1669-438a-9bc4-01ab9abcb1af.jpg" /> are invariant.</p></sec><sec id="s4"><title>4. Scaling in a Lorentz Transformation</title><p>Although the metric is Lorentz invariant in the local reference frame, where scaling<img src="1-7501391\65834d50-f42e-4859-884b-f69d952e4f6e.jpg" />, it is not Lorentz invariant for all observers. With proper choice of coordinates, a Lorentz transformation of a vector <img src="1-7501391\5555c20c-3da2-4ddb-a273-4f63b585fe4f.jpg" /> is</p><disp-formula id="scirp.36066-formula11815"><label>(1.13)</label><graphic position="anchor" xlink:href="1-7501391\309f52c6-b121-4034-bfd2-61e15b304797.jpg"  xlink:type="simple"/></disp-formula><p>where the Lorentz scaling is</p><disp-formula id="scirp.36066-formula11816"><label>(1.14)</label><graphic position="anchor" xlink:href="1-7501391\e44d1d4b-2c70-4842-905b-f06c77160838.jpg"  xlink:type="simple"/></disp-formula><p>To simplify display in the rest of this section, dimensions not affected by a Lorentz transformation will not be displayed. Then a Lorentz transformation and its inverse are</p><disp-formula id="scirp.36066-formula11817"><label>(1.15)</label><graphic position="anchor" xlink:href="1-7501391\2667360a-1d61-4d5b-9fbf-14644eb7c199.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.36066-formula11818"><label>(1.16)</label><graphic position="anchor" xlink:href="1-7501391\ea997c3e-ae10-4e64-8492-c871f2a27e45.jpg"  xlink:type="simple"/></disp-formula><p>While the metric is not Lorentz invariant for all observers, the length differential is, when written in the form</p><p><img src="1-7501391\3a1c1829-bf2d-426e-8429-f904ab2a990a.jpg" /><img src="1-7501391\fabbd7f8-7f51-4d5e-8895-1873ec08782f.jpg" />&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;(1.17)</p><p>Insertion of the Lorentz transformation and its inverse shows the Lorentz invariance of the length differential,</p><p><img src="1-7501391\8d33c90f-3b78-4fcd-b074-58315b18dd02.jpg" /><img src="1-7501391\d4e3fd65-682e-4ec2-9010-ce8099213fe1.jpg" /> &#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;(1.18)</p><p>where<img src="1-7501391\609d3a53-dda4-4a62-9ef7-472f902cb148.jpg" />, <img src="1-7501391\5092a8c1-cc7b-4a46-b8c9-c17a147d462b.jpg" />, <img src="1-7501391\97233d93-1d4b-4587-bbcf-f2da2139d647.jpg" />, and <img src="1-7501391\8b8b4440-3fdb-4492-bd68-c6a02dac5258.jpg" /> are all the same Lorentz transformation. Then the Lorentz transformed metric</p><disp-formula id="scirp.36066-formula11819"><label>(1.19)</label><graphic position="anchor" xlink:href="1-7501391\e0c66969-c281-477e-b242-06119f79bc63.jpg"  xlink:type="simple"/></disp-formula><p>is Lorentz invariant. But, in remote coordinates, Equation (1.17) becomes,</p><disp-formula id="scirp.36066-formula11820"><label>(1.20)</label><graphic position="anchor" xlink:href="1-7501391\d219b8dc-518e-45ee-a3a1-f13c3a1c7d89.jpg"  xlink:type="simple"/></disp-formula><p>where in the last step, the scaling transfers from the coordinates to the metric tensor. Insertion of a Lorentz transformation and its inverse, in remote coordinates, shows that the Lorentz transformed metric is</p><disp-formula id="scirp.36066-formula11821"><label>(1.21)</label><graphic position="anchor" xlink:href="1-7501391\ca742a2a-6e5e-4b62-a0d9-91efd1c3bbee.jpg"  xlink:type="simple"/></disp-formula><p>yielding a length differential in expected form in remote coordinates,</p><p><img src="1-7501391\902aaee6-4446-4bfb-aaaf-f41edb06b13d.jpg" /><img