<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article  PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd"><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article"><front><journal-meta><journal-id journal-id-type="publisher-id">JMP</journal-id><journal-title-group><journal-title>Journal of Modern Physics</journal-title></journal-title-group><issn pub-type="epub">2153-1196</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/jmp.2017.82013</article-id><article-id pub-id-type="publisher-id">JMP-74074</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 Tired Light/Contracting Universe Model from the Union2.1 Supernovae Data
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>John</surname><given-names>Glover</given-names></name><xref ref-type="aff" rid="aff1"><sub>1</sub></xref></contrib></contrib-group><aff id="aff1"><label>1</label><addr-line>Chemical Engineering Department, Loughborough University, Loughborough, UK</addr-line></aff><author-notes><corresp id="cor1">* E-mail:</corresp></author-notes><pub-date pub-type="epub"><day>13</day><month>02</month><year>2017</year></pub-date><volume>08</volume><issue>02</issue><fpage>147</fpage><lpage>155</lpage><history><date date-type="received"><day>January</day>	<month>2,</month>	<year>2017</year></date><date date-type="rev-recd"><day>Accepted:</day>	<month>February</month>	<year>10,</year>	</date><date date-type="accepted"><day>February</day>	<month>13,</month>	<year>2017</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>
 
 
  A tired light/contracting universe (TLCU) model is shown to be an excellent fit to the redshift/distance modulus data for the 580 supernovae 1a in the Union2.1 compilation. The data reveal that the Milky Way is in a static region with a radius of about 450 Mpc. Beyond the static region the universe is contracting with a space velocity which is linearly proportional to distance over the whole range of the data (
  K=&amp;minus;7.6+2.3km&amp;sdot;s<sup>&amp;minus;1</sup>&amp;sdot;Mpc<sup>&amp;minus;1</sup>). The other constant of the model is the Hubble constant for which a value of 
  H=69.51 &#177;0.86 km
  &amp;sdot;s
  <sup>&amp;minus;1</sup>
  &amp;sdot;Mpc
  <sup>&amp;minus;1 </sup>is obtained. The fit of the TLCU model to the Union2.1 data is at least as good as the fit of the two constant ΛCDM model to the same data. A formula for photon travel distance is derived and an experiment for the possible detection of the tired light process is proposed.
 
</p></abstract><kwd-group><kwd>Cosmology</kwd><kwd> Observations</kwd><kwd> Theory</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Theory [<xref ref-type="bibr" rid="scirp.74074-ref1">1</xref>] predicts that the universe is either expanding or contracting with a space velocity which is linearly proportional to distance. An expansion may continue for ever or it may halt and then contract giving rise to the possibility of a “periodic world”.</p><p>When it was observed that the redshift and distance for galaxies beyond the Local Group had a linear relationship [<xref ref-type="bibr" rid="scirp.74074-ref2">2</xref>] the expanding universe theory became established. Observations of supernovae 1a show that at higher redshifts [<xref ref-type="bibr" rid="scirp.74074-ref3">3</xref>] , [<xref ref-type="bibr" rid="scirp.74074-ref4">4</xref>] the distances measured are greater than expected by the expanding universe theory and this is interpreted as an accelerating expansion for which a new force called “dark energy” is proposed.</p><p>The tired light theory [<xref ref-type="bibr" rid="scirp.74074-ref5">5</xref>] is an alternative explanation for the systematic redshift. The viewpoint on the supernovae 1a observations from the tired light theory is that for a given distance the observed redshift is less than expected as a result of the blueshift of a contracting universe. Hence it is suggested that the new physics required by the supernovae 1a observations may possibly be the old idea of tired light instead of the new idea of dark energy.</p><p>A tired light/contracting universe (TLCU) model is developed here using the Union2.1 supernovae 1a data [<xref ref-type="bibr" rid="scirp.74074-ref6">6</xref>] and compared to the ΛCDM model. The TLCU model uses photon travel distance for which a formula is derived. A possible mechanism for the tired light effect is discussed and an experiment to test this mechanism is proposed.</p></sec><sec id="s2"><title>2. The TLCU Model</title><p>The TLCU model is built on the idea [<xref ref-type="bibr" rid="scirp.74074-ref7">7</xref>] that the observed systematic redshift (z) has two components</p><disp-formula id="scirp.74074-formula22"><label>(1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-7503044x4.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x5.png" xlink:type="simple"/></inline-formula> is the result of an energy loss process and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x6.png" xlink:type="simple"/></inline-formula> is the result of space contraction. Assuming that photons lose energy by a first order rate process [<xref ref-type="bibr" rid="scirp.74074-ref8">8</xref>] the tired light component is given by</p><disp-formula id="scirp.74074-formula23"><label>(2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-7503044x7.