<?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.2016.23028</article-id><article-id pub-id-type="publisher-id">JHEPGC-67740</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>
 
 
  Cosmological Constant and Energy Density of Random Electromagnetic Field
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Ilya</surname><given-names>A. Obukhov</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>Research &amp;amp; Development Company “System Recourses”, Moscow, Russia</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>i_obukhov@systemres.ru</email></corresp></author-notes><pub-date pub-type="epub"><day>20</day><month>06</month><year>2016</year></pub-date><volume>02</volume><issue>03</issue><fpage>312</fpage><lpage>319</lpage><history><date date-type="received"><day>14</day>	<month>April</month>	<year>2016</year></date><date date-type="rev-recd"><day>accepted</day>	<month>25</month>	<year>June</year>	</date><date date-type="accepted"><day>28</day>	<month>June</month>	<year>2016</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>
 
 
  It is shown that the non-equilibrium electrically neutral and relativistically invariant vacuum-like state with the negative energy density and positive pressure may exist at the non-zero temperature in the system of spinor particles, antiparticles, and random electromagnetic field generated by particle-particle, particle-antiparticle, and antiparticle-antiparticle transitions. At the temperature of the order of 10 
  <sup>-5</sup> K, the energy density of its state corresponds to the dark energy density in absolute magnitude. The cosmological constant for such material medium turns out to be negative.
 
</p></abstract><kwd-group><kwd>Dark Energy</kwd><kwd> Cosmological Constant</kwd><kwd> Stochastic Electromagnetic Field</kwd><kwd> Spinor Particles</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Article [<xref ref-type="bibr" rid="scirp.67740-ref1">1</xref>] shows that the quantum theory allows building up the relativistically invariant state of matter, for which pressure p and energy density <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x6.png" xlink:type="simple"/></inline-formula> are related as follows</p><disp-formula id="scirp.67740-formula1732"><label>(1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x7.png"  xlink:type="simple"/></disp-formula><p>Interest in the investigation of such states is related to search for the physical interpretation of the cosmological constant in the Einstein’s equations [<xref ref-type="bibr" rid="scirp.67740-ref1">1</xref>] - [<xref ref-type="bibr" rid="scirp.67740-ref3">3</xref>] and dark energy nature [<xref ref-type="bibr" rid="scirp.67740-ref4">4</xref>] - [<xref ref-type="bibr" rid="scirp.67740-ref6">6</xref>] .</p><p>If a material medium exists, whose energy-momentum density tensor is expressible in the following form</p><disp-formula id="scirp.67740-formula1733"><label>(2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x8.png"  xlink:type="simple"/></disp-formula><p>then the cosmological constant <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x9.png" xlink:type="simple"/></inline-formula> in the Einstein’s equations [<xref ref-type="bibr" rid="scirp.67740-ref1">1</xref>] can be related to the energy density of such medium <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x10.png" xlink:type="simple"/></inline-formula><sup> </sup></p><disp-formula id="scirp.67740-formula1734"><label>. (3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x11.png"  xlink:type="simple"/></disp-formula><p>Here G is the gravitation constant, c is the velocity of light. In case of the empty flat space, when the Minkovsky’s tensor <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x12.png" xlink:type="simple"/></inline-formula> with <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x13.png" xlink:type="simple"/></inline-formula> diagonal is the metric tensor<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x14.png" xlink:type="simple"/></inline-formula>, energy density <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x15.png" xlink:type="simple"/></inline-formula> and pressure <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x16.png" xlink:type="simple"/></inline-formula> obviously satisfy the relationship (1).</p><p>If<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x17.png" xlink:type="simple"/></inline-formula>, then negative pressure <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x18.png" xlink:type="simple"/></inline-formula> can be interpreted [<xref ref-type="bibr" rid="scirp.67740-ref4">4</xref>] [<xref ref-type="bibr" rid="scirp.67740-ref6">6</xref>] as the cause of the antigravity. The opposite possibility, where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x19.png" xlink:type="simple"/></inline-formula> [<xref ref-type="bibr" rid="scirp.67740-ref1">1</xref>] [<xref ref-type="bibr" rid="scirp.67740-ref2">2</xref>] , is not also excluded. In such a case, the gravitational attraction between massive objects starts increasing at the distances exceeding some threshold one.</p><p>The cosmological constant problem is particularly relevant in the context of the experimental confirmation of the accelerated expansion of the Universe [<xref ref-type="bibr" rid="scirp.67740-ref6">6</xref>] . However, this phenomenon can be explained not only with the help of the General Relativity, but also by the different alternative versions of the Gravity Theory (see [<xref ref-type="bibr" rid="scirp.67740-ref7">7</xref>] and the articles cited there), where dark energy concept isn’t introduced. In paper [<xref ref-type="bibr" rid="scirp.67740-ref7">7</xref>] it is shown that the analysis of the interference of gravitational waves will allow making a choice for that or another Gravity Theory.