<?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">OALibJ</journal-id><journal-title-group><journal-title>Open Access Library Journal</journal-title></journal-title-group><issn pub-type="epub">2333-9705</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/oalib.1102031</article-id><article-id pub-id-type="publisher-id">OALibJ-68748</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Biomedical&amp;Life Sciences</subject><subject> Business&amp;Economics</subject><subject> Chemistry&amp;Materials Science</subject><subject> Computer Science&amp;Communications</subject><subject> Earth&amp;Environmental Sciences</subject><subject> Engineering</subject><subject> Medicine&amp;Healthcare</subject><subject> Physics&amp;Mathematics</subject><subject> Social Sciences&amp;Humanities</subject></subj-group></article-categories><title-group><article-title>
 
 
  The Decay of a Black Hole in a GUT Model
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Risto</surname><given-names>Raitio</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>02230 Espoo, Finland</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>risto.raitio@gmail.com</email></corresp></author-notes><pub-date pub-type="epub"><day>30</day><month>10</month><year>2015</year></pub-date><volume>02</volume><issue>10</issue><fpage>1</fpage><lpage>4</lpage><history><date date-type="received"><day>3</day>	<month>October</month>	<year>2015</year></date><date date-type="rev-recd"><day>accepted</day>	<month>23</month>	<year>October</year>	</date><date date-type="accepted"><day>28</day>	<month>October</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>
 
 
   
   I propose a phenomenological model for the decay of black holes near Planck mass. The decay takes place via a quantum state between general relativity and a grand unified field theory like SO(10). This group is favored also by a no-scale SUGRA GUT model for Starobinsky inflation by other authors. 
  
 
</p></abstract><kwd-group><kwd>Quantum Black Hole</kwd><kwd> Singularity</kwd><kwd> Dark Matter</kwd><kwd> Grand Unified Theory</kwd><kwd> Standard Model</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>The purpose of this note is to propose a quantum model for a decaying (disappearing) black hole [<xref ref-type="bibr" rid="scirp.68748-ref1">1</xref>] [<xref ref-type="bibr" rid="scirp.68748-ref2">2</xref>] . The model is defined on the horizon of the hole. The key element is the gravon state, a critical state which connects general relativity to a grand unified quantum field theory (GUT).<sup>1</sup> Instead of vanishing totally after enough of Hawking radiation a black hole, with mass above the GUT scale, triggers the operators of a grand unified quantum field theory like SO(10). Thereafter the black hole energy decays into SO(10) particles and finally into standard model (SM) particles.</p><p>The SO(10) GUT gets support from a different direction, and time, in the universe. In [<xref ref-type="bibr" rid="scirp.68748-ref3">3</xref>] the authors study Starobinsky inflation in a renormalizable grand unified theory based on the SO(10) gauge group with no scale supergravity theory (SUGRA).</p><p>The black hole decay model is not designed to give new predictions for cosmic microwave background (CMB), or any other, measurements. Most current models, like the Starobinsky or the Higgs inflation model, compare very well with all available data. The purpose of the model is to take a new look “inside” black holes.</p><p>With the Planck scale having its the conventional value 10<sup>19</sup> GeV finding the possible gravon particle near that mass value is hard. Gamma-ray signals from the sky may be a promising way. A gamma-ray, or jet, with energy about half the Planck mass would be a favorable signal for the model. In fact, primordial black holes (PBH) with mass about 10<sup>15</sup> g will be evaporating today and their abundance is constrained by the flux of gamma-rays, for a comprehensive treatment see [<xref ref-type="bibr" rid="scirp.68748-ref4">4</xref>] . Experimental estimate of its lifetime could give information of the internal properties of a black hole. A long lifetime would indicate gravitational and/or inflationary matter properties of the internals of BHs while a short lifetime would be a sign of SM particle internals including QCD contributions.</p><p>In this note I disclose the physical motivation and description of the model. In Section 2 I discuss the core qualitatively. Section 3 is devoted to SO(10) SUGRA GUT inflation model rich multiplet structure. I finish in Section 4 with conclusions.</p></sec><sec id="s2"><title>2. Properties of the Gravon</title><p>The universe consists of classical general relativity and a grand unified quantum field theory of particles. The gravon is a critical connecting state between these two. As seen from the quantum side there is the equivalent of state vector collapse into the classical theory. Seen from the classical side the black hole looses its horizon and makes a transition into quantum fields. The horizon obviously requires proper mathematical treatment, but the physical picture given here seems clear.