src="1-7501391\84c44a17-6a41-49f2-bfc6-33f429934921.jpg" /> &#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;(1.22)</p><p><img src="1-7501391\b9f7c9f4-4ff6-4238-9602-42fb40efaed6.jpg" /></p><p><img src="1-7501391\02016383-19de-4713-abc1-d72a234aefe8.jpg" /><img src="1-7501391\e6bbdf1b-fa6a-410d-8385-10ba15411b50.jpg" /></p><p>Under a Lorentz transformation, the metric loses its isotropy, and acquires off-diagonal terms. Diagonalization generates the Lorentz transformation back to the local rest frame of the gravitational field, where the metric scaling factor <img src="1-7501391\e66c4afc-1046-40df-8c77-2c743fa009e9.jpg" /> appears like an eigenvalue.</p></sec><sec id="s5"><title>5. Scaling in Stress Tensors</title><p>Covariant differentiation of vector<img src="1-7501391\3ed25f3e-241f-4b85-a1d4-cc3e36943d92.jpg" />,</p><disp-formula id="scirp.36066-formula11822"><label>(1.23)</label><graphic position="anchor" xlink:href="1-7501391\4e6413ec-4f73-4445-a478-1e877de8a6c5.jpg"  xlink:type="simple"/></disp-formula><p>takes into account both the change in<img src="1-7501391\58161a13-581f-4b30-aeb5-e25d9711adf4.jpg" />, in<img src="1-7501391\9aa33834-567f-459f-9e36-11e8ac3ae354.jpg" />, and an additional apparent transformation of <img src="1-7501391\dcf4a8d5-1053-4d59-a20b-a50148ca981e.jpg" /> in the curved space, in<img src="1-7501391\f45bedff-c282-4aee-9613-7ef2a4d62296.jpg" />, where the Christoffel symbol for the affine connection is</p><disp-formula id="scirp.36066-formula11823"><label>(1.24)</label><graphic position="anchor" xlink:href="1-7501391\72319467-2c46-4e3d-be1f-369971bda4b5.jpg"  xlink:type="simple"/></disp-formula><p>For example, the covariant derivative in the y-direction of a vector along the <img src="1-7501391\9f60f08a-963d-4817-b5ea-6fb156899c7a.jpg" />-direction is <img src="1-7501391\3bc26943-f76c-4f31-bd27-f0223983b46c.jpg" /> is</p><disp-formula id="scirp.36066-formula11824"><label>(1.25)</label><graphic position="anchor" xlink:href="1-7501391\0eb8cd28-f95e-4cca-bd03-2271f163b1ab.jpg"  xlink:type="simple"/></disp-formula><p>If one divides through by<img src="1-7501391\d11d5695-2fe6-41bc-810c-cbd5a3ddf4fc.jpg" />,</p><disp-formula id="scirp.36066-formula11825"><label>(1.26)</label><graphic position="anchor" xlink:href="1-7501391\e51c6e48-213d-46d0-b0c8-f8012633ab7d.jpg"  xlink:type="simple"/></disp-formula><p>then the equation takes a form where the terms are scaled to the local observer’s coordinates, plus a rotation:</p><disp-formula id="scirp.36066-formula11826"><label>(1.27)</label><graphic position="anchor" xlink:href="1-7501391\8f9454c0-b9bc-4c28-b72d-d279de200f6e.jpg"  xlink:type="simple"/></disp-formula><p>So, covariant differentiation implicitly accounts for scaling.</p><p>Since, in the Dirac Equation, the electromagnetic vector potential couples to fermion momentum and energy, as in<img src="1-7501391\f31d6ad5-5f63-4a70-8b96-125823fcc228.jpg" />, and since charge <img src="1-7501391\df942de5-0860-4cc4-83b8-6a31ec71dbab.jpg" /> is unaffected by scaling, then each component of the vector potential should scale like the operator to which it couples. For example, <img src="1-7501391\0ac68b99-6ae4-4dbd-8990-af368b35506a.jpg" />scales like momentum. The electromagnetic field tensor in covariant form</p><disp-formula id="scirp.36066-formula11827"><label>(1.28)</label><graphic position="anchor" xlink:href="1-7501391\142ed63d-6275-4d1b-bad4-0e4809293408.jpg"  