</p><p>Experimental discovery of gravitational waves [<xref ref-type="bibr" rid="scirp.67740-ref8">8</xref>] allows hoping for increasing of our understanding of the nature of gravitation. Data obtained now confirm justice of the General Relativity [<xref ref-type="bibr" rid="scirp.67740-ref8">8</xref>] . But it is only the first experiments and it is not enough for final conclusions.</p><p>In any case, up to date, the material medium model-building problem, for which relationship (1) is true and density</p><disp-formula id="scirp.67740-formula1735"><label>(4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x20.png"  xlink:type="simple"/></disp-formula><p>is close, at least in the order-of-magnitude, to the value of</p><disp-formula id="scirp.67740-formula1736"><graphic  xlink:href="http://html.scirp.org/file/5-2180096x21.png"  xlink:type="simple"/></disp-formula><p>resulted from the interpretation of astrophysical data [<xref ref-type="bibr" rid="scirp.67740-ref6">6</xref>] that has not been solved. Solving this problem seems important for the understanding of potential physical phenomena leading to the formation of such material medium.</p></sec><sec id="s2"><title>2. Energy-Momentum Tensor of Random Electromagnetic Field</title><p>Let us consider the model where the electromagnetic field tensor</p><disp-formula id="scirp.67740-formula1737"><label>(5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x22.png"  xlink:type="simple"/></disp-formula><p>is governed by the Maxwell’s equations</p><disp-formula id="scirp.67740-formula1738"><label>, (6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x23.png"  xlink:type="simple"/></disp-formula><p>with random source <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x24.png" xlink:type="simple"/></inline-formula> on the right side. Here <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x24.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x25.png" xlink:type="simple"/></inline-formula> is the vector potential of electromagnetic field, and e is the electric charge.</p><p>We consider that for flow density <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x26.png" xlink:type="simple"/></inline-formula> the conservation law is true</p><disp-formula id="scirp.67740-formula1739"><label>, (7)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x27.png"  xlink:type="simple"/></disp-formula><p>and for potential <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x28.png" xlink:type="simple"/></inline-formula> the Lorentz’ gage condition is true</p><disp-formula id="scirp.67740-formula1740"><label>. (8)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x29.png"  xlink:type="simple"/></disp-formula><p>Suppose, devices available enable measuring only some time interval and/or volume mean values, which will be indicated with brackets<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x30.png" xlink:type="simple"/></inline-formula>. Suppose that</p><disp-formula id="scirp.67740-formula1741"><label>, (9)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x31.png"  xlink:type="simple"/></disp-formula><p>but at the same time for decomposition components <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x32.png" xlink:type="simple"/></inline-formula> on some set of functions<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x32.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x33.png" xlink:type="simple"/></inline-formula>,</p><disp-formula id="scirp.67740-formula1742"><label>(10)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x34.png"  xlink:type="simple"/></disp-formula><p>the following relationship is true:</p><disp-formula id="scirp.67740-formula1743"><label>, (11)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x35.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x36.png" xlink:type="simple"/></inline-formula> is the tensor, whose exact form will be defined later on.</p><p>The formal solution of Equations (6) for <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x37.png" xlink:type="simple"/></inline-formula> meeting the initial condition</p><disp-formula id="scirp.67740-formula1744"><label>, (12)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x38.png"  xlink:type="simple"/></disp-formula><p>taking into account Decomposition (10), can be written down in the following form</p><disp-formula id="scirp.67740-formula1745"><label>, (13)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x39.png"  xlink:type="simple"/></disp-formula><p>where<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x40.png" xlink:type="simple"/></inline-formula>. According to Equations (5), (9), and (13)</p><disp-formula id="scirp.67740-formula1746"><label>. (14)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x41.png"  xlink:type="simple"/></disp-formula><p>Let us determine energy-momentum density tensors of electromagnetic field <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x42.png" xlink:type="simple"/></inline-formula> and its interaction with charged flow <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x42.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x43.png" xlink:type="simple"/></inline-formula></p><disp-formula id="scirp.67740-formula1747"><label>, (15.1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x44.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.67740-formula1748"><label>. (15.2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x45.png"  xlink:type="simple"/></disp-formula><p>These tensors can be presented using quadratic combinations<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x46.png" xlink:type="simple"/></inline-formula>, and therefore their average values may be non-zero. Using Formula (11), for the average value of the sum of tensors <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x46.