<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article  PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd"><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article"><front><journal-meta><journal-id journal-id-type="publisher-id">JHEPGC</journal-id><journal-title-group><journal-title>Journal of High Energy Physics, Gravitation and Cosmology</journal-title></journal-title-group><issn pub-type="epub">2380-4327</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/jhepgc.2020.63025</article-id><article-id pub-id-type="publisher-id">JHEPGC-100713</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>
 
 
  Note on the Formation of Supermassive Black Holes
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Kenneth</surname><given-names>Dalton</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>Th. Pongprasart, Bang Saphan, Prachuap Kiri Khan, Thailand</addr-line></aff><pub-date pub-type="epub"><day>03</day><month>06</month><year>2020</year></pub-date><volume>06</volume><issue>03</issue><fpage>321</fpage><lpage>323</lpage><history><date date-type="received"><day>1,</day>	<month>May</month>	<year>2020</year></date><date date-type="rev-recd"><day>2,</day>	<month>June</month>	<year>2020</year>	</date><date date-type="accepted"><day>5,</day>	<month>June</month>	<year>2020</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>
 
 
  Supermassive black holes formed during the lepton epoch of the Big Bang. What follows is a description of how this may have happened.
 
</p></abstract><kwd-group><kwd>Supermassive Black Holes</kwd><kwd> Electron-Positron Model</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>The electron-positron model of supermassive black holes is given in two recent papers [<xref ref-type="bibr" rid="scirp.100713-ref1">1</xref>] [<xref ref-type="bibr" rid="scirp.100713-ref2">2</xref>]. The equilibrium conditions from [<xref ref-type="bibr" rid="scirp.100713-ref1">1</xref>] are reproduced below. The intermediate masses (<xref ref-type="table" rid="table1">Table 1</xref>) range from 10<sup>3</sup> to 8 &#215; 10 6   M ⊙ . They are supported against gravity by electron degeneracy pressure and are characterized by the central Fermi energy ϵ F 0 . They are in a quantum ground state and do not radiate. Larger masses (<xref ref-type="table" rid="table2">Table 2</xref>) are supported by ideal gas and radiation pressure, with a central thermal energy k T 0 . They are equal in size to the Schwarzschild radius, so that the gas and radiation are confined.</p><p>Clusters of black holes can explain the dark matter in elliptical galaxies, dwarf galaxies, star clusters and galactic clusters [<xref ref-type="bibr" rid="scirp.100713-ref3">3</xref>]. Spiral galaxies evolved around a single black hole, and the missing mass must be treated separately [<xref ref-type="bibr" rid="scirp.100713-ref4">4</xref>]. In these</p><table-wrap id="table1" ><label><xref ref-type="table" rid="table1">Table 1</xref></label><caption><title> Intermediate-mass</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >M ( M ⊙ )</th><th align="center" valign="middle" >R &gt; R s (cm)</th><th align="center" valign="middle" >ρ 0 (g∙cm<sup>−</sup><sup>3</sup>)</th><th align="center" valign="middle" >P 0 (Pa)</th><th align="center" valign="middle" >ϵ F 0 (eV)</th></tr></thead><tr><td align="center" valign="middle" >10<sup>3</sup></td><td align="center" valign="middle" >4.8 (10<sup>13</sup>)</td><td align="center" valign="middle" >2.6 (10<sup>−</sup><sup>5</sup>)</td><td align="center" valign="middle" >3.9 (10<sup>9</sup>)</td><td align="center" valign="middle" >2.1</td></tr><tr><td align="center" valign="middle" >10<sup>4</sup></td><td align="center" valign="middle" >2.25 (10<sup>13</sup>)</td><td align="center" valign="middle" >2.6 (10<sup>−</sup><sup>3</sup>)</td><td align="center" valign="middle" >8.4 (10<sup>12</sup>)</td><td align="center" valign="middle" >4.5 (10)</td></tr><tr><td align="center" valign="middle" >10<sup>5</sup></td><td align="center" valign="middle" >1.05 (10<sup>13</sup>)</td><td align="center" valign="middle" >2.6 (10<sup>−</sup><sup>1</sup>)</td><td align="center" valign="middle" >1.8 (10<sup>16</sup>)</td><td align="center" valign="middle" >9.6 (10<sup>2</sup>)</td></tr><tr><td align="center" valign="middle" >10<sup>6</sup></td><td align="center" valign="middle" >4.8 (10<sup>12</sup>)</td><td align="center" valign="middle" >2.6 (10)</td><td align="center" valign="middle" >3.9 (10<sup>19</sup>)</td><td align="center" valign="middle" >2.1 (10<sup>4</sup>)</td></tr><tr><td align="center" valign="middle" >8 (10<sup>6</sup>)</td><td align="center" valign="middle" >2.4 (10<sup>12</sup>)</td><td align="center" valign="middle" >1.7 (10<sup>3</sup>)</td><td align="center" valign="middle" >3.9 (10<sup>22</sup>)</td><td align="center" valign="middle" >3.3 (10<sup>5</sup>)</td></tr></tbody></table></table-wrap><table-wrap id="table2" ><label><xref ref-type="table" rid="table2">Table 2</xref></label><caption><title> Supermassive</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >M ( M ⊙ )</th><th align="center" valign="middle" >R = R s (cm)</th><th align="center" valign="middle" >ρ 0 (g∙cm<sup>−</sup><sup>3</sup>)</th><th align="center" valign="middle" >P 0 (Pa)</th><th align="center" valign="middle" >k T 0 (eV)</th></tr></thead><tr><td align="center" valign="middle" >8 (10<sup>6</sup>)</td><td