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.74074-formula24"><graphic  xlink:href="http://html.scirp.org/file/1-7503044x8.png"  xlink:type="simple"/></disp-formula><p><sup>1</sup>The Hubble constant used in the TLCU model is a constant of nature and assumed to be independent of time and space. The usual units used for the Hubble constant are <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x9.png" xlink:type="simple"/></inline-formula> although the SI unit is s<sup>−1</sup>, which is characteristic of a first order rate process. (<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x10.png" xlink:type="simple"/></inline-formula>).</p><p>where d is the photon travel distance, H is the Hubble constant<sup>1</sup> and c is the speed of light. The distance between the emitter and observer at the moment the photon is emitted (<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x11.png" xlink:type="simple"/></inline-formula>) is here called the “initial distance” and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x12.png" xlink:type="simple"/></inline-formula> for low values of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x13.png" xlink:type="simple"/></inline-formula>. The exact relationship between <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x14.png" xlink:type="simple"/></inline-formula> and d is considered later. Assuming a flat (i.e. Euclidean) universe the initial distance is related [<xref ref-type="bibr" rid="scirp.74074-ref9">9</xref>] to the luminosity distance (D) by</p><disp-formula id="scirp.74074-formula25"><label>(3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-7503044x15.png"  xlink:type="simple"/></disp-formula><p>The luminosity distance (D) is obtained from the distance modulus (dm) by the standard relationship.</p><disp-formula id="scirp.74074-formula26"><label>(4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-7503044x16.png"  xlink:type="simple"/></disp-formula><p>The distance modulus (dm) is defined as<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x17.png" xlink:type="simple"/></inline-formula>, where m is the observed apparent magnitude of an object and M is it’s absolute magnitude. For supernovae 1a “m” is the peak observed apparent magnitude (with appropriate corrections).</p><sec id="s2_1"><title>2.1. Preliminary Calculations</title><p>Initially <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x18.png" xlink:type="simple"/></inline-formula> was calculated from the redshift and distance modulus data for each of the 580 SN 1a in the Union2.1 compilation using Equations (1) to (4) and with the assumptions that <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x19.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x19.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x20.png" xlink:type="simple"/></inline-formula>. The results of the calculations are shown in <xref ref-type="fig" rid="fig1">Figure 1</xref>.</p><p>The 580 values of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x21.png" xlink:type="simple"/></inline-formula> consist of 158 positive values (redshifts) and 422 negative values (blueshifts). In a static universe <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x21.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x22.png" xlink:type="simple"/></inline-formula> would consist of an equal number of redshifts/blueshifts and the 158/422 split rejects a static universe (<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x21.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x22.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x23.png" xlink:type="simple"/></inline-formula>). Since <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x21.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x22.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x23.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x24.png" xlink:type="simple"/></inline-formula> is essentially negative the initial assumption of a contracting universe is confirmed.</p><p>Although the overall picture is of a contracting universe the local situation is different. There are 176 supernovae with <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x25.png" xlink:type="simple"/></inline-formula> for which the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x25.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x26.png" xlink:type="simple"/></inline-formula> values show 78 redshifts and 98 blueshifts which is consistent (<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x25.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x26.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x27.png" xlink:type="simple"/></inline-formula>) with an even split. So the next conclusion is that the Milky Way is situated in a static region of about 450 Mpc radius.</p></sec><sec id="s2_2"><title>2.2. The Final Model</title><p>In a gravitationally bound region of space the force of Newtonian gravity is greater than the cosmic force of expansion/contraction and although the region as a whole will take part in the universal cosmic expansion/contraction the effect of cosmic expansion/contraction cannot be measured within the region. It is now assumed that the static region extending to about 450 Mpc around the Milky Way is gravitationally bound. For the purpose of the model it is assumed that the Milky Way is located at the center of a static sphere with a radius of 450 Mpc. In order to be consistent with the observations it is also assumed that the cosmic contraction starts at the edge of the static sphere. For a cosmic con- traction the velocity of contraction is proportional to distance, so that</p><disp-formula id="scirp.74074-formula27"><label>(5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-7503044x28.png"  xlink:type="simple"/></disp-formula><fig id="fig1"  position="float"><label><xref ref-type="fig" rid="fig1">Figure 1</xref></label><caption><title> 580 values of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x30.png" xlink:type="simple"/></inline-formula> from the Union2.1 supernovae data with<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x30.