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x47.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x46.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x47.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x48.png" xlink:type="simple"/></inline-formula>, we obtain</p><disp-formula id="scirp.67740-formula1749"><label>(16.1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x49.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.67740-formula1750"><label>(16.2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x50.png"  xlink:type="simple"/></disp-formula><p>Suppose, tensor <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x51.png" xlink:type="simple"/></inline-formula> describes transitions between acceptable states of spinor particles and antiparticles with mass m and charges e and −e in the binary mixture of their gases. Then it can be defined using the following relationships</p><disp-formula id="scirp.67740-formula1751"><label>(17.1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x52.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.67740-formula1752"><label>(17.2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x53.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.67740-formula1753"><label>(17.3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x54.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.67740-formula1754"><label>(17.4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x55.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.67740-formula1755"><label>, (17.5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x56.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.67740-formula1756"><label>, (17.6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x57.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.67740-formula1757"><label>. (17.7)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x58.png"  xlink:type="simple"/></disp-formula><p>Here indices e and h pertain to particles and antiparticles, respectively; <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x59.png" xlink:type="simple"/></inline-formula>is the Plank’s constant divided by<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x59.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x60.png" xlink:type="simple"/></inline-formula>;<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x59.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x60.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x61.png" xlink:type="simple"/></inline-formula>, and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x59.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x60.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x61.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x62.png" xlink:type="simple"/></inline-formula> are four-dimensional momenta of particles and antiparticles, for which the following dispersion relationship is true</p><disp-formula id="scirp.67740-formula1758"><label>, (18)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x63.png"  xlink:type="simple"/></disp-formula><p>indices r and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x64.png" xlink:type="simple"/></inline-formula> take on the values of &#177;1 and correspond to the two possible spin states of particles and antiparticles; <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x64.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x65.png" xlink:type="simple"/></inline-formula>and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x64.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x65.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x66.png" xlink:type="simple"/></inline-formula> are chemical potentials of particles and antiparticles, which we will consider as constant;</p><disp-formula id="scirp.67740-formula1759"><label>, (19)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x67.png"  xlink:type="simple"/></disp-formula><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x68.png" xlink:type="simple"/></inline-formula>is the Boltzmann’s constant, T is the temperature;</p><disp-formula id="scirp.67740-formula1760"><label>(20)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x69.png"  xlink:type="simple"/></disp-formula><p>the Fermi-Dirac distribution function;</p><disp-formula id="scirp.67740-formula1761"><label>, (21)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x70.png"  xlink:type="simple"/></disp-formula><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x71.png" xlink:type="simple"/></inline-formula>is the hydrodynamic velocity [<xref ref-type="bibr" rid="scirp.67740-ref9">9</xref>] that meets the relationship</p><disp-formula id="scirp.67740-formula1762"><label>. (22)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x72.png"  xlink:type="simple"/></disp-formula><p>Vectors <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x73.png" xlink:type="simple"/></inline-formula> correspond to flows of transitions between the states of particles and antiparticles</p><disp-formula id="scirp.67740-formula1763"><label>(23)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x74.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x75.png" xlink:type="simple"/></inline-formula> is the Dirac gamma-matrices, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x75.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x76.png" xlink:type="simple"/></inline-formula>and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x75.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x76.