</p><p>Properties of the gravon model of black holes are the following:</p><p>1) the black hole generates the gravitational field of general relativity at r &gt; r<sub>c</sub>, at r = r<sub>c</sub> there is the horizon, and with r &lt; r<sub>c</sub> there is nothing dynamical, in particular no singularity,</p><p>2) the gravon is a critical state between a minimum energy classical black hole, with energy just above $\MP$, and a quantum field with maximum energy just below M<sub>Planck</sub>,</p><p>3) the critical state makes a transition up in energy to a black hole by absorbing a graviton and down to a fireball by emitting a graviton<sup>2</sup>. The fireball does not have a horizon and it decays explosively into SO(10) particles. Properties of black holes, other than the core, are beyond the scope of this note,</p><p>4) for calculational purposes with Feynman diagrams the fireball can be approximated by a heavy Higgs-like scalar (or a fermion). The energy scale is 2 - 3 orders of magnitude above the grand unified theory scale. SO(10) is a well proven GUT group which accommodates all one generation quarks and leptons in a 16 dimensional spinorial representation (16). Therefore at the energy considered, all particles have zero mass, all interactions have the same strength, all gauge bosons 45 can be produced freely and all quarks can transform into leptons. The Higgs come in the representations 10, 16 and 45. Gravity is not, for the present, part of unification,</p><p>5) the gravon is a horizonless remnant of a thermally end-radiated black hole, either stable or with some (short I suppose) lifetime [<xref ref-type="bibr" rid="scirp.68748-ref6">6</xref>] . Remnants have no singularity or information loss problems, see the recent review [<xref ref-type="bibr" rid="scirp.68748-ref7">7</xref>] .</p><p>Quantization of GR, outside black hole horizon, is not part of this scheme but it can be done independently.</p></sec><sec id="s3"><title>3. SO(10) in Inflation</title><p>In [<xref ref-type="bibr" rid="scirp.68748-ref3">3</xref>] the authors study inflation in a renormalizable grand unified theory based on the SO(10) gauge group with no scale SUGRA. The authors show that a renormalizable Wess-Zumino superpotential of SO(10) GUT along with no-scale K&#228;hler potential can give Starobinsky kind of inflationary potential with specific choice of superpotential parameters. The Higgs supermultiplets the authors consider are 10, 210, 126 (<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x7.png" xlink:type="simple"/></inline-formula>). Among these, the 210 and 126 (<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x8.png" xlink:type="simple"/></inline-formula>) are responsible for breaking of SO(10) symmetry down to minimal supersymmetric standard model (MSSM). The 210 supermultiplet alone can give different intermediate symmetries [<xref ref-type="bibr" rid="scirp.68748-ref8">8</xref>] depending upon which of its MSSM singlet field takes a vacuum expectation value (vev). Then 126 (<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x9.png" xlink:type="simple"/></inline-formula>) breaks this intermediate symmetry to MSSM. Successful inflationary potential can be achieved in the case of</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x10.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x11.png" xlink:type="simple"/></inline-formula>and flipped <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x12.png" xlink:type="simple"/></inline-formula> symmetry.</p><p>At the end of inflation, the reheating can occur via non perturbative decay of inflaton to bosons of the intermediate scale model. After the end of reheating, when universe cools down, the finite temperature potential can have a minimum which corresponds to MSSM and the universe rolls down to this minimum at temperature &lt;&lt; T<sub>R</sub> (reheat temperature).</p><p>In this note the interest is in the multiplet structure of the inflation model. The minimal supersymmetric grand unified theory based on SO(10) gauge group has 10 (H<sub>i</sub>), 210 (Φ<sub>ijkl</sub>) and 126 (Σ<sub>ijklm</sub>) (<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x13.png" xlink:type="simple"/></inline-formula>) Higgs supermultiplets. The representations H<sub>i</sub> is 1 index real, Σ<sub>ijklm</sub> is complex (5 index, totally-antisymmetric, self dual) and Φ<sub>ijkl</sub> is 4 index totally-antisymmetric tensor. Here <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x14.png" xlink:type="simple"/></inline-formula> run over the vector representation of SO(10). The renormalizable superpotential for the above mentioned fields is given by</p><disp-formula id="scirp.68748-formula1018"><label>(1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/68748x15.png"  xlink:type="simple"/></disp-formula><p>The no-scale form of K&#228;hler potential is taken to be</p><disp-formula id="scirp.68748-formula1019"><label>(2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/68748x16.png"  xlink:type="simple"/></disp-formula><p>Here T is the single modulus field arising due to string compactification and M<sub>Planck</sub> = 1.