xlink:type="simple"/></disp-formula><p>contravariant form,</p><disp-formula id="scirp.36066-formula11828"><label>(1.29)</label><graphic position="anchor" xlink:href="1-7501391\c066dd25-d606-4e86-bd79-0f06c372fcd3.jpg"  xlink:type="simple"/></disp-formula><p>and mixed form</p><disp-formula id="scirp.36066-formula11829"><label>(1.30)</label><graphic position="anchor" xlink:href="1-7501391\07afe73c-518f-4d29-86df-3b32f599e305.jpg"  xlink:type="simple"/></disp-formula><p>all appear in the electromagnetic stress tensor</p><disp-formula id="scirp.36066-formula11830"><label>(1.31)</label><graphic position="anchor" xlink:href="1-7501391\652d8df4-a703-4c45-a498-416142eff031.jpg"  xlink:type="simple"/></disp-formula><p>If a gravitational field is present, then one should use covariant differentiation, to account for curved space. As shown above, covariant differentiation also accounts for scaling.</p><disp-formula id="scirp.36066-formula11831"><label>(1.32)</label><graphic position="anchor" xlink:href="1-7501391\b59e7f03-ea3d-48ee-a9ab-720012c35260.jpg"  xlink:type="simple"/></disp-formula><p>To preserve the symmetry of Equation (1.28), which suppresses factors of<img src="1-7501391\8ebf2d48-544c-4512-8fef-4a0db7032c48.jpg" />, and to keep scaling consistent for the two terms of<img src="1-7501391\ca9234c1-0e1e-4fa6-86db-be6e8bbef7ed.jpg" />, one can require <img src="1-7501391\4d80bf45-08b7-4f5e-89a1-38b98a6100d9.jpg" /> to couple to<img src="1-7501391\68cd4c4d-e548-4f5f-a43f-bc5c1470706a.jpg" />, instead of the energy operator <img src="1-7501391\33905735-5f51-4ba8-a8aa-fc21e3681451.jpg" /> alone, so that all components of the vector potential scale like momentum. In the same way, any other derivative with respect to time should be divided by a factor of<img src="1-7501391\6ebf78fc-1dbd-445a-a7ac-e04c89726958.jpg" />, to scale it like derivatives with respect to space. Then, <img src="1-7501391\174078cc-5289-4c98-b86b-9e82a1f5d1fa.jpg" />and <img src="1-7501391\514dff52-1483-4bbc-8e36-9e798c4fa50b.jpg" /> for all diagonal components of the metric. Since, <img src="1-7501391\d9870714-f124-4951-8523-e27b1d32740b.jpg" />scales like momentum, then <img src="1-7501391\a2ba05ab-9758-4e79-8527-35e56eabf125.jpg" /> and<img src="1-7501391\94f0d4bc-997f-476b-a2c4-c82c2eced23b.jpg" />. Likewise, since <img src="1-7501391\897ece03-ff91-4518-8e3c-1a4db974652c.jpg" />, then<img src="1-7501391\86470a3d-4a44-4c3d-91cc-b6461eb83f47.jpg" />, and<img src="1-7501391\d61acba5-2e31-466c-b834-d5bf1c0255ad.jpg" />. One should expect <img src="1-7501391\ff373d33-c118-4ef0-9a46-75b3937a7899.jpg" /> to scale like an energy density<img src="1-7501391\0ddeb73b-45bf-46ca-a795-1c0c187cba0a.jpg" />. The scaling for the forms of <img src="1-7501391\15f2acf8-064a-493d-be6d-8fda43b57699.jpg" /> suggest that <img src="1-7501391\12ac865d-8375-4565-ba98-429942fd00a2.jpg" /> scales as<img src="1-7501391\e0448f3e-7e52-4a48-913b-4bcc483d8568.jpg" />. The implicit factors, which are the permitivity <img src="1-7501391\963d300d-40df-47bd-a389-f68a05867119.jpg" /> and permeability<img src="1-7501391\8a48abad-62fe-40ff-9509-fc0aaa8c98f7.jpg" />, scale as<img src="1-7501391\33fa18d7-ddb3-4efb-916a-203d2b0ff136.jpg" />, as shown above in Equation (1.11). Therefore, to get the expected scaling for<img src="1-7501391\5f614c6c-b52a-4565-990e-0cf0e928a080.jpg" />, one should also divide by a factor of<img src="1-7501391\cd64a69f-5d3f-443b-9398-e4de59aa7a01.jpg" />.