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x77.png" xlink:type="simple"/></inline-formula> are spinors that satisfy Equations</p><disp-formula id="scirp.67740-formula1764"><label>, (24.1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x78.png"  xlink:type="simple"/></disp-formula><p>and normalization conditions</p><disp-formula id="scirp.67740-formula1765"><label>(24.2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x79.png"  xlink:type="simple"/></disp-formula><p>It is easy to show that the relations of orthogonality are true</p><disp-formula id="scirp.67740-formula1766"><label>. (25)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x80.png"  xlink:type="simple"/></disp-formula><p>With account of these definitions, Expressions (25), and the formula for the transition from the summation over composite index <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x81.png" xlink:type="simple"/></inline-formula> to the integration over momentum p</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x82.png" xlink:type="simple"/></inline-formula>,</p><p>we obtain from Relationships (16.1) and (16.2)</p><disp-formula id="scirp.67740-formula1767"><label>, (26.1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x83.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.67740-formula1768"><label>, (26.2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x84.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.67740-formula1769"><label>(26.3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x85.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.67740-formula1770"><label>(26.4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x86.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.67740-formula1771"><label>(26.5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x87.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x88.png" xlink:type="simple"/></inline-formula> is the fine-structure constant approximately equal to 1/137, if e is the electron charge.</p></sec><sec id="s3"><title>3. Energy Density and Pressure of Interacting Mixture</title><p>Assume, the inequations are true</p><disp-formula id="scirp.67740-formula1772"><label>, (27)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x89.png"  xlink:type="simple"/></disp-formula><p>i.e. particle and antiparticle gases are degenerating ones. Let us consider the range of temperature and chemical potential values that satisfy the following conditions:</p><disp-formula id="scirp.67740-formula1773"><label>. (28)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x90.png"  xlink:type="simple"/></disp-formula><p>Here <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x91.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x91.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x92.png" xlink:type="simple"/></inline-formula> are Fermi momenta defined in the following relationships:</p><disp-formula id="scirp.67740-formula1774"><label>. (29)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x93.png"  xlink:type="simple"/></disp-formula><p>In the frame of reference where<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x94.png" xlink:type="simple"/></inline-formula>, we obtain the expressions for energy density and pressure</p><disp-formula id="scirp.67740-formula1775"><label>, (30.1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x95.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.67740-formula1776"><label>(30.2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x96.png"  xlink:type="simple"/></disp-formula><p>related to the components of the energy-momentum tensor by simple relationships</p><disp-formula id="scirp.67740-formula1777"><label>. (31)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x97.png"  xlink:type="simple"/></disp-formula><p>The following formulas are true under Conditions (28) in the same frame of reference for concentrations of particles and antiparticles <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x98.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x98.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x99.png" xlink:type="simple"/></inline-formula>, their energy densities and pressures</p><disp-formula id="scirp.67740-formula1778"><label>, (32.1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x100.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.67740-formula1779"><label>, (32.2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x101.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.67740-formula1780"><label>(32.3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x102.png"  xlink:type="simple"/></disp-formula><p>The condition of electroneutrality of the particle and antiparticle gases mixture has the following form</p><disp-formula id="scirp.67740-formula1781"><label>, (33)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x103.png"  xlink:type="simple"/></disp-formula><p>whence it follows that</p><disp-formula id="scirp.67740-formula1782"><label>. (34)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x104.png"  xlink:type="simple"/></disp-formula><p>In such a case, we obtain for the total energy density and pressure</p><disp-formula id="scirp.67740-formula1783"><label>, (35.1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x105.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.67740-formula1784"><label>. (35.2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x106.png"  xlink:type="simple"/></disp-formula><p>The energy density and pressure of electrically neutral particle and antiparticle gases mixture will be relativistically invariant in two cases [<xref ref-type="bibr" rid="scirp.67740-ref1">1</xref>] where</p><disp-formula id="scirp.67740-formula1785"><graphic  xlink:href="http://html.scirp.org/file/5-2180096x107.png"  xlink:type="simple"/></disp-formula><p>and where condition (1) is met. In the first case, we obtain from Equations (35.1) and (35.2)</p><disp-formula id="scirp.67740-formula1786"><label>. (36)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x108.png"  xlink:type="simple"/></disp-formula><p>Furthermore, according to Formulas (32.1), concentrations of particles and antiparticles are zero.