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x31.png" xlink:type="simple"/></inline-formula></title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-7503044x29.png"/></fig><p>where k (km・s<sup>−1</sup>・Mpc<sup>−1</sup>) is the constant for cosmic contraction. Within the static region<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x32.png" xlink:type="simple"/></inline-formula>, but, beyond the static region it is necessary to allow for the contraction that occurs during the photon travel time. The relationship between<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x32.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x33.png" xlink:type="simple"/></inline-formula>, k and d is derived in Appendix 1, from which, Equation (11) re-arranged as</p><disp-formula id="scirp.74074-formula28"><label>(6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-7503044x34.png"  xlink:type="simple"/></disp-formula><p>is more convenient for finding d from <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x35.png" xlink:type="simple"/></inline-formula> and k by repeated substitution. Equation (6) was used to calculate that part of the photon travel distance which is beyond the static region. The values of H and k for the TLCU model were found by fitting the model to the Union2.1 data. The sum of the weighted squares of the the dm residuals (S) is given by</p><disp-formula id="scirp.74074-formula29"><label>(7)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-7503044x36.png"  xlink:type="simple"/></disp-formula><p>where the weighting factor (w) is proportional to the inverse square of the estimated error in dm. For the Union2.1 data (<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x37.png" xlink:type="simple"/></inline-formula>), the values of the constants which minimize S are <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x37.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x38.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x37.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x38.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x39.png" xlink:type="simple"/></inline-formula>. The rms weighted residual<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x37.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x38.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x39.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x40.png" xlink:type="simple"/></inline-formula>. while the rms un-weighted residual<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x37.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x38.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x39.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x40.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x41.png" xlink:type="simple"/></inline-formula>.</p><p><xref ref-type="fig" rid="fig1">Figure 1</xref> shows a large scatter in <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x42.png" xlink:type="simple"/></inline-formula> so the data were binned in order to make the relationship between velocity of contraction and distance more precise. The 580 SN 1a were sorted into z order and divided into 29 bins each containing 20 SN 1a. The weighted average redshift and distance modulus were calculated for each bin (see <xref ref-type="table" rid="table1">Table 1</xref>). The procedure for finding H and k was repeated using the bin averages of redshift and distance modulus and gave <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x42.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x43.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x42.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x43.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x44.png" xlink:type="simple"/></inline-formula> with the rms of the residual<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x42.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x43.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x44.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x45.png" xlink:type="simple"/></inline-formula>. The values of the contraction velocity calculated from the binned data using using <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x42.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x43.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x44.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x45.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x46.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x42.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x43.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x44.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x45.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x46.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x47.png" xlink:type="simple"/></inline-formula> are shown in <xref ref-type="fig" rid="fig2">Figure 2</xref>. It is seen that the contraction velocity has an approximate linear relationship with distance beyond the static region over the whole range of the Union2.1 data. Hence the assumptions on which the model is based are consistent with the observed data. <xref ref-type="fig" rid="fig2">Figure 2</xref> also shows a hint of periodicity in the velocity/distance relationship.