<?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.2015.610146</article-id><article-id pub-id-type="publisher-id">JMP-59227</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>
 
 
  Temperature Structure of Compact Objects
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>ukio</surname><given-names>Tomozawa</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, University of Michigan, Ann Arbor, USA</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>tomozawa@umich.edu</email></corresp></author-notes><pub-date pub-type="epub"><day>28</day><month>08</month><year>2015</year></pub-date><volume>06</volume><issue>10</issue><fpage>1412</fpage><lpage>1420</lpage><history><date date-type="received"><day>11</day>	<month>June</month>	<year>2015</year></date><date date-type="rev-recd"><day>accepted</day>	<month>25</month>	<year>August</year>	</date><date date-type="accepted"><day>28</day>	<month>August</month>	<year>2015</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>
 
 
  Based on the physical metric proposed by the author, temperature distribution for compact objects, neutron stars and black holes, has been explained. Outside the extended horizon, the temperature is positive and approaches infinity at the extended horizon boundary. Inside the extended horizon, the temperature is negative which implies higher temperature than outside the horizon. This outcome is the result of the repulsive nature of gravity inside the extended horizon in the author’s physical metric. Overall, the physical metric explains temperature structure of compact objects more completely than the Schwarzschild metric, and is supported by the emerging evidence of X-ray data collected from neutron stars and black holes (AGN).
 
</p></abstract><kwd-group><kwd>Physical Metric</kwd><kwd> Extended Horizon</kwd><kwd> Compact Objects</kwd><kwd> Neutron Stars</kwd><kwd> Black Holes</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>The physical metric has been introduced by the author [<xref ref-type="bibr" rid="scirp.59227-ref1">1</xref>] [<xref ref-type="bibr" rid="scirp.59227-ref2">2</xref>] as the metric in general relativity which fits all the experimental data, in particular, time delay experiments of Shapiro et al. [<xref ref-type="bibr" rid="scirp.59227-ref3">3</xref>] [<xref ref-type="bibr" rid="scirp.59227-ref4">4</xref>] . It is a metric in which the speed of light on the spherical direction is unchanged from that in vacuum. Since the spherical direction is perpendi- cular to the radial direction of gravity, it is remarkable that the invariance of the speed of light in the spherical direction from the vacuum value is required for reconciling with the experimental data. In other words, such a natural condition is set up on the basis of general relativity. It will be shown that the physical metric requires a dramatic change in the way that we understand gravity for compact objects. In Section 2, the physical metric is reviewed. The temperature distribution has been described for non-rotating system in Section 3. This is extended to rotating system in Section 4. This introduces a high temperature environment for compact objects. The observational evidence for both neutron stars and black holes are emerging and they are discussed in Section 5. Section 6 presents the author’s summary and discussion.</p></sec><sec id="s2"><title>2. The Physical Metric and the Extended Horizon</title><p>In the spherical symmetric and static (SSS) metric of general relativity,</p><disp-formula id="scirp.59227-formula1135"><label>(1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x5.png"  xlink:type="simple"/></disp-formula><p>the physical metric is defined as</p><disp-formula id="scirp.59227-formula1136"><label>(2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x6.png"  xlink:type="simple"/></disp-formula><p>In other words, the speed of light in the spherical direction that is perpendicular to the radial direction of gravity is unchanged from the vacuum value. It is remarkable that such a condition is required to fit the experi- mental data for general relativity test. In the original formulation of Schwarzschild metric [<xref ref-type="bibr" rid="scirp.59227-ref5">5</xref>] , he proceeded to require that the determinant of modification of the metric to be unity,</p><disp-formula id="scirp.59227-formula1137"><label>(3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x7.png"  xlink:type="simple"/></disp-formula><p>In order to get the physical metric, one has to get the Schwarzschild metric after the coordinate transformation</p><disp-formula id="scirp.59227-formula1138"><label>(4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x8.png"  xlink:type="simple"/></disp-formula><p>which implies that</p><disp-formula id="scirp.59227-formula1139"><label>(5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x9.png"  xlink:type="simple"/></disp-formula><p>where</p><disp-formula id="scirp.59227-formula1140"><label>(6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x10.png"  xlink:type="simple"/></disp-formula><p>is the Schwarzschild radius for mass M. Then one gets</p><disp-formula