</p><p>The 10 and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x17.png" xlink:type="simple"/></inline-formula> are required for Yukawa terms to give masses to the fermions while 126 (<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x18.png" xlink:type="simple"/></inline-formula>) breaks the SO(10) gauge symmetry to MSSM together with 210. However to have a intermediate symmetry rather than MSSM, the 210 Higgs is sufficient. It can lead to various possible intermediate symmetries depending on which components of the 210 take vevs. The decomposition of Higgs supermultiplets required for SO(10) symmetry</p><p>breaking in terms of Pati-Salam gauge group <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x19.png" xlink:type="simple"/></inline-formula> is given by</p><disp-formula id="scirp.68748-formula1020"><graphic  xlink:href="http://html.scirp.org/file/68748x20.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.68748-formula1021"><graphic  xlink:href="http://html.scirp.org/file/68748x21.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.68748-formula1022"><graphic  xlink:href="http://html.scirp.org/file/68748x22.png"  xlink:type="simple"/></disp-formula><p>The field components which will not break the MSSM symmetry are allowed to take vevs. In this case they are [<xref ref-type="bibr" rid="scirp.68748-ref9">9</xref>]</p><disp-formula id="scirp.68748-formula1023"><graphic  xlink:href="http://html.scirp.org/file/68748x23.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.68748-formula1024"><graphic  xlink:href="http://html.scirp.org/file/68748x24.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.68748-formula1025"><graphic  xlink:href="http://html.scirp.org/file/68748x25.png"  xlink:type="simple"/></disp-formula><p>The Superpotential in terms of these vevs is</p><disp-formula id="scirp.68748-formula1026"><graphic  xlink:href="http://html.scirp.org/file/68748x26.png"  xlink:type="simple"/></disp-formula><p>The vanishing of D-terms gives the condition <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x27.png" xlink:type="simple"/></inline-formula> [<xref ref-type="bibr" rid="scirp.68748-ref9">9</xref>] . The symmetry breaking path of SO(10) is</p><disp-formula id="scirp.68748-formula1027"><graphic  xlink:href="http://html.scirp.org/file/68748x28.png"  xlink:type="simple"/></disp-formula><p>where the first step is caused by 210 and the second by 126. For the first step symmetry breaking one can set<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x29.png" xlink:type="simple"/></inline-formula>. Then the possible intermediate symmetries with 210 only are [<xref ref-type="bibr" rid="scirp.68748-ref9">9</xref>]</p><p>1) If <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x30.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x30.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x31.png" xlink:type="simple"/></inline-formula>, it gives <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x30.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x31.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x32.png" xlink:type="simple"/></inline-formula> symmetry.</p><p>2) If <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x33.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x33.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x34.png" xlink:type="simple"/></inline-formula>, this results in <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x33.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x34.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x35.png" xlink:type="simple"/></inline-formula> symmetry.</p><p>3) If <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x36.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x36.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x37.png" xlink:type="simple"/></inline-formula>, it gives <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x36.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x37.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x38.png" xlink:type="simple"/></inline-formula> symmetry.</p><p>4) If<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x39.png" xlink:type="simple"/></inline-formula>, this has <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x39.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x40.png" xlink:type="simple"/></inline-formula> symmetry.