<?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">IJAA</journal-id><journal-title-group><journal-title>International Journal of Astronomy and Astrophysics</journal-title></journal-title-group><issn pub-type="epub">2161-4717</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/ijaa.2016.61010</article-id><article-id pub-id-type="publisher-id">IJAA-65213</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>
 
 
  A New Solution for the Friedmann Equations
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>aser</surname><given-names>Mostaghel</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>Department of Civil Engineering, University of Toledo, Toledo, USA</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>naser.mostaghel@utoledo.edu</email></corresp></author-notes><pub-date pub-type="epub"><day>07</day><month>03</month><year>2016</year></pub-date><volume>06</volume><issue>01</issue><fpage>122</fpage><lpage>134</lpage><history><date date-type="received"><day>30</day>	<month>November</month>	<year>2015</year></date><date date-type="rev-recd"><day>accepted</day>	<month>27</month>	<year>March</year>	</date><date date-type="accepted"><day>30</day>	<month>March</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>
 
 
  Assuming a flat universe expanding under a constant pressure and combining the first and the second Friedmann equations, a new equation, describing the evolution of the scale factor, is derived. The equation is a general kinematic equation. It includes all the ingredients composing the universe. An exact closed form solution for this equation is presented. The solution shows remarkable agreement with available observational data for redshifts from a low of z = 0.0152 to as high as z = 8.68. As such, this solution provides an alternative way of describing the expansion of space without involving the controversial dark energy.
 
</p></abstract><kwd-group><kwd>Cosmological Constant</kwd><kwd> Distances and Redshifts</kwd><kwd> Expanding Universe</kwd><kwd> Friedmann Equations</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>The evolution of the universe has already been investigated through the first Friedmann equation. As discussed by Carrol [<xref ref-type="bibr" rid="scirp.65213-ref1">1</xref>] , the first Friedmann equation is used because it only involves the first derivative of the scale factor. However, the resulting models such as ΛCDM-based models are in terms of limited numbers of parameters representing the ingredients of the universe. Two analytical solutions with restrictive assumptions are already available [<xref ref-type="bibr" rid="scirp.65213-ref2">2</xref>] [<xref ref-type="bibr" rid="scirp.65213-ref3">3</xref>] , which will be presented in Section three. There exists no general analytical solution for the Friedmann equations. Here, through combining the first and the second Friedmann equations, a general equation is formulated. Assuming a flat universe, an exact closed form solution for this general equation is obtained. This solution is remarkably consistent with the observational data over a wide range of measured redshifts from a low of z = 0.0152 to the highest recently measured value of z = 8.68.</p><p>Except for the flatness assumption, the analytical solution is completely general. It includes all the ingredients forming the universe. The ΛCDM-based models only consider specific combinations of limited numbers of ingredients. Also the value of the cosmological density parameter is analytically estimated to be<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x6.png" xlink:type="simple"/></inline-formula>. This is essentially identical to the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x7.png" xlink:type="simple"/></inline-formula> value estimated in 2014 by the Plank Collaboration [<xref ref-type="bibr" rid="scirp.65213-ref4">4</xref>] , based on combined data from “Plank + WP + high L + BAO”. It is also shown that the contribution of the cosmological constant is to cancel the pressure term in the Friedmann acceleration equation. As a consequence, the expansion equation turns out to be a kinematic equation in terms of the scale factor and its rates of change.</p><p>In the next section we develop the new general equation and derive an analytical estimate of the cosmological density parameter. The new analytical solution together with the two existing analytical solutions is presented in Section 3. Comparison of the new analytical solution with the analytical solution involving matter and lamda is presented in Section 4.1. Comparisons of the new analytical solution with the ΛCDM-based models are presented in Section 4.2. In Section 5, the efficacy of the new analytical solution is shown through comparisons with two ΛCDM-based solutions and through comparisons with three sets of observational data.</p></sec><sec id="s2"><title>2. The New General Equation</title><p>The first Friedmann equation, including the curvature, k, and the cosmological constant, Λ, is</p><disp-formula id="scirp.65213-formula242"><label>(1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/10-4500521x8.png"  xlink:type="simple"/></disp-formula><p>Alternatively, including the cosmological term in the total density, the above equation can be represented by</p><disp-formula id="scirp.65213-formula243"><label>(2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/10-4500521x9.png"  xlink:type="simple"/></disp-formula><p>where now the density, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x10.png" xlink:type="simple"/></inline-formula>, is defined by</p><disp-formula id="scirp.65213-formula244"><label>(3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/10-4500521x11.