</p></sec><sec id="s6"><title>6. Orbit Equation for an Isotropic Metric</title><p>Recently, long-lived stars have been found orbiting the black-hole in the center of the Milky Way galaxy, in unexpectedly small orbits [6,7]. Measurement of the precession of orbits might make it possible to distinguish between a Schwarzschild metric and an isotropic metric, especially if one can observe an orbit smaller than the Schwarzschild radius. Furthermore, for an isotropic metric, non-decaying orbits exist at all distances from a black-hole.</p><p>As usual, equations of motion are</p><disp-formula id="scirp.36066-formula11832"><label>(1.33)</label><graphic position="anchor" xlink:href="1-7501391\4d002c63-3a72-46c9-a12c-0e388cba9248.jpg"  xlink:type="simple"/></disp-formula><p>For <img src="1-7501391\229846f8-094a-498b-a441-01cb8a319cbb.jpg" /> in Equation (1.33),</p><disp-formula id="scirp.36066-formula11833"><label>(1.34)</label><graphic position="anchor" xlink:href="1-7501391\fa722fc7-6d7a-462c-8c67-8dac6bc2f67a.jpg"  xlink:type="simple"/></disp-formula><p>Integration yields a constant of motion</p><disp-formula id="scirp.36066-formula11834"><label>(1.35)</label><graphic position="anchor" xlink:href="1-7501391\604bbe77-08ab-4377-a40b-d2f1a6fbacf8.jpg"  xlink:type="simple"/></disp-formula><p>This scaling might seem to contradict <img src="1-7501391\775c45a3-db52-41cc-92cd-17c11d255688.jpg" /> evident in (1.1), but the scaling in (1.35) describes a curved orbit, while that in (1.1) describes a straight-line distance. From (1.1),</p><disp-formula id="scirp.36066-formula11835"><label>(1.36)</label><graphic position="anchor" xlink:href="1-7501391\6a95c8eb-c56c-4f3e-ad38-633f5ae64c28.jpg"  xlink:type="simple"/></disp-formula><p>Substitution of this <img src="1-7501391\d9d3791b-e55e-4bae-8efb-011100c852f5.jpg" /> into (1.35) shows that along an orbit,</p><disp-formula id="scirp.36066-formula11836"><label>(1.37)</label><graphic position="anchor" xlink:href="1-7501391\a7ce52e1-6a1c-4f10-a285-d554c7edf09e.jpg"  xlink:type="simple"/></disp-formula><p>Special and general relativistic effects have the same magnitude. The orbiter’s energy and the remote observer’s metric determine constant of motion<img src="1-7501391\211a06ee-bb2f-4153-b1de-4273df777bfc.jpg" />.</p><p>Application of Equation (1.33) to<img src="1-7501391\243dac14-dee0-4ffa-812b-13d06059c2ec.jpg" />, the polar angle, yields</p><disp-formula id="scirp.36066-formula11837"><label>(1.38)</label><graphic position="anchor" xlink:href="1-7501391\3f6a966a-2408-4904-996e-d3c16d722dcd.jpg"  xlink:type="simple"/></disp-formula><p>With choice of coordinates such that<img src="1-7501391\de7b0154-727b-4272-a730-7e79874b1bcf.jpg" />, this equation integrates to a constant of motion that is the angular momentum,</p><disp-formula id="scirp.36066-formula11838"><label>(1.39)</label><graphic position="anchor" xlink:href="1-7501391\6a97cca5-d95f-4f9d-9e45-4984da498dc8.jpg"  xlink:type="simple"/></disp-formula><p>Again, scaling for this constant is reconciled to invariant angular momentum,</p><disp-formula id="scirp.36066-formula11839"><label>(1.40)</label><graphic position="anchor" xlink:href="1-7501391\b3d5e15b-2471-4285-8419-d14695f599a8.jpg"  xlink:type="simple"/></disp-formula><p>by substitution<img src="1-7501391\c56121a0-b6f4-4205-80f9-53e5a1b98894.jpg" />. While all observers agree on the angular momentum of a particle, the contribution of the particle to the total angular momentum varies over its orbit, since its rest mass does not change while it traverses different values of the metric.