</p></sec></sec><sec id="s3"><title>3. Comparison of TLCU and ΛCDM Models</title><p>In the two constant ΛCDM model the initial distance (from Equation (13) of ref. [<xref ref-type="bibr" rid="scirp.74074-ref10">10</xref>] ) is</p><disp-formula id="scirp.74074-formula30"><label>(8)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-7503044x48.png"  xlink:type="simple"/></disp-formula><p>In order to compare the models on the same basis the constants for the ΛCDM model were found by fitting Equation (8) to the Union2.1 data using the best fit criterium (Equation (6)). This gave <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x49.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x49.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x50.png" xlink:type="simple"/></inline-formula> with a rms weighted residual <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x49.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x50.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x51.png" xlink:type="simple"/></inline-formula> while the rms un-</p><table-wrap id="table1" ><label><xref ref-type="table" rid="table1">Table 1</xref></label><caption><title> The bin Hubble constants for the TLCU and ΛCDM models</title></caption><table><tbody><thead><tr><th align="center" valign="middle"  rowspan="2"  >z</th><th align="center" valign="middle"  rowspan="2"  >dm</th><th align="center" valign="middle"  rowspan="2"  >d<sub>o</sub><sub> </sub> Mpc</th><th align="center" valign="middle"  rowspan="2"  >d Mpc</th><th align="center" valign="middle"  rowspan="2"  >z<sub>c</sub></th><th align="center" valign="middle"  rowspan="2"  >z<sub>tl</sub></th><th align="center" valign="middle"  colspan="2"  >TLCU</th><th align="center" valign="middle"  colspan="2"  >ΛCDM</th></tr></thead><tr><td align="center" valign="middle" >H</td><td align="center" valign="middle" >resid.</td><td align="center" valign="middle" >H<sub>o</sub></td><td align="center" valign="middle" >resid.</td></tr><tr><td align="center" valign="middle" >(1)</td><td align="center" valign="middle" >(2)</td><td align="center" valign="middle" >(3)</td><td align="center" valign="middle" >(4)</td><td align="center" valign="middle" >(5)</td><td align="center" valign="middle" >(6)</td><td align="center" valign="middle" >(7)</td><td align="center" valign="middle" >(8)</td><td align="center" valign="middle" >(9)</td><td align="center" valign="middle" >(10)</td></tr><tr><td align="center" valign="middle" >0.0157</td><td align="center" valign="middle" >34.158</td><td align="center" valign="middle" >67</td><td align="center" valign="middle" >67</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >0.0157</td><td align="center" valign="middle" >69.99</td><td align="center" valign="middle" >−0.79</td><td align="center" valign="middle" >70.31</td><td align="center" valign="middle" >−0.31</td></tr><tr><td align="center" valign="middle" >0.0192</td><td align="center" valign="middle" >34.589</td><td align="center" valign="middle" >81</td><td align="center" valign="middle" >81</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >0.0192</td><td align="center" valign="middle" >70.33</td><td align="center" valign="middle" >−1.13</td><td align="center" valign="middle" >70.71</td><td align="center" valign="middle" >−0.71</td></tr><tr><td align="center" valign="middle" >0.0231</td><td align="center" valign="middle" >35.033</td><td align="center" valign="middle" >99</td><td align="center" valign="middle" >99</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >0.0231</td><td align="center" valign="middle" >69.05</td><td align="center" valign="middle" >0.15</td><td align="center" valign="middle" >69.51</td><td align="center" valign="middle" >0.49</td></tr><tr><td align="center" valign="middle" >0.0260</td><td align="center" valign="middle" >35.294</td><td align="center" valign="middle" >112</td><td align="center" valign="middle" >112</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >0.0260</td><td align="center" valign="middle" >68.99</td><td align="center" valign="middle" >0.21</td><td align="center" valign="middle" >69.51</td><td align="center" valign="middle" >0.49</td></tr><tr><td align="center" valign="middle" >0.0304</td><td align="center" valign="middle" >35.659</td><td align="center" valign="middle" >131</td><td align="center" valign="middle" >131</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >0.0304</td><td align="center" valign="middle" >68.34</td><td align="center" valign="middle" >0.86</td><td align="center" valign="middle" >68.93</td><td align="center" valign="middle" >1.07</td></tr><tr><td align="center" valign="middle" >0.0338</td><td align="center" valign="middle" >35.862</td><td align="center" valign="middle" >144</td><td align="center" valign="middle" >144</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >0.0338</td><td align="center" valign="middle" >69.21</td><td align="center" valign="middle" >−0.01</td><td align="center" valign="middle" >69.88</td><td align="center" valign="middle" >0.12</td></tr><tr><td align="center" valign="middle" >0.0437</td><td align="center" valign="middle" >36.409</td><td align="center" valign="middle" >183</td><td align="center" valign="middle" >183</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >0.0437</td><td align="center" valign="middle" >69.90</td><td align="center" valign="middle" >−0.70</td><td align="center" valign="middle" >70.76</td><td align="center" valign="middle" >−0.76</td></tr><tr><td align="center" valign="middle" >0.0597</td><td align="center" valign="middle" >37.109</td><td align="center" valign="middle" >249</td><td align="center" valign="middle" >249</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >0.0597</td><td