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x12.png" xlink:type="simple"/></inline-formula> represents the mass density; <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x13.png" xlink:type="simple"/></inline-formula>represents the energy density; <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x14.png" xlink:type="simple"/></inline-formula>represents the radiation energy density and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x15.png" xlink:type="simple"/></inline-formula> is the intrinsic vacuum energy density, which is defined by</p><disp-formula id="scirp.65213-formula245"><label>(4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/10-4500521x16.png"  xlink:type="simple"/></disp-formula><p>The curvature can be represented by</p><disp-formula id="scirp.65213-formula246"><label>(5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/10-4500521x17.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x18.png" xlink:type="simple"/></inline-formula> represents the present time and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x19.png" xlink:type="simple"/></inline-formula> is the scale factor. The Friedmann acceleration equation is given by</p><disp-formula id="scirp.65213-formula247"><label>(6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/10-4500521x20.png"  xlink:type="simple"/></disp-formula><p>Substitutions for <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x21.png" xlink:type="simple"/></inline-formula> from Equation (2) and for k from Equation (5) back into the above equation yield</p><disp-formula id="scirp.65213-formula248"><label>(7)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/10-4500521x22.png"  xlink:type="simple"/></disp-formula><p>For the present time, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x23.png" xlink:type="simple"/></inline-formula>, the scale factor,<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x23.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x24.png" xlink:type="simple"/></inline-formula>. Thus the above equation yields</p><disp-formula id="scirp.65213-formula249"><label>(8)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/10-4500521x25.png"  xlink:type="simple"/></disp-formula><p>To evaluate Λ from Equation (8), we need to evaluate <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x26.png" xlink:type="simple"/></inline-formula> first. The value of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x26.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x27.png" xlink:type="simple"/></inline-formula> at the present time is given by</p><disp-formula id="scirp.65213-formula250"><label>(9)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/10-4500521x28.png"  xlink:type="simple"/></disp-formula><p>To evaluate the present time values of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x29.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x29.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x30.png" xlink:type="simple"/></inline-formula>, consider the conservation of energy or the alternative form of the first Friedman equation</p><disp-formula id="scirp.65213-formula251"><label>(10)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/10-4500521x31.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x32.png" xlink:type="simple"/></inline-formula> is an equivalent mass. It represents the total mass-energy of the universe including the total mass of all forms of ordinary and non-ordinary masses as well as the total equivalent mass of all forms of energies; including the effect of the cosmological constant. Because of the conservation of the total mass-energy of the un</p><p>iverse, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x33.png" xlink:type="simple"/></inline-formula>has to be a constant. But<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x33.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x34.png" xlink:type="simple"/></inline-formula>. Therefore</p><disp-formula id="scirp.65213-formula252"><label>(11)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/10-4500521x35.png"  xlink:type="simple"/></disp-formula><p>Because at all points the expansion is taking place in all directions, to evaluate the rate of increase of space between any two galaxies, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x36.png" xlink:type="simple"/></inline-formula>must be replaced by<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x36.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x37.png" xlink:type="simple"/></inline-formula>. Thus</p><disp-formula id="scirp.65213-formula253"><label>(12)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/10-4500521x38.png"  xlink:type="simple"/></disp-formula><p>Correcting the velocity in the above relation for the effect of time dilation yields</p><disp-formula id="scirp.65213-formula254"><label>(13)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/10-4500521x39.png"  xlink:type="simple"/></disp-formula><p>where c represents the speed of light. The value of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x40.png" xlink:type="simple"/></inline-formula> has been analytically determined [<xref ref-type="bibr" rid="scirp.65213-ref5">5</xref>] to be</p><disp-formula id="scirp.65213-formula255"><label>(14)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/10-4500521x41.png"  xlink:type="simple"/></disp-formula><p>Therefore the corrected expansion velocity at the present time is given by</p><disp-formula id="scirp.65213-formula256"><label>(15)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/10-4500521x42.png"  xlink:type="simple"/></disp-formula><p>Also the present time value of the expansion acceleration, according to Equations (13) and (14), is given by</p><disp-formula id="scirp.65213-formula257"><label>(16)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/10-4500521x43.png"  xlink:type="simple"/></disp-formula><p>Substitutions for <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x44.png" xlink:type="simple"/></inline-formula> from Equation (9), for the corrected velocity <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x44.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x45.png" xlink:type="simple"/></inline-formula> from Equation (15), and for <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x44.