</p><p>5) If<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x41.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x41.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x42.png" xlink:type="simple"/></inline-formula>symmetry but with flipped assignments for particles.</p><p>The superpotential in terms of vevs of 210 is given by</p><disp-formula id="scirp.68748-formula1028"><graphic  xlink:href="http://html.scirp.org/file/68748x43.png"  xlink:type="simple"/></disp-formula><p>Here<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x44.png" xlink:type="simple"/></inline-formula>. Similarly no-scale K&#228;hler potential is</p><disp-formula id="scirp.68748-formula1029"><graphic  xlink:href="http://html.scirp.org/file/68748x45.png"  xlink:type="simple"/></disp-formula><p>The F-term potential has the following form</p><disp-formula id="scirp.68748-formula1030"><label>(3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/68748x46.png"  xlink:type="simple"/></disp-formula><p>where</p><disp-formula id="scirp.68748-formula1031"><graphic  xlink:href="http://html.scirp.org/file/68748x47.png"  xlink:type="simple"/></disp-formula><p>The kinetic term is given as<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x50.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x50.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x49.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x50.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x49.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x48.png" xlink:type="simple"/></inline-formula>. Here i runs over different fields T, p, a and ω. <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x50.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x49.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x48.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x51.png" xlink:type="simple"/></inline-formula>is the inverse of K&#228;hler metric<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x50.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x49.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x48.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x51.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x52.png" xlink:type="simple"/></inline-formula>. After simplifying, the potential given above has the following form</p><disp-formula id="scirp.68748-formula1032"><label>(4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/68748x53.png"  xlink:type="simple"/></disp-formula><p>The authors assume that the non-perturbative Planck scale dynamics fixes the values of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/68748x54.png" xlink:type="simple"/></inline-formula>. After fixing the vev for T the kinetic terms of T can be neglected. The authors study all possible cases of intermediate symmetries mentioned earlier for inflationary conditions in SO(10) with no-scale SUGRA. For simplicity they assume the fields to be real.</p></sec><sec id="s4"><title>4. Conclusions</title><p>The present note contains a proposal of a model for black hole decay. The structure and behavior of Planck mass black holes have not, to my best knowledge, been discussed in terms of GUT fields [<xref ref-type="bibr" rid="scirp.68748-ref2">2</xref>] in the literature. So the present model fulfills this gap. It takes a step beyond the standard model of particles towards a GUT model of Planck scale phenomena including gravity.</p><p>The major conclusion is that the GUT theory based on SO(10) provides very much what is wanted for a description of the universe from big bang to collapse of matter into black holes, whose decays generate bouncing phenomena on all length scales. The dynamical details of the simple black hole decay model and the more involved supersymmetric inflationary theory referred to above should be studied and fitted together.</p><p>It seems one can handle the whole life cycle of particles in the (bouncing) universe using the SO(10) based GUTs. Finally, it seems that there are several elements of quantum gravity available to us if we only could see them properly organized.</p></sec><sec id="s5"><title>Cite this paper</title><p>Risto Raitio, (2015) The Decay of a Black Hole in a GUT Model. Open Access Library Journal,02,1-4. doi: 10.4236/oalib.1102031</p></sec><sec id="s6"><title>NOTES</title></sec></body><back><ref-list><title>References</title><ref id="scirp.68748-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Raitio, R. (2015) Black Holes without Singularity? [viXra:1505.0051v3].</mixed-citation></ref><ref id="scirp.68748-ref2"><label>2</label><mixed-citation publication-type="other" xlink:type="simple">Raitio, R. (2015) A Standard Model at Planck Scale, [viXra:1507.0023v5].</mixed-citation></ref><ref id="scirp.68748-ref3"><label>3</label><mixed-citation publication-type="other" xlink:type="simple">Garg, I. and Mohanty, S. 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