</p><p>In the second case, we obtain the condition of implementing the electrically neutral and relativistically invariant state for the mixture under consideration from Relationships (1), (35.1) and (35.2)</p><disp-formula id="scirp.67740-formula1787"><label>. (37)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x109.png"  xlink:type="simple"/></disp-formula><p>Here the Fermi momentum and temperature, at which conditions (1) is met, are indicated using <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x110.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x110.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x111.png" xlink:type="simple"/></inline-formula>. It is easy to show that momentum <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x110.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x111.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x112.png" xlink:type="simple"/></inline-formula> satisfying Equation (37) satisfies also Inequations (28)</p><disp-formula id="scirp.67740-formula1788"><graphic  xlink:href="http://html.scirp.org/file/5-2180096x113.png"  xlink:type="simple"/></disp-formula><p>The following expressions are true for the concentrations of particles and antiparticles, energy density and pressure of the mixture</p><disp-formula id="scirp.67740-formula1789"><label>(38.1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x114.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.67740-formula1790"><label>(38.2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x115.png"  xlink:type="simple"/></disp-formula><p>We receive the following from Formulas (3), (4), and (38.2) for the cosmological constant and dark energy density</p><disp-formula id="scirp.67740-formula1791"><label>(39.1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x116.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.67740-formula1792"><label>(39.2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-2180096x117.png"  xlink:type="simple"/></disp-formula><p>Here the following is specified</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x118.png" xlink:type="simple"/></inline-formula>,</p><p>−a dimensionless value representing a gravitational analogue of the fine structure constant in terms of the build-up method, if m is the mass of electron, then<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x119.png" xlink:type="simple"/></inline-formula>;</p><disp-formula id="scirp.67740-formula1793"><graphic  xlink:href="http://html.scirp.org/file/5-2180096x120.png"  xlink:type="simple"/></disp-formula><p>is the analogue of the Compton wave-length</p><disp-formula id="scirp.67740-formula1794"><graphic  xlink:href="http://html.scirp.org/file/5-2180096x121.png"  xlink:type="simple"/></disp-formula><p>for an object with the energy equal to<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x122.png" xlink:type="simple"/></inline-formula>.</p><p>If e and m are the charge and mass of electron, and dark energy density</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x123.png" xlink:type="simple"/></inline-formula>,</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x124.png" xlink:type="simple"/></inline-formula>.</p><p>The second of Formulas (39.2) for density <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x125.png" xlink:type="simple"/></inline-formula> has the strongly non-isotropic form. As if the dark energy is distributed in a parallelepiped with the very small height <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x125.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x126.png" xlink:type="simple"/></inline-formula> as compared with the typical dimensions of edges of bases <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x125.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x126.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x127.png" xlink:type="simple"/></inline-formula></p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x128.png" xlink:type="simple"/></inline-formula>.</p><p>Note that the contribution of the random electromagnetic field, including the contribution of interaction of this field with particles and antiparticles, to the total energy density in absolute magnitude is thrice as much as the contributions of particles and antiparticles equal to each other</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x129.png" xlink:type="simple"/></inline-formula>.</p><p>Just due to the random electromagnetic field generated by transitions between particles and antiparticles, the state that satisfies Condition (1) is possible in the system studied.</p><p>In the approximation considered, energy density <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x130.png" xlink:type="simple"/></inline-formula> and pressure <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x130.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x131.png" xlink:type="simple"/></inline-formula> are resulting mainly from particle- particle and antiparticle-antiparticle transitions. The energy density and pressure related to particle-antiparticle transitions are much less than <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x130.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x131.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x132.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x130.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x131.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x132.