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x45.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x46.png" xlink:type="simple"/></inline-formula> from Equation (16) back into Equation (8) yields</p><disp-formula id="scirp.65213-formula258"><label>(17)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/10-4500521x47.png"  xlink:type="simple"/></disp-formula><p>Solving the above relation for Λ yields</p><disp-formula id="scirp.65213-formula259"><label>(18)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/10-4500521x48.png"  xlink:type="simple"/></disp-formula><p>Therefore the cosmological density parameter can be represented by</p><disp-formula id="scirp.65213-formula260"><label>(19)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/10-4500521x49.png"  xlink:type="simple"/></disp-formula><p>Now substitution for Λ from Equation (18) back into Equation (7) yields the Friedmann acceleration equation as</p><disp-formula id="scirp.65213-formula261"><label>(20)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/10-4500521x50.png"  xlink:type="simple"/></disp-formula><p>In the next section, assuming a flat universe expanding under the constant pressure<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x51.png" xlink:type="simple"/></inline-formula>, we present an exact closed form solution for the above equation. Before getting to the next section, we will evaluate the value of the cosmological density parameter<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x51.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x52.png" xlink:type="simple"/></inline-formula>. The pressure, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x51.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x52.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x53.png" xlink:type="simple"/></inline-formula>, in Equation (19) has been given by [<xref ref-type="bibr" rid="scirp.65213-ref5">5</xref>] the following relation</p><disp-formula id="scirp.65213-formula262"><label>(21)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/10-4500521x54.png"  xlink:type="simple"/></disp-formula><p>where</p><disp-formula id="scirp.65213-formula263"><label>(22)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/10-4500521x55.png"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.65213-formula264"><label>(23)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/10-4500521x56.png"  xlink:type="simple"/></disp-formula><p>Assuming a flat universe, i.e., <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x57.png" xlink:type="simple"/></inline-formula>, substitutions of the above values into Equation (19) yield the cosmological density parameter as</p><disp-formula id="scirp.65213-formula265"><label>(24)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/10-4500521x58.png"  xlink:type="simple"/></disp-formula><p>This value of the energy density parameter is essentially identical to the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x59.png" xlink:type="simple"/></inline-formula> value estimated in 2014 by the Plank Collaboration [<xref ref-type="bibr" rid="scirp.65213-ref4">4</xref>] , based on data from “Plank + WP + high L + BAO”. This remarkable agreement provides further evidence supporting the description of the pressure as given by Equation (21).</p></sec><sec id="s3"><title>3. The New Analytical Solution for the Friedmann Equations</title><p>Already there exist two analytical solutions for the Friedmann equations. One is for the case of a flat universe containing only matter, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x60.png" xlink:type="simple"/></inline-formula>, where the analytical solution is<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x60.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x61.png" xlink:type="simple"/></inline-formula>, and the other is for the case of a flat universe containing matter and lambda [<xref ref-type="bibr" rid="scirp.65213-ref2">2</xref>] [<xref ref-type="bibr" rid="scirp.65213-ref3">3</xref>] . The analytical solution for the second case is given as</p><disp-formula id="scirp.65213-formula266"><label>(25)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/10-4500521x62.png"  xlink:type="simple"/></disp-formula><p>where<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x63.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x63.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x64.png" xlink:type="simple"/></inline-formula>is the scale factor and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x63.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x64.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x65.png" xlink:type="simple"/></inline-formula>. The new analytical solution considers a flat universe containing all the ingredients including matter, energy, radiation, etc. Considering Equation (20), it is seen that as the time flows from the initiation of expansion to the present time, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x63.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x64.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x65.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x66.png" xlink:type="simple"/></inline-formula>, the coefficient of the curvature term, k, reduces. Thus as time flows, the universe tends toward becoming flatter. Therefore, according to Equation (20), by the present time, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x63.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x64.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x65.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x66.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x67.png" xlink:type="simple"/></inline-formula>, the universe has become completely flat. Assuming a flat universe eliminates the effects of curvature and simplifies the Friedmann acceleration equation to the following form</p><disp-formula id="scirp.65213-formula267"><label>(26)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/10-4500521x68.png"  xlink:type="simple"/></disp-formula><p>Assuming the pressure to be constant implies that in the above equation the term<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x69.png" xlink:type="simple"/></inline-formula>. Since <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x69.