</p><p>For <img src="1-7501391\d6aa6dc8-b032-4a6a-a8e8-818da13ccccb.jpg" /> in Equation (1.33),</p><disp-formula id="scirp.36066-formula11840"><label>(1.41)</label><graphic position="anchor" xlink:href="1-7501391\c6d0efaa-c33a-4ed6-8e67-a124968b157f.jpg"  xlink:type="simple"/></disp-formula><p>which reduces to</p><disp-formula id="scirp.36066-formula11841"><label>(1.42)</label><graphic position="anchor" xlink:href="1-7501391\6f618857-6930-4757-836a-0345a5441cac.jpg"  xlink:type="simple"/></disp-formula><p>Integration of this equation gives</p><disp-formula id="scirp.36066-formula11842"><label>(1.43)</label><graphic position="anchor" xlink:href="1-7501391\4ef8d169-705e-43d9-9443-89a6368b151d.jpg"  xlink:type="simple"/></disp-formula><p>where</p><disp-formula id="scirp.36066-formula11843"><label>(1.44)</label><graphic position="anchor" xlink:href="1-7501391\beb620ea-f1d1-444e-82ba-9d8e02e3c508.jpg"  xlink:type="simple"/></disp-formula><p>which is an expansion of Equation (1.37),<img src="1-7501391\b98a6179-32ba-41c6-9b75-1bb41153ac11.jpg" />. At sufficiently small<img src="1-7501391\9ea8509d-078b-4630-927f-efd4892802cf.jpg" />, the negative terms of Equation (1.44) make<img src="1-7501391\5325731b-eeca-4e18-b361-3e2bbbad6839.jpg" />. Unlike the Schwarzschild metric, stable orbits exist at all radii for an isotropic metric. Multiplication of Equation (1.43) by <img src="1-7501391\f7da22fe-d8b7-43d0-9025-db8ea475b7a9.jpg" /> gives an effective potential in the Newtonian approximation.</p><disp-formula id="scirp.36066-formula11844"><label>(1.45)</label><graphic position="anchor" xlink:href="1-7501391\0d7a037f-867f-4c61-a0eb-ed0aa0045154.jpg"  xlink:type="simple"/></disp-formula><p>to first order in<img src="1-7501391\e12e755f-53be-423c-aedd-73d5961a15d3.jpg" />. The last term comes from the harmonic expansion</p><disp-formula id="scirp.36066-formula11845"><label>(1.46)</label><graphic position="anchor" xlink:href="1-7501391\fc7ac0ce-72a7-49a1-9001-9bcbf66bb3f4.jpg"  xlink:type="simple"/></disp-formula><p>Expansion (1.45) first differs from that for a Schwarzschild metric in the factor of two on the last term. So, correction to the orbital period for an isotropic metric is twice that for a Schwarzschild metric. Since, <img src="1-7501391\e165ce97-48d5-4e9f-a5c0-57aa5177d51c.jpg" />,</p><disp-formula id="scirp.36066-formula11846"><label>(1.47)</label><graphic position="anchor" xlink:href="1-7501391\337c4b21-07d7-4cf9-aa91-5e1ac74e8c12.jpg"  xlink:type="simple"/></disp-formula><p>which then yields</p><disp-formula id="scirp.36066-formula11847"><label>(1.48)</label><graphic position="anchor" xlink:href="1-7501391\c040865b-71c1-4e7b-ad92-5036b54cf94f.jpg"  xlink:type="simple"/></disp-formula><p>The ratio <img src="1-7501391\bee1b43c-277f-4f33-969c-ab61e74dfeb9.jpg" /> from Equations (1.39) and (1.44) gives the orbit equation</p><disp-formula id="scirp.36066-formula11848"><label>(1.49)</label><graphic position="anchor" xlink:href="1-7501391\64f932fd-92a6-44d2-93bf-a9e6a05fd372.jpg"  xlink:type="simple"/></disp-formula><p>With expansion to <img src="1-7501391\510d851c-8229-4023-8dc3-31c16143e83d.jpg" /> of powers of <img src="1-7501391\a9f9f248-572f-4675-a723-898945baf6c4.jpg" />, Equation (1.49) becomes</p><disp-formula id="scirp.36066-formula11849"><label>(1.50)</label><graphic position="anchor" xlink:href="1-7501391\ae34456e-9056-4612-894a-8f6cff1c1cc5.jpg"  xlink:type="simple"/></disp-formula><p>For the Newtonian approximation, <img src="1-7501391\1e1cd286-93cb-4908-a40e-4b25c99e9601.jpg" />, where<img src="1-7501391\3c6ee193-f660-4a58-bff9-154c92d74f2e.jpg" />, <img src="1-7501391\78606bcd-b9f6-4db2-ab4c-0975468c6ed6.jpg" />, and<img src="1-7501391\77bb8902-c56a-44f4-8f1e-dacd09dcaa7d.jpg" />, are constants to be determined,</p><disp-formula id="scirp.36066-formula11850"><label>(1.51)</label><graphic position="anchor" xlink:href="1-7501391\ee16716f-2440-4b42-91d9-6e1bad513661.jpg"  xlink:type="simple"/></disp-formula><p>Comparison of the above two equations shows that<img src="1-7501391\4c73d5bc-8e32-4f8c-bb7b-bf7c457e6f6c.jpg" />. The precession <img src="1-7501391\37fadc15-8c2a-42f7-a704-63b1e9978942.jpg" /> is 50% larger than that given for a Schwarzschild metric. The comparison would be complicated by rotation of the gravitational field.</p><p>For scattering,<img src="1-7501391\053534a6-dc83-449c-85c6-0a8910986fd7.jpg" />. For a massless particle at this limit, <img src="1-7501391\658e066f-e653-4000-850c-8f97547183a2.jpg" />, because g is one; and <img src="1-7501391\343f5df3-f7e1-4da2-9035-24153f1f0ac5.jpg" />, where <img src="1-7501391\1e679231-b660-4716-ad53-9132792104b6.jpg" /> is the impact parameter and <img src="1-7501391\3d8bcf14-7174-4094-a394-63308c4da561.jpg" /> is the initial speed. For a small deflection, in this limit,<img src="1-7501391\af68c931-2f9c-4f3b-8603-d78d04dc09a8.jpg" />.</p><disp-formula id="scirp.36066-formula11851"><label>(1.52)</label><graphic position="anchor" xlink:href="1-7501391\b3a4f268-165f-4d02-b0e5-7b03e4196f9c.jpg"  xlink:type="simple"/></disp-formula><p>for an isotropic metric, versus</p><disp-formula id="scirp.36066-formula11852"><label>(1.53)</label><graphic position="anchor" xlink:href="1-7501391\b972b44e-497d-4d73-acd1-d17746196f50.jpg"  xlink:type="simple"/></disp-formula><p>for a Schwarzschild metric.</p></sec><sec id="s7"><title>7. Inconsistency for a Schwarzschild Metric</title><p>The Schwarzschild metric has inherent inconsistencies, mostly due to neglecting to scale the speed of light. For the Schwarzschild metric,</p><disp-formula id="scirp.36066-formula11853"><label>(1.54)</label><graphic position="anchor" xlink:href="1-7501391\8de60751-a931-464b-b4f4-35890d0666e8.jpg"  xlink:type="simple"/></disp-formula><p>As already explained, primed quantities are distant measures, while unprimed are local measures. For a point source, the Schwarzschild metric scaling</p><disp-formula id="scirp.36066-formula11854"><label>(1.55)</label><graphic position="anchor" xlink:href="1-7501391\a9085320-a63c-428d-a751-844bede974f7.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="1-7501391\171c1bf2-f0a4-4869-baed-21d9f7989fc9.jpg" /> is one. The standard interpretation assumes that all observers agree on the metric. Therefore</p><disp-formula id="scirp.36066-formula11855"><label>(1.56)</label><graphic position="anchor" xlink:href="1-7501391\1d1a716f-a778-4777-a7cb-46c8375672d3.jpg"  xlink:type="simple"/></disp-formula><p>To relate the gravitational potential energy of a system, as measured locally, to that measured remotely, suppose, as an ansatz, that energy scales as</p><disp-formula id="scirp.36066-formula11856"><label>(1.57)</label><graphic position="anchor" xlink:href="1-7501391\a772bbed-8ff9-4e75-9ddc-374f80a85e36.