id="scirp.59227-formula1141"><label>(7)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x11.png"  xlink:type="simple"/></disp-formula><p>For positive value of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502307x12.png" xlink:type="simple"/></inline-formula>, the value of r is restricted to</p><disp-formula id="scirp.59227-formula1142"><label>(8)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x13.png"  xlink:type="simple"/></disp-formula><p>and we restrict the range of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502307x14.png" xlink:type="simple"/></inline-formula> to be</p><disp-formula id="scirp.59227-formula1143"><label>(9)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x15.png"  xlink:type="simple"/></disp-formula><p>From Equation (7), one gets</p><disp-formula id="scirp.59227-formula1144"><label>(10)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x16.png"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.59227-formula1145"><label>(11)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x17.png"  xlink:type="simple"/></disp-formula><p>In order to extend the solution for the physical metric beyond Equation (8), one uses the non-asymptotic solution,</p><disp-formula id="scirp.59227-formula1146"><label>(12)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x18.png"  xlink:type="simple"/></disp-formula><p>for</p><disp-formula id="scirp.59227-formula1147"><label>(13)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x19.png"  xlink:type="simple"/></disp-formula><p>Then one gets</p><disp-formula id="scirp.59227-formula1148"><label>(14)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x20.png"  xlink:type="simple"/></disp-formula><p>The continuity of Equation (7) and Equation (14) at the boundary yields</p><disp-formula id="scirp.59227-formula1149"><label>(15)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x21.png"  xlink:type="simple"/></disp-formula><p>Differentiating Equation (14), one gets</p><disp-formula id="scirp.59227-formula1150"><label>(16)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x22.png"  xlink:type="simple"/></disp-formula><p>Then one gets</p><disp-formula id="scirp.59227-formula1151"><label>(17)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x23.png"  xlink:type="simple"/></disp-formula><p>Choosing the parameter space in Equation (15)</p><disp-formula id="scirp.59227-formula1152"><label>(18)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x24.png"  xlink:type="simple"/></disp-formula><p>all metric functions are positive definite. With the choice of these parameter ranges, the speed of light are well defined throughout all the space time points. This is very different from the Schwarzschild metric. It is remark- able that only such a natural metric fits the experimental data, as was stated earlier.</p><p><xref ref-type="fig" rid="fig1">Figure 1</xref> describes the metric function, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502307x25.png" xlink:type="simple"/></inline-formula>, for the whole region of r.</p><p>The distance r can be reached at zero when <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502307x26.png" xlink:type="simple"/></inline-formula> reaches<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502307x26.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502307x27.png" xlink:type="simple"/></inline-formula>, as</p><disp-formula id="scirp.59227-formula1153"><label>(19)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x28.png"  xlink:type="simple"/></disp-formula><p>One may note that there is an undecided one parameter which can be fixed from the physics inside the dis- tance at</p><fig id="fig1"  position="float"><label><xref ref-type="fig" rid="fig1">Figure 1</xref></label><caption><title> The metric function, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502307x30.png" xlink:type="simple"/></inline-formula>(y-axis), as a func- tion of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502307x30.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502307x31.png" xlink:type="simple"/></inline-formula> (x-axis) in the SSS physical metric</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/4-7502307x29.png"/></fig><disp-formula id="scirp.59227-formula1154"><label>(20)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x32.png"  xlink:type="simple"/></disp-formula><p>At<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502307x33.png" xlink:type="simple"/></inline-formula>,</p><disp-formula id="scirp.59227-formula1155"><label>(21)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x34.png"  xlink:type="simple"/></disp-formula><p>and from Equation (10)</p><disp-formula id="scirp.59227-formula1156"><label>(22)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x35.png"  xlink:type="simple"/></disp-formula><p>and hence <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502307x36.png" xlink:type="simple"/></inline-formula> is called the extended horizon and defines the size of compact objects. This defines the size of neutron stars as well as black holes. In fact, the size of a neutron star of mass, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502307x36.