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x70.png" xlink:type="simple"/></inline-formula> represents the contribution of the cosmological constant, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x69.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x70.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x71.png" xlink:type="simple"/></inline-formula>being zero is consistent with the vacuum</p><p>pressure being equal to the negative of the vacuum density as discussed by Carroll [<xref ref-type="bibr" rid="scirp.65213-ref6">6</xref>] . Thus the Friedmann acceleration equation is further simplified to the following form:</p><disp-formula id="scirp.65213-formula268"><label>(27)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/10-4500521x72.png"  xlink:type="simple"/></disp-formula><p>It is clear that the above equation satisfies the present time boundary conditions as given in Equations (9), (15) and (16). To non-dimensionalize the above equation, let <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x73.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x73.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x74.png" xlink:type="simple"/></inline-formula>. Substitutions in the above equation yield</p><disp-formula id="scirp.65213-formula269"><label>(28)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/10-4500521x75.png"  xlink:type="simple"/></disp-formula><p>where now dot denotes differentiation with respect to<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x76.png" xlink:type="simple"/></inline-formula>, and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x76.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x77.png" xlink:type="simple"/></inline-formula> represents the scale factor. The present time boundary conditions on the above equation, as derived from Equations (9) and (15), are <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x76.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x77.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x78.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x76.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x77.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x78.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x79.png" xlink:type="simple"/></inline-formula>. The exact solution of the above nonlinear differential equation with the specified boundary conditions is</p><disp-formula id="scirp.65213-formula270"><label>(29)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/10-4500521x80.png"  xlink:type="simple"/></disp-formula><p>The beauty of the above analytical solution is the fact that it does not involve the fractional components forming the mix of the universe. Using the Mathematica code [<xref ref-type="bibr" rid="scirp.65213-ref7">7</xref>] , a plot of the scale factor as given by the above equation together with its first and second derivatives is presented in <xref ref-type="fig" rid="fig1">Figure 1</xref>.</p><p>As seen from the above figure, at the present time, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x81.png" xlink:type="simple"/></inline-formula>, the scale factor, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x81.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x82.png" xlink:type="simple"/></inline-formula>, and its rates of change are, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x81.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x82.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x83.png" xlink:type="simple"/></inline-formula>, and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x81.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x82.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x83.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x84.png" xlink:type="simple"/></inline-formula>. Based on observational data [<xref ref-type="bibr" rid="scirp.65213-ref8">8</xref>] - [<xref ref-type="bibr" rid="scirp.65213-ref10">10</xref>] , it has been concluded that the expansion initially decelerates but then continues to grow with an accelerating rate.</p><p>Considering Equation (18), it is clear that in Equation (20), the pressure <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x85.png" xlink:type="simple"/></inline-formula> represents the contribution of the cosmological constant. It is this pressure, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x85.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x86.png" xlink:type="simple"/></inline-formula>, that cancels the constant pressure, P, allowing the Friedmann acceleration equation to be simplified to the form given by Equation (28).</p><p>In the following subsections the analytical solution given by Equation (29) is compared with the analytical solution for a universe containing only matter and lambda as given by Equation (25). It is also compared with other models based on ΛCDM parameterizations.</p></sec><sec id="s4"><title>4. Comparison of Analytical Solutions</title><p>In order to compare the analytical solution given by Equation (29) with the one given by Equation (25), we need to first decide on the value of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x87.png" xlink:type="simple"/></inline-formula> for substitution in Equation (25). We will use the analytically predicted value as given by Equation (24), i.e.,<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x87.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x88.png" xlink:type="simple"/></inline-formula>. The value of the constant C in Equation (25) is calculated by equating the present time value of the scale factor to unity. In this way, the value of C is determined to be<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x87.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x88.