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x133.png" xlink:type="simple"/></inline-formula></p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x134.png" xlink:type="simple"/></inline-formula>.</p><p>Furthermore, the energy dominance [<xref ref-type="bibr" rid="scirp.67740-ref2">2</xref>] is disrupted for <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x135.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x135.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x136.png" xlink:type="simple"/></inline-formula>, and their components.</p></sec><sec id="s4"><title>4. Conclusions</title><p>The model of the material medium, for which the electrically neutral relativistically invariant state with non-zero energy density, pressure, concentrations of particles and antiparticles is possible, has been considered. At the same time particles and antiparticles are in the thermal equilibrium, but far from the chemical equilibrium state governed by the equality of their chemical potentials. In the considered case, the expression is true</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x137.png" xlink:type="simple"/></inline-formula>.</p><p>This non-equilibrium electrically neutral state exists due to the random electromagnetic field generated by spontaneous transitions between particles and antiparticles being in different quantum states. The average vector potential and intensity of this field are zero. But the average components of the energy-momentum density tensor in the random process of transitions between the states of particles and antiparticles are non-zero.</p><p>The energy density of the above vacuum-like state can be expressed in terms of its temperature<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x138.png" xlink:type="simple"/></inline-formula>. The state electroneutrality requirement leads to the equality of Fermi momentum of particles and antiparticles, and the relativistic invariance requirement to the equation relating the Fermi momentum with the temperature.</p><p>If the energy density of the system considered is identified with the dark energy density, then temperature <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x139.png" xlink:type="simple"/></inline-formula> turns to be of the order of 10<sup>−5</sup> K and Fermi velocity of particles and antiparticles <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x139.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-2180096x140.png" xlink:type="simple"/></inline-formula> to be approximately 1 cm/s (m is the mass of electron). Furthermore, the dark energy density and cosmological constant are negative.</p></sec><sec id="s5"><title>Cite this paper</title><p>Ilya A. Obukhov, (2016) Cosmological Constant and Energy Density of Random Electromagnetic Field. Journal of High Energy Physics, Gravitation and Cosmology,02,312-319. doi: 10.4236/jhepgc.2016.23028</p></sec></body><back><ref-list><title>References</title><ref id="scirp.67740-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Zel’dovich, Ya.B. (1968) The Cosmological Constant and the Theory of Elementary Particles. Soviet Physics Uspekhi, 11, 381-393. http://ufn.ru/ru/articles/1968/5/m/</mixed-citation></ref><ref id="scirp.67740-ref2"><label>2</label><mixed-citation publication-type="other" xlink:type="simple">Zel’dovich, Ya.B. (1981) Vacuum Theory: A Possible Solution to the Singularity Problem of Cosmology. Soviet Physics Uspekhi, 24, 216-230. http://ufn.ru/ru/articles/1981/3/c/</mixed-citation></ref><ref id="scirp.67740-ref3"><label>3</label><mixed-citation publication-type="other" xlink:type="simple">Gliner, E.B. (1966) Algebraic Properties of the Energy-Momentum Tensor and Vacuum-Like States of Matter. Soviet Physics JETP, 22, 378-382. http://www.jetp.ac.ru/cgi-bin/r/index/e/22/2/p378?a=list</mixed-citation></ref><ref id="scirp.67740-ref4"><label>4</label><mixed-citation publication-type="other" xlink:type="simple">Chernin, A.D. (2008) Dark Energy and Universal Antigravitation. Physics-Uspekhi, 51, 253-282.  
http://ufn.ru/ru/articles/2008/3/c/</mixed-citation></ref><ref id="scirp.67740-ref5"><label>5</label><mixed-citation publication-type="other" xlink:type="simple">Lukash, V.N. and Rubakov, V.A. (2008) Dark Energy: Myths and Reality. Physics-Uspekhi, 51, 283-289.  
http://ufn.ru/ru/articles/2008/3/d/</mixed-citation></ref><ref id="scirp.67740-ref6"><label>6</label><mixed-citation publication-type="other" xlink:type="simple">Chernin, A.D. (2013) Dark Energy in Systems of Galaxies. JETP Letters, 98, 394-407.  
http://www.jetpletters.ac.ru/ps/2018/article_30426.pdf http://dx.doi.org/10.1134/S002136401319003X</mixed-citation></ref><ref id="scirp.67740-ref7"><label>7</label><mixed-citation publication-type="other" xlink:type="simple">Corda, C. (2009) Interferometric Detection of Gravitational Waves: The Definitive Test for General Relativity. International Journal of Modern Physics D, 18, 2275-2282. http://dx.doi.org/10.1142/S0218271809015904</mixed-citation></ref><ref id="scirp.67740-ref8"><label>8</label><mixed-citation publication-type="other" xlink:type="simple">Abbott, B.P., et al. (2016) Observation of Gravitational Waves from a Binary Black Hole Merger. Physical Review Letters, 116, 061102-01-061102-16. https://journals.aps.org/prl/abstract/10.1103/PhysRevLett.116.061102 
http://dx.doi.org/10.1103/physrevlett.116.061102</mixed-citation></ref><ref id="scirp.67740-ref9"><label>9</label><mixed-citation publication-type="other" xlink:type="simple">de Groot, S.R., van Leeuwen, W.A. and van Weert, Ch.G. (1980) Relativistic Kinetic Theory. Principles and Applications. North-Holland Publishing Company, Amsterdam, New York and Oxford.</mixed-citation></ref></ref-list></back></article>