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502307x37.png" xlink:type="simple"/></inline-formula>, is very close to the extended horizon</p><disp-formula id="scirp.59227-formula1157"><label>(23)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x38.png"  xlink:type="simple"/></disp-formula><p>From <xref ref-type="fig" rid="fig1">Figure 1</xref>, as well as from Equation (10) and Equation (16), one can see that the gravity outside/inside the extended horizon is attractive/repulsive or the derivative of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502307x39.png" xlink:type="simple"/></inline-formula> is positive/negative. This is an impor- tant relevance to the temperature structure of compact objects, as will be seen from the following sections.</p></sec><sec id="s3"><title>3. Temperature Distribution for Non-Rotating Compact Objects</title><p>The temperature of compact objects can be calculated as the extension of the Hawking temperature</p><disp-formula id="scirp.59227-formula1158"><label>(24)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x40.png"  xlink:type="simple"/></disp-formula><p>for the outside of the extended horizon. This has the same structure as the Hawking temperature, since it is inversely proportional to the distance. The only difference is that the coefficient becomes infinitely large for <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502307x41.png" xlink:type="simple"/></inline-formula> or at the extended horizon. In order to see the variation of the temperature as a function of the distance from the extended horizon, one expands r and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502307x41.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502307x42.png" xlink:type="simple"/></inline-formula> as</p><disp-formula id="scirp.59227-formula1159"><label>(25)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x43.png"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.59227-formula1160"><label>(26)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x44.png"  xlink:type="simple"/></disp-formula><p>where</p><disp-formula id="scirp.59227-formula1161"><label>(27)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x45.png"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.59227-formula1162"><label>(28)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x46.png"  xlink:type="simple"/></disp-formula><p>Using Equation (7), one gets</p><disp-formula id="scirp.59227-formula1163"><label>(29)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x47.png"  xlink:type="simple"/></disp-formula><p>and the expansion of Equation (24) yields</p><disp-formula id="scirp.59227-formula1164"><label>(30)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x48.png"  xlink:type="simple"/></disp-formula><p>For</p><disp-formula id="scirp.59227-formula1165"><label>(31)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x49.png"  xlink:type="simple"/></disp-formula><p>and then</p><disp-formula id="scirp.59227-formula1166"><label>(32)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x50.png"  xlink:type="simple"/></disp-formula><p>the temperature becoms infinitely large towards the extended horizon.</p><p>Using the conversion formula (for<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502307x51.png" xlink:type="simple"/></inline-formula>)</p><disp-formula id="scirp.59227-formula1167"><label>(33)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x52.png"  xlink:type="simple"/></disp-formula><p>the 1 keV temperature corresponds to</p><disp-formula id="scirp.59227-formula1168"><label>, (34)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x54.png"  xlink:type="simple"/></disp-formula><p>then the location of 1 keV is</p><disp-formula id="scirp.59227-formula1169"><label>(35)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x55.png"  xlink:type="simple"/></disp-formula><p>Then, for the value of Equation (23), one gets</p><disp-formula id="scirp.59227-formula1170"><label>(36)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x56.png"  xlink:type="simple"/></disp-formula><p>or</p><disp-formula id="scirp.59227-formula1171"><label>(37)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x57.png"  xlink:type="simple"/></disp-formula><p>and hence</p><disp-formula id="scirp.59227-formula1172"><label>(38)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x58.png"  xlink:type="simple"/></disp-formula><p>This small value of the high temperature thickness makes the observation from this thin layer very unlikely, even by using high density of neutron star (~10<sup>39</sup> neutrons/cm<sup>3</sup>).