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x89.png" xlink:type="simple"/></inline-formula>. A plot of scale factors from Equations (25) and (29) is presented in <xref ref-type="fig" rid="fig2">Figure 2</xref>.</p><fig id="fig1"  position="float"><label><xref ref-type="fig" rid="fig1">Figure 1</xref></label><caption><title> Evolution of the scale factor</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/10-4500521x90.png"/></fig><fig id="fig2"  position="float"><label><xref ref-type="fig" rid="fig2">Figure 2</xref></label><caption><title> Evolution of the scale factor with time</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/10-4500521x91.png"/></fig><p>The time <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x92.png" xlink:type="simple"/></inline-formula> in <xref ref-type="fig" rid="fig2">Figure 2</xref> represents the present time. For the new analytical solution, shown as a solid line in this figure, the zero time of the scale factor occurs at the time<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x92.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x93.png" xlink:type="simple"/></inline-formula>. Equation (29) describes the evolution of the scale factor for a flat universe including all its ingredients. The scale factor calculated from Equation (25), shown as a dashed line, is for a universe composed of matter and Λ only. Its zero time occurs at<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x92.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x93.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x94.png" xlink:type="simple"/></inline-formula>. The difference between these two analytical solutions is due to the fact that one of them includes all the ingredients of the universe and the other one considers a universe composed of a specified mix of only two ingredients, matter and Λ.</p><sec id="s4_1"><title>4.1. Comparisons of the New Solution with ΛCDM-Based Models</title><p>The ΛCDM-based models characterize the universe with a limited number of energy density parameters as fractions of constituent ingredients. The values of these fractions are estimated through finding the optimum fit to the observationally measured data. The results are presented in terms of distance modulus versus redshift. Here, a comparison of the variation of scale factors versus redshift will be carried out first. The relation between the scale factor and the redshift, z, is defined by</p><disp-formula id="scirp.65213-formula271"><label>(30)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/10-4500521x95.png"  xlink:type="simple"/></disp-formula><p>Thus</p><disp-formula id="scirp.65213-formula272"><label>(31)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/10-4500521x96.png"  xlink:type="simple"/></disp-formula><p>To express the scale factor given by Equation (29) in terms of redshift, substitution for the scale factor, a, from Equation (29) back into Equation (31) yields the relation between the red shift, z, and the time <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x97.png" xlink:type="simple"/></inline-formula> as</p><disp-formula id="scirp.65213-formula273"><label>(32)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/10-4500521x98.png"  xlink:type="simple"/></disp-formula><p>Using the above equation, the variation of time versus the redshift is presented in <xref ref-type="fig" rid="fig3">Figure 3</xref>.</p><p>In <xref ref-type="fig" rid="fig3">Figure 3</xref> the present time, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x99.png" xlink:type="simple"/></inline-formula>, corresponds to the redshift,<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x99.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x100.png" xlink:type="simple"/></inline-formula>. Consistent with this, for comparison with observational data, a transformation is made such that <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x99.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x100.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x101.png" xlink:type="simple"/></inline-formula> would correspond to the present time,<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x99.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x100.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x101.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x102.png" xlink:type="simple"/></inline-formula>. To this end the values of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x99.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x100.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x101.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x102.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x103.png" xlink:type="simple"/></inline-formula> from Equation (29) and the values of the redshifts z from Equation (32)</p><p>are tabulated for values of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x104.png" xlink:type="simple"/></inline-formula> varying from zero to one. Next the tabulated values of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x104.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x105.png" xlink:type="simple"/></inline-formula> are plotted</p><fig id="fig3"  position="float"><label><xref ref-type="fig" rid="fig3">Figure 3</xref></label><caption><title> Variation of time with the redshift</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/10-4500521x106.png"/></fig><p>versus the tabulated values of the redshift, z, in <xref ref-type="fig" rid="fig4">Figure 4</xref>. Through this process, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x107.png" xlink:type="simple"/></inline-formula>corresponds to the present time,<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x107.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x108.png" xlink:type="simple"/></inline-formula>.