align="center" valign="middle" >2.4 (10<sup>12</sup>)</td><td align="center" valign="middle" >2 (10<sup>3</sup>)</td><td align="center" valign="middle" >3.9 (10<sup>22</sup>)</td><td align="center" valign="middle" >1.1 (10<sup>5</sup>)</td></tr><tr><td align="center" valign="middle" >10<sup>7</sup></td><td align="center" valign="middle" >3 (10<sup>12</sup>)</td><td align="center" valign="middle" >1.3 (10<sup>3</sup>)</td><td align="center" valign="middle" >2.5 (10<sup>22</sup>)</td><td align="center" valign="middle" >1.1 (10<sup>5</sup>)</td></tr><tr><td align="center" valign="middle" >10<sup>8</sup></td><td align="center" valign="middle" >3 (10<sup>13</sup>)</td><td align="center" valign="middle" >1.3 (10)</td><td align="center" valign="middle" >2.5 (10<sup>20</sup>)</td><td align="center" valign="middle" >6.2 (10<sup>4</sup>)</td></tr><tr><td align="center" valign="middle" >10<sup>9</sup></td><td align="center" valign="middle" >3 (10<sup>14</sup>)</td><td align="center" valign="middle" >1.3 (10<sup>−</sup><sup>1</sup>)</td><td align="center" valign="middle" >2.5 (10<sup>18</sup>)</td><td align="center" valign="middle" >2.3 (10<sup>4</sup>)</td></tr><tr><td align="center" valign="middle" >10<sup>10</sup></td><td align="center" valign="middle" >3 (10<sup>15</sup>)</td><td align="center" valign="middle" >1.3 (10<sup>−</sup><sup>3</sup>)</td><td align="center" valign="middle" >2.5 (10<sup>16</sup>)</td><td align="center" valign="middle" >8 (10<sup>3</sup>)</td></tr><tr><td align="center" valign="middle" >10<sup>11</sup></td><td align="center" valign="middle" >3 (10<sup>16</sup>)</td><td align="center" valign="middle" >1.3 (10<sup>−</sup><sup>5</sup>)</td><td align="center" valign="middle" >2.5 (10<sup>14</sup>)</td><td align="center" valign="middle" >2 (10<sup>3</sup>)</td></tr></tbody></table></table-wrap><p>and other cases, it is the arrival of black holes in the early Universe that helps to explain recent discoveries in astronomy.</p></sec><sec id="s2"><title>2. Formation of Black Holes</title><p>A great profusion of electrons and positrons occurred during the lepton epoch of the Big Bang. It is estimated that for every nucleon there were 10<sup>9</sup> leptons, so that the mass of leptons exceeded that of nucleons by a factor of 10<sup>6</sup> [<xref ref-type="bibr" rid="scirp.100713-ref5">5</xref>]. It may be said that this period began at time t = 10 − 4 s , temperature T = 10 12 K and density ρ = 10 14 g ⋅ cm − 3 , when the final creation of muons took place. This was followed by annihilation and by the decay of muons into electrons and neutrinos (but no photons). The latter reaction depleted the photon density in favor of electrons and positrons. The lepton energy density u lep = 3 ρ lep k T / m will be greater than that of radiation u rad = a T 4 if</p><p>ρ lep &gt; a m 3 k   T 3 (1)</p><p>The corresponding Jeans mass is [<xref ref-type="bibr" rid="scirp.100713-ref6">6</xref>]</p><p>M J = ( 750 π ) 1 / 2 ( k G m ) 3 / 2 ( T 3 ρ lep ) 1 / 2 &lt; 2 &#215; 10 8 M ⊙ (2)</p><p>Any mass greater than M J will be unstable toward gravitational collapse. In response to the surge in density, the lepton mass shattered into billions of spherical masses, each with a decreasing rate of expansion. They became supermassive black holes.</p><p>The time required for expansion from the highly compressed state to equilibrium may be estimated from R/c in the tables. This ranges from 10<sup>2</sup> to 10<sup>6</sup> seconds. During this length of time, a great deal of annihilation occurred. In the present-day Universe, the mass ratio of dark (leptonic) matter to normal (baryonic) matter is five or six to one. Comparison with the above-cited factor of 10<sup>6</sup> shows that a minute portion of leptons achieved equilibrium as a black hole. The vast majority annihilated and replenished the expanding radiation field.</p></sec><sec id="s3"><title>3. Remark</title><p>The conventional treatment of black holes is mathematical. It posits a solution to the field equations of general relativity, which yields a singular metric at the Schwarzschild radius [<xref ref-type="bibr" rid="scirp.100713-ref7">7</xref>]. This implies that light cannot escape from a black hole. However, this phenomenon was already known to Laplace and others [<xref ref-type="bibr" rid="scirp.100713-ref8">8</xref>]. Since that time, the difficulty has been to find a suitable concentration of mass. The electron-positron model solves that problem, and it provides a physical understanding of black holes.</p></sec><sec id="s4"><title>Conflicts of Interest</title><p>The author declares no conflicts of interest regarding the publication of this paper.</p></sec><sec id="s5"><title>Cite this paper</title><p>Dalton, K. (2020) Note on the Formation of Supermassive Black Holes. Journal of High Energy Physics, Gravitation and Cosmology, 6, 321-323. https://doi.org/10.4236/jhepgc.2020.63025</p></sec></body><back><ref-list><title>References</title><ref id="scirp.100713-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Dalton, K. (2019) Supermassive Black Holes. JHEPGC, 5, 984-988. https://doi.org/10.4236/jhepgc.2019.53052</mixed-citation></ref><ref id="scirp.100713-ref2"><label>2</label><mixed-citation publication-type="other" xlink:type="simple">Dalton, K. (2014) The Galactic Black Hole. 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