</p><p>Inside the extended horizon, the expression for the temperature becomes</p><disp-formula id="scirp.59227-formula1173"><label>(39)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x59.png"  xlink:type="simple"/></disp-formula><p>where Equation (16) has been used. Since</p><disp-formula id="scirp.59227-formula1174"><label>(40)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x60.png"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.59227-formula1175"><label>(41)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x61.png"  xlink:type="simple"/></disp-formula><p>the temperature in Equation (39) is negative definite. In other words, the temperature inside the extended horizon is negative. A negative temperature is a temperature higher than any positive temperature, since high energy states are more abundant than lower energy states [<xref ref-type="bibr" rid="scirp.59227-ref6">6</xref>] . Notice that the Boltzman statistcal factor, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502307x62.png" xlink:type="simple"/></inline-formula>, is larger for higher energy than that for lower energy for a negative temperature.</p><p>The matter inside the extended horizon is in a higher temperature environment. However any phenomena in a deep inside region is not exposed to outside observers. However the matter near the extended horizon is subject to an oscillation between the attractive force outside the extended horizon and the repulsive force inside the extended horizon. One notices that the outside layer is thin, since the attractive force at the extended horizon is infinitely large. Any phenomena of the oscillating matter through the extended horizon is subject to the observation of the outside observers. The X-ray emission from highly ionized atoms of a neutron density in 1 cm thickness can be observed from the edge of the Milky Way.</p><p>For AGN or massive black holes with higher mass, the density is reduced by 1/M<sup>2</sup>, but the surface area is increased by M<sup>2</sup>. Hence the number of events are independent on mass. Only the difference is the distance to the events from the observers on the Earth. So the events from the nearer AGN are more likely observable. Of course, the radiation of lower frequency can be more observable, since the depth of the radiation is increased with the wave length. The recent report [<xref ref-type="bibr" rid="scirp.59227-ref7">7</xref>] of the most luminous galaxy observed by WISE at z &gt; 3 might be related with high temperature nature of AGN in this section.</p></sec><sec id="s4"><title>4. Temperature Distribution of Rotating Compact Objects</title><p>The metric for a mass with rotation is expressed as [<xref ref-type="bibr" rid="scirp.59227-ref8">8</xref>]</p><disp-formula id="scirp.59227-formula1176"><label>(42)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x63.png"  xlink:type="simple"/></disp-formula><p>where the metric functions, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502307x64.png" xlink:type="simple"/></inline-formula>, is constructed from the Boyer-Lindquist representation of the Kerr metric by the coordinate transformation,</p><disp-formula id="scirp.59227-formula1177"><label>(43)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x65.png"  xlink:type="simple"/></disp-formula><p>in order to accommodate to the physical metric in the limit of no rotation. For the asymptotic region</p><disp-formula id="scirp.59227-formula1178"><label>(44)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x66.png"  xlink:type="simple"/></disp-formula><p>or outside of the extended horizon, one gets</p><disp-formula id="scirp.59227-formula1179"><label>(45)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x67.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.59227-formula1180"><label>(46)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x68.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.59227-formula1181"><label>(47)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x69.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.59227-formula1182"><label>(48)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x70.png"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.59227-formula1183"><label>(49)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x71.png"  xlink:type="simple"/></disp-formula><p>where a is the angular momentum per mass. Here, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502307x72.png" xlink:type="simple"/></inline-formula>was introduced in the discussion of the physical metric,</p><disp-formula id="scirp.59227-formula1184"><label>(50)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x73.png"  xlink:type="simple"/></disp-formula><p>in Equation (18). In the limit of</p><disp-formula id="scirp.59227-formula1185"><label>(51)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x74.png"  xlink:type="simple"/></disp-formula><p>these metric functions coincide with the physical metric in Section 2.</p><p>In order to find the gravitational force implied by this Kerr metric, let us compute<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502307x75.png" xlink:type="simple"/></inline-formula>,</p><disp-formula id="scirp.59227-formula1186"><label>(52)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x76.png"  xlink:type="simple"/></disp-formula><p>Here</p><disp-formula id="scirp.59227-formula1187"><label>(53)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x77.png"  xlink:type="simple"/></disp-formula><p>becomes positive infinity at the extended horizon. For a uniform distribution of the density, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502307x78.png" xlink:type="simple"/></inline-formula>, and uniform rotation speed, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502307x78.