</p><p>For ΛCDM-based models, considering Equation (30), and rewriting Friedmann Equation (2) in terms of fractions of constituent densities, for a universe containing mass, energy, radiation and curvature, one obtains the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x109.png" xlink:type="simple"/></inline-formula> in terms of the redshift as</p><disp-formula id="scirp.65213-formula274"><label>(33)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/10-4500521x110.png"  xlink:type="simple"/></disp-formula><p>Using the above equation, the values of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x111.png" xlink:type="simple"/></inline-formula> are plotted versus z in <xref ref-type="fig" rid="fig4">Figure 4</xref> for two sets of ΛCDM-based parameters, estimated by the Plank Collaboration [<xref ref-type="bibr" rid="scirp.65213-ref4">4</xref>] , as presented in <xref ref-type="table" rid="table1">Table 1</xref>. As seen from <xref ref-type="fig" rid="fig4">Figure 4</xref>, the ΛCDM-based curves are consistent with the analytical curve. But they are not identical to the analytical curve. There are two reasons for not being identical. The first reason is the differences in the fractions of ingredients included in the models. The second reason is the fact that the initial times for the scale factors of the - based models are not defined.</p><p>In the next subsection the analytical curve and the curves based on ΛCDM parameterization are compared with the observational data.</p><fig id="fig4"  position="float"><label><xref ref-type="fig" rid="fig4">Figure 4</xref></label><caption><title> Comparisons of scale factors</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/10-4500521x112.png"/></fig><table-wrap id="table1" ><label><xref ref-type="table" rid="table1">Table 1</xref></label><caption><title> Cosmological parameters used for ΛCDM based models</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >Parameters</th><th align="center" valign="middle" >ΛCDM-1 Plank + WP + high L + BAO</th><th align="center" valign="middle" >ΛCDM-2 WMAP-9 + BAO</th></tr></thead><tr><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x113.png" xlink:type="simple"/></inline-formula></td><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x114.png" xlink:type="simple"/></inline-formula></td><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x115.png" xlink:type="simple"/></inline-formula></td></tr><tr><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x116.png" xlink:type="simple"/></inline-formula></td><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x117.png" xlink:type="simple"/></inline-formula></td><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x118.png" xlink:type="simple"/></inline-formula></td></tr><tr><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x119.png" xlink:type="simple"/></inline-formula></td><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x120.png" xlink:type="simple"/></inline-formula></td><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x121.png" xlink:type="simple"/></inline-formula></td></tr><tr><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x122.png" xlink:type="simple"/></inline-formula></td><td align="center" valign="middle" >0.0</td><td align="center" valign="middle" >0.0</td></tr><tr><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x123.png" xlink:type="simple"/></inline-formula></td><td align="center" valign="middle" >0.0</td><td align="center" valign="middle" >0.0</td></tr></tbody></table></table-wrap></sec><sec id="s4_2"><title>4.2. Comparison of the New Solution with Observational Data</title><p>In this part the curve of the analytical scale factor given by Equation (29), transformed through Equation (32), is compared with the curves based on ΛCDM, as given by Equation (33), for the two different sets of ingredients presented in <xref ref-type="table" rid="table1">Table 1</xref>. To check how well these curves represent the reality, the following three sets of observational data will be used:</p><p>1) A set of 557 SNe data with redshifts from a low of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x124.png" xlink:type="simple"/></inline-formula> to a maximum of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x124.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x125.png" xlink:type="simple"/></inline-formula>, as reported in 2010 in the Union2 Compilation [<xref ref-type="bibr" rid="scirp.65213-ref11">11</xref>] ;</p><p>2) A set of 394 extragalactic distances to 349 galaxies at cosmological redshifts significantly higher than the Union2 Compilation with redshifts from a low of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x126.png" xlink:type="simple"/></inline-formula> to a maximum of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x126.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x127.png" xlink:type="simple"/></inline-formula>, as reported in 2008 by Mador and Steer [<xref ref-type="bibr" rid="scirp.65213-ref12">12</xref>] ;</p><p>3) A set of data for a quasar and the three most distant recently confirmed galaxies, as presented in <xref ref-type="table" rid="table2">Table 2</xref>.</p><p>To compare with the aforementioned observational data, the scale factors have to be presented in terms of distance modulus and redshift. The SNe and the Union2 data are already available in terms of distance modulus and redshift. The data for the galaxies and for the quasar are listed in <xref ref-type="table" rid="table2">Table 2</xref>, and, for the new analytical solution, the data for the scale factors in terms of distance modulus and redshift are represented through the following relation</p><disp-formula id="scirp.65213-formula275"><label>(34)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/10-4500521x128.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x129.png" xlink:type="simple"/></inline-formula> represents distance modulus; a represents the scale factor; <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x129.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x130.png" xlink:type="simple"/></inline-formula>is in megaparsecs and the factor <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x129.