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="1-7501391\129a41a8-48c7-4287-8fbe-c7cbc7cb0095.jpg" /> is yet to be determined. Then</p><disp-formula id="scirp.36066-formula11857"><label>(1.58)</label><graphic position="anchor" xlink:href="1-7501391\abac78f1-c412-4e69-8fa4-95ca10b13711.jpg"  xlink:type="simple"/></disp-formula><p>With the scaling for <img src="1-7501391\0df7a39d-1ff5-42d7-9023-d83cafca824e.jpg" /> for radial motion,</p><disp-formula id="scirp.36066-formula11858"><label>(1.59)</label><graphic position="anchor" xlink:href="1-7501391\dfb5c3d4-a9f2-4ad2-80a1-88ec6a91c0a8.jpg"  xlink:type="simple"/></disp-formula><p>With scaling for <img src="1-7501391\e58fe7c0-906c-49dc-8a3f-0e3ee647935a.jpg" /> for azimuthal motion,</p><disp-formula id="scirp.36066-formula11859"><label>(1.60)</label><graphic position="anchor" xlink:href="1-7501391\35f37739-f452-429d-9441-fbc5d19a89fa.jpg"  xlink:type="simple"/></disp-formula><p>Substitution for <img src="1-7501391\167c3e50-0248-41c1-a464-2cfb372a034c.jpg" /> into Equation (1.58), from Equation (1.59) yields</p><disp-formula id="scirp.36066-formula11860"><label>(1.61)</label><graphic position="anchor" xlink:href="1-7501391\6fc592b9-ecd4-4a49-a87b-194677d7464f.jpg"  xlink:type="simple"/></disp-formula><p>Then substitution into Equation (1.56) shows that gravitational potential energy scales as</p><disp-formula id="scirp.36066-formula11861"><label>(1.62)</label><graphic position="anchor" xlink:href="1-7501391\f1ab4757-d259-44a7-a614-cbc5df8215f3.jpg"  xlink:type="simple"/></disp-formula><p>The scaling of this gravitational energy contradicts that in Equation (1.57). The scaling for <img src="1-7501391\427b179e-4bd2-4c57-b19b-d9abffb6f794.jpg" /> in Equation (1.60) has the same problem. Therefore the Schwarzschild metric implies a preferred remote frame of reference in which physics is self-consistent; one cannot use potentials to conserve momentum and energy in any physical reference frame. In contrast, an isotropic metric has selfconsistency across all inertial frames of reference, as shown by Equation (1.9).</p></sec><sec id="s8"><title>8. Conclusion</title><p>That an isotropic metric accounts for the energy of a gravitational field, should be sufficient reason to adopt an isotropic metric over a Schwarzschild metric. Further reason is provided by the symmetries of scaling for an isotropic metric, such as that between the length differential and the mass-energy-momentum equation. The invariance under isotropic scaling of force, angular momentum, electric field, electric charge, and fine structure constant provide consistency of general relativity with both quantum mechanics and electromagnetism. Orbits no longer cross event horizons. Inconsistencies in scaling for a Schwarzschild metric make the Schwarzschild metric untenable, necessitating adoption of the isotropic metric.</p></sec><sec id="s9"><title>9. Acknowledgements</title><p>The author thanks his parents, his brother David Rudmin, and George Gillies for proofreading and encouragement.</p></sec><sec id="s10"><title>REFERENCES</title></sec></body><back><ref-list><title>References</title><ref id="scirp.36066-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">S. B. Giddings, Physics Today, Vol. 66, 2013, pp. 30-35. 
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