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502307x79.png" xlink:type="simple"/></inline-formula>, one gets</p><disp-formula id="scirp.59227-formula1188"><label>(54)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x80.png"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.59227-formula1189"><label>(55)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x81.png"  xlink:type="simple"/></disp-formula><p>Using</p><disp-formula id="scirp.59227-formula1190"><label>(56)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x82.png"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.59227-formula1191"><label>(57)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x83.png"  xlink:type="simple"/></disp-formula><p>one gets</p><disp-formula id="scirp.59227-formula1192"><label>(58)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x84.png"  xlink:type="simple"/></disp-formula><p>For<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502307x85.png" xlink:type="simple"/></inline-formula>, using Equation (23) and Equation (56) one gets</p><disp-formula id="scirp.59227-formula1193"><label>(59)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x86.png"  xlink:type="simple"/></disp-formula><p>or</p><disp-formula id="scirp.59227-formula1194"><label>(60)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x87.png"  xlink:type="simple"/></disp-formula><p>Notice that the fastest rotation observed [<xref ref-type="bibr" rid="scirp.59227-ref9">9</xref>] of neutron star is 716 Hz for PSR J1748-2446 and the effect of the rotation of neutron stars are limitted by</p><disp-formula id="scirp.59227-formula1195"><label>(61)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x88.png"  xlink:type="simple"/></disp-formula><p>Expanding all quantities in this section for a small value of a and making the angular averages</p><disp-formula id="scirp.59227-formula1196"><label>(62)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x89.png"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.59227-formula1197"><label>(63)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x90.png"  xlink:type="simple"/></disp-formula><p>or more generally</p><disp-formula id="scirp.59227-formula1198"><label>(64)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x91.png"  xlink:type="simple"/></disp-formula><p>one gets</p><disp-formula id="scirp.59227-formula1199"><label>(65)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x92.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.59227-formula1200"><label>(66)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x93.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.59227-formula1201"><label>(67)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x94.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.59227-formula1202"><label>(68)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x95.png"  xlink:type="simple"/></disp-formula><p>For Equation (52), using the expansion, Equation (25) and Equation (26), one can get</p><disp-formula id="scirp.59227-formula1203"><label>(69)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x96.png"  xlink:type="simple"/></disp-formula><p>which reproduces the temperature structure of non-rotating compact objects for outside the extended horizon, with small variation of the rotation effects.</p><p>For the temperature structure inside the extended horizon, one may use the Kerr metric for the internal solution of the physical metric,</p><disp-formula id="scirp.59227-formula1204"><label>(70)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x97.png"  xlink:type="simple"/></disp-formula><p>where</p><disp-formula id="scirp.59227-formula1205"><label>(71)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x98.png"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.59227-formula1206"><label>(72)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x99.png"  xlink:type="simple"/></disp-formula><p>The coordinate transformation to the physical netric inside the extended horizon defines</p><disp-formula id="scirp.59227-formula1207"><label>(73)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x100.png"  xlink:type="simple"/></disp-formula><p>as in Equation (14), and the continuity of the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502307x101.png" xlink:type="simple"/></inline-formula> metric requires</p><disp-formula id="scirp.59227-formula1208"><label>(74)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x102.png"  xlink:type="simple"/></disp-formula><p>with constraints</p><disp-formula id="scirp.59227-formula1209"><label>(75)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x103.png"  xlink:type="simple"/></disp-formula><p>for positive definite metric functions.</p><p>From Equation (70) one gets</p><disp-formula id="scirp.59227-formula1210"><label>(76)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x104.png"  xlink:type="simple"/></disp-formula><p>The expansion in a parameter a gives</p><disp-formula id="scirp.59227-formula1211"><label>(77)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x105.