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x130.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x131.png" xlink:type="simple"/></inline-formula> represents the effects of observational data such as source luminosity, and data processing correc-</p><p>tions including the instrument corrections and the K-correction. These are well known corrections and they are</p><p>considered in various ways [<xref ref-type="bibr" rid="scirp.65213-ref17">17</xref>] - [<xref ref-type="bibr" rid="scirp.65213-ref20">20</xref>] . We evaluate the factor <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x132.png" xlink:type="simple"/></inline-formula> through matching of the analytical curve</p><p>with the first set of the observational data. Then we check the validity of its value through comparisons with the</p><p>second and third sets of observational data as well as with the ΛCDM-based curves. To evaluate<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x133.png" xlink:type="simple"/></inline-formula>, using</p><p>the analytical curve, we only need to have the value for the Hubble constant. The recent estimated values of the</p><p>Hubble constant based on observational data are: (the Seven-Year Wilkinson Microwave Anisotropy Probe [<xref ref-type="bibr" rid="scirp.65213-ref21">21</xref>] , 2011),<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x134.png" xlink:type="simple"/></inline-formula>; (the Planck Collaboration [<xref ref-type="bibr" rid="scirp.65213-ref4">4</xref>] , 2014),<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x134.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x135.png" xlink:type="simple"/></inline-formula>; (the Nine-Year Wilkinson Microwave Anisotropy Probe [<xref ref-type="bibr" rid="scirp.65213-ref22">22</xref>] , 2013),<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x134.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x135.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x136.png" xlink:type="simple"/></inline-formula>; and (the Megamaser Cosmology Project IV, [<xref ref-type="bibr" rid="scirp.65213-ref23">23</xref>] , 2013),<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x134.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x135.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x136.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x137.png" xlink:type="simple"/></inline-formula>. The average of these four values is<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x134.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x135.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x136.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x137.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x138.png" xlink:type="simple"/></inline-formula>. But most recently (Mostaghel [<xref ref-type="bibr" rid="scirp.65213-ref5">5</xref>] , 2015), the value of the Hubble constant is analytically estimated to be</p><disp-formula id="scirp.65213-formula276"><label>(35)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/10-4500521x139.png"  xlink:type="simple"/></disp-formula><p>Because this value is remarkably consistent with the observationally estimated values, we will use this value and substitute it together with the values of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x140.png" xlink:type="simple"/></inline-formula>, as obtained through Equations (29) and (32), into Equation (34). Through matching the curve of Equation (34) with the first set of observational data presented in <xref ref-type="fig" rid="fig5">Figure 5</xref>, the factor <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x140.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x141.png" xlink:type="simple"/></inline-formula> is found to be given by</p><table-wrap id="table2" ><label><xref ref-type="table" rid="table2">Table 2</xref></label><caption><title> Data for recently confirmed galaxies</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >Name</th><th align="center" valign="middle" >Reference</th><th align="center" valign="middle" >Light Travel Distance, Gly</th><th align="center" valign="middle" >Redshift, z</th></tr></thead><tr><td align="center" valign="middle" >Galaxy, EGSY8p7</td><td align="center" valign="middle" >Zitrin, 2015 [<xref ref-type="bibr" rid="scirp.65213-ref13">13</xref>]</td><td align="center" valign="middle" >13.2</td><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x142.png" xlink:type="simple"/></inline-formula></td></tr><tr><td align="center" valign="middle" >Galaxy, EGS-zs8-1</td><td align="center" valign="middle" >Oesch, 2015 [<xref ref-type="bibr" rid="scirp.65213-ref14">14</xref>]</td><td align="center" valign="middle" >13.044</td><td align="center" valign="middle" >7.730</td></tr><tr><td align="center" valign="middle" >Galaxy, z8GND 5296</td><td align="center" valign="middle" >Finkelstein, 2013 [<xref ref-type="bibr" rid="scirp.65213-ref15">15</xref>]</td><td align="center" valign="middle" >13.02</td><td align="center" valign="middle" >7.51</td></tr><tr><td align="center" valign="middle" >Quasar, ULAS J1120+0641</td><td align="center" valign="middle" >Matson, 2011 [<xref ref-type="bibr" rid="scirp.65213-ref16">16</xref>]</td><td align="center" valign="middle" >12.9</td><td align="center" valign="middle" >7.085</td></tr></tbody></table></table-wrap><fig id="fig5"  position="float"><label><xref ref-type="fig" rid="fig5">Figure 5</xref></label><caption><title> Hubble diagram, evaluation of the factor<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x144.png" xlink:type="simple"/></inline-formula></title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/10-4500521x143.png"/></fig><disp-formula id="scirp.65213-formula277"><label>(36)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/10-4500521x145.png"  xlink:type="simple"/></disp-formula><p>As can be seen from <xref ref-type="fig" rid="fig5">Figure 5</xref>, with this <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x146.png" xlink:type="simple"/></inline-formula> the analytically derived scale factor fits the first set of observational data remarkably well. Substitution for <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x146.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x147.png" xlink:type="simple"/></inline-formula> from the above equation back into Equation (35) yields the distance modulus as</p><disp-formula id="scirp.65213-formula278"><label>(37)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/10-4500521x148.png"  xlink:type="simple"/></disp-formula><p>where<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x149.png" xlink:type="simple"/></inline-formula>, c is in<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x149.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x150.png" xlink:type="simple"/></inline-formula>, and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x149.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x150.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x151.png" xlink:type="simple"/></inline-formula> is in<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x149.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x150.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x151.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x152.png" xlink:type="simple"/></inline-formula>. The above relation directly gives the distance modulus in terms of the scale factor and the redshift.</p><p>Now, to check the validity of the factor<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x153.png" xlink:type="simple"/></inline-formula>, we include the second and the third sets of observational data. Equation (37) will be used to compare the analytical solution with the ΛCDM-based models and the observational data. The parameters for the ΛCDM curves are given in <xref ref-type="table" rid="table1">Table 1</xref>. For the analytical solution, as mentioned above, we use<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x153.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x154.png" xlink:type="simple"/></inline-formula>. The three sets of observational data, the analytical curve based</p><p>on Equations (29) and (32), and the two ΛCDM curves based on Equation (33), are presented in Figures 6-9. As seen from these figures, in all cases, the analytical curve is remarkably consistent with the observational data as well as with the ΛCDM-based curves. The log-linear plots and the linear plots show how well the curves represent the observational data at the low and high values of the redshifts respectively.</p><p>The excellent match of the analytical curve and the ΛCDM curves with the second and the third set of the observational data validates Equation (36) representing the factor<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x155.png" xlink:type="simple"/></inline-formula>. It also confirms the analytically eva-</p><p>luated value for the Hubble constant as given in Equation (35). It should be noted that, except for the flatness assumption, the analytical solution is completely general. It includes all the ingredients forming the universe. The ΛCDM-based solutions only consider specific combinations of limited numbers of ingredients.</p></sec></sec><sec id="s5"><title>5. Summary and Remarks</title><p>The value of the energy density parameter was analytically estimated to be<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/10-4500521x156.png" xlink:type="simple"/></inline-formula>. This value is essentially identical to the estimated value based on the observational data. This fact and the remarkable consis-</p><fig id="fig6"  position="float"><label><xref ref-type="fig" rid="fig6">Figure 6</xref></label><caption><title> Hubble diagram, comparison of analytical and ΛCDM-1 curves with observational data</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/10-4500521x157.png"/></fig><fig id="fig7"  position="float"><label><xref ref-type="fig" rid="fig7">Figure 7</xref></label><caption><title> Hubble diagram, comparison of analytical and ΛCDM-1 curves with observational data</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/10-4500521x158.png"/></fig><p>tency of the analytical solution with the observational data, as well as with the -based models, provide the necessary confidence in the fidelity of the analytical solution in the representation of reality.</p><p>The pressure is cancelled from the Friedmann acceleration equation through the contribution of the cosmological constant. As the result, Equation (28) may be interpreted as a kinematic equation. Its solution, Equation</p><fig id="fig8"  position="float"><label><xref ref-type="fig" rid="fig8">Figure 8</xref></label><caption><title> Hubble diagram, comparison of analytical and ΛCDM-2 curves with observational data</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/10-4500521x159.png"/></fig><fig id="fig9"  position="float"><label><xref ref-type="fig" rid="fig9">Figure 9</xref></label><caption><title> Hubble diagram, comparison of analytical and ΛCDM-2 curves with observational data</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/10-4500521x160.png"/></fig><p>(29) describes the evolution of the expansion of space. As such, this equation provides an alternative way of describing the expansion of space without involving the controversial dark energy.</p></sec><sec id="s6"><title>Cite this paper</title><p>Naser Mostaghel, (2016) A New Solution for the Friedmann Equations. International Journal of Astronomy and Astrophysics,06,122-134. doi: 10.4236/ijaa.2016.61010</p></sec></body><back><ref-list><title>References</title><ref id="scirp.65213-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Carroll, S.M. (2013) Why Does Dark Energy Make the Universe Accelerate? Posted on 16 November. http://www.preposterousuniverse.com/blog/2013/11/16/</mixed-citation></ref><ref id="scirp.65213-ref2"><label>2</label><mixed-citation publication-type="other" xlink:type="simple">Christiansen, J.L. and Siver, A. 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