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.59227-formula1212"><label>(78)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x106.png"  xlink:type="simple"/></disp-formula><p>Near the surface of the extended horizon, the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502307x107.png" xlink:type="simple"/></inline-formula> term dominates, so the temperature structure is determined by non-rotating behavior, and it is a negative temperature. Therefore, high temperature behavior of compact objects near the extended horizon persists and should be observable, as long as</p><disp-formula id="scirp.59227-formula1213"><label>(79)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x108.png"  xlink:type="simple"/></disp-formula><p>This constraint is well satisfied for all the observed neutron stars, as is seen from Equation (61).</p><p>If one may replaces <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502307x109.png" xlink:type="simple"/></inline-formula> by [<xref ref-type="bibr" rid="scirp.59227-ref10">10</xref>]</p><disp-formula id="scirp.59227-formula1214"><label>(80)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502307x110.png"  xlink:type="simple"/></disp-formula><p>in Equation (52), one gets the same expressions for Equation (69) and Equation (78) with different coefficients for the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502307x111.png" xlink:type="simple"/></inline-formula> term. Then, one can reach the same conclusion for the temperature structure of rotating compact objects.</p><p>In conclusion, the temperature structure for rotating compact objects near the extended horizon is the same as those for non-rotating compact objects, as long as the condition of Equation (79) is satisfied. Namely, the temperature outside the extended horizon is positive approaching infinitely large value at the extended horizon, and the temperature inside the extended horizon is negative in the neighborhood of the extended horizon.</p></sec><sec id="s5"><title>5. Observation of High Temperature Signature from Compact Objects</title><p>The active observation of X-ray spectra from compact objects is going on using X-ray satellites. Many emission lines in the range of 10 - 30 &#197; ngstrom indicate the presence of multiplly ionized atoms [<xref ref-type="bibr" rid="scirp.59227-ref11">11</xref>] on the surface on neutron stars. From AGN in the range of z &#163; 0.441, one observed a distinguished X-ray peak [<xref ref-type="bibr" rid="scirp.59227-ref12">12</xref>] at 4 - 6 keV. Using the physical metric for compact objects, the author identified [<xref ref-type="bibr" rid="scirp.59227-ref13">13</xref>] the peak as that of Ni XXVIII. More recently, the most luminous galaxies are discovered by WISE [<xref ref-type="bibr" rid="scirp.59227-ref7">7</xref>] .</p><p>These are the indication of high temperature nature of the surface of compact objects. Since the physical metric suggests a definite value of gravitational redshift on the surface of the extended horizon of the compact objects, a consistent description of gravitational redshift will be tested in the future.</p></sec><sec id="s6"><title>6. Summary</title><p>From the introduction of the physical metric, one encounters a revolutionary change in the feature of compact objects, black holes and neutron stars. The extended horizon, 2.60 times of that of the Schwarzschild radius, is the size of compact objects. The gravitational red shift on the surface of compact objects is the universal value of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502307x112.png" xlink:type="simple"/></inline-formula> except for the rotation of critical frequency. This universal prediction is valid for any mass and any species, black holes or neutron stars. In this article, the temperature structure implied by the physical metric is explored. Temperature outside the extended horizon can reach infinitely high at the extended horizon, while temperature inside the extended horizon is negative, higher than any positive temperature. This characteristic persists near the extended horizon as long as the effect of the rotation is limited as are satistfied for all observed neutron stars.</p><p>It is a great pleasure to thank Peter K. Tomozawa for reading the manuscript.</p></sec><sec id="s7"><title>Cite this paper</title><p>YukioTomozawa, (2015) Temperature Structure of Compact Objects. Journal of Modern Physics,06,1412-1420. doi: 10.4236/jmp.2015.610146</p></sec></body><back><ref-list><title>References</title><ref id="scirp.59227-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Tomozawa, Y. (2015) Journal of Modern Physics, 6, 335-345. http://dx.doi.org/10.4236/jmp.2015.63036</mixed-citation></ref><ref id="scirp.59227-ref2"><label>2</label><mixed-citation publication-type="other" xlink:type="simple">Tomozawa, Y. (2015) Journal of Modern Physics, 6, 972-981. http://dx.doi.org/10.4236/jmp.2015.67101</mixed-citation></ref><ref id="scirp.59227-ref3"><label>3</label><mixed-citation publication-type="other" xlink:type="simple">Resenberg, R.D. and Shapiro, I.I. 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