align="center" valign="middle" >69.72</td><td align="center" valign="middle" >−0.52</td><td align="center" valign="middle" >70.87</td><td align="center" valign="middle" >−0.87</td></tr><tr><td align="center" valign="middle" >0.0894</td><td align="center" valign="middle" >38.033</td><td align="center" valign="middle" >371</td><td align="center" valign="middle" >371</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >0.0894</td><td align="center" valign="middle" >69.15</td><td align="center" valign="middle" >0.05</td><td align="center" valign="middle" >70.82</td><td align="center" valign="middle" >−0.82</td></tr><tr><td align="center" valign="middle" >0.1287</td><td align="center" valign="middle" >38.894</td><td align="center" valign="middle" >532</td><td align="center" valign="middle" >532</td><td align="center" valign="middle" >−0.0020</td><td align="center" valign="middle" >0.1307</td><td align="center" valign="middle" >69.18</td><td align="center" valign="middle" >0.02</td><td align="center" valign="middle" >70.49</td><td align="center" valign="middle" >−0.49</td></tr><tr><td align="center" valign="middle" >0.1632</td><td align="center" valign="middle" >39.444</td><td align="center" valign="middle" >665</td><td align="center" valign="middle" >664</td><td align="center" valign="middle" >−0.0051</td><td align="center" valign="middle" >0.1683</td><td align="center" valign="middle" >70.20</td><td align="center" valign="middle" >−1.00</td><td align="center" valign="middle" >70.94</td><td align="center" valign="middle" >−0.94</td></tr><tr><td align="center" valign="middle" >0.1976</td><td align="center" valign="middle" >39.935</td><td align="center" valign="middle" >810</td><td align="center" valign="middle" >807</td><td align="center" valign="middle" >−0.0085</td><td align="center" valign="middle" >0.2061</td><td align="center" valign="middle" >69.58</td><td align="center" valign="middle" >−0.38</td><td align="center" valign="middle" >69.96</td><td align="center" valign="middle" >0.04</td></tr><tr><td align="center" valign="middle" >0.2352</td><td align="center" valign="middle" >40.378</td><td align="center" valign="middle" >964</td><td align="center" valign="middle" >957</td><td align="center" valign="middle" >−0.0122</td><td align="center" valign="middle" >0.2474</td><td align="center" valign="middle" >69.22</td><td align="center" valign="middle" >−0.02</td><td align="center" valign="middle" >69.44</td><td align="center" valign="middle" >0.56</td></tr><tr><td align="center" valign="middle" >0.2641</td><td align="center" valign="middle" >40.646</td><td align="center" valign="middle" >1065</td><td align="center" valign="middle" >1056</td><td align="center" valign="middle" >−0.0146</td><td align="center" valign="middle" >0.2786</td><td align="center" valign="middle" >69.76</td><td align="center" valign="middle" >−0.56</td><td align="center" valign="middle" >70.04</td><td align="center" valign="middle" >−0.04</td></tr><tr><td align="center" valign="middle" >0.2914</td><td align="center" valign="middle" >40.899</td><td align="center" valign="middle" >1171</td><td align="center" valign="middle" >1159</td><td align="center" valign="middle" >−0.0171</td><td align="center" valign="middle" >0.3085</td><td align="center" valign="middle" >69.52</td><td align="center" valign="middle" >−0.32</td><td align="center" valign="middle" >69.80</td><td align="center" valign="middle" >0.20</td></tr><tr><td align="center" valign="middle" >0.3243</td><td align="center" valign="middle" >41.135</td><td align="center" valign="middle" >1274</td><td align="center" valign="middle" >1258</td><td align="center" valign="middle" >−0.0195</td><td align="center" valign="middle" >0.3438</td><td align="center" valign="middle" >70.42</td><td align="center" valign="middle" >−1.22</td><td align="center" valign="middle" >70.88</td><td align="center" valign="middle" >−0.88</td></tr><tr><td align="center" valign="middle" >0.3554</td><td align="center" valign="middle" >41.416</td><td align="center" valign="middle" >1416</td><td align="center" valign="middle" >1395</td><td align="center" valign="middle" >−0.0229</td><td align="center" valign="middle" >0.3782</td><td align="center" valign="middle" >68.96</td><td align="center" valign="middle" >0.24</td><td align="center" valign="middle" >69.33</td><td align="center" valign="middle" >0.67</td></tr><tr><td align="center" valign="middle" >0.3897</td><td align="center" valign="middle" >41.671</td><td align="center" valign="middle" >1553</td><td align="center" valign="middle" >1526</td><td align="center" valign="middle" >−0.0261</td><td align="center" valign="middle" >0.4159</td><td align="center" valign="middle" >68.33</td><td align="center" valign="middle" >0.87</td><td align="center" valign="middle" >68.73</td><td align="center" valign="middle" >1.27</td></tr><tr><td align="center" valign="middle" >0.4221</td><td align="center" valign="middle" >41.862</td><td align="center" valign="middle" >1658</td><td align="center" valign="middle" >1625</td><td align="center" valign="middle" >−0.0286</td><td align="center" valign="middle" >0.4507</td><td align="center" valign="middle" >68.66</td><td align="center" valign="middle" >0.54</td><td align="center" valign="middle" >69.19</td><td align="center" valign="middle" >0.81</td></tr><tr><td align="center" valign="middle" >0.4538</td><td align="center" valign="middle" >42.076</td><td align="center" valign="middle" >1789</td><td align="center" valign="middle" >1749</td><td align="center" valign="middle" >−0.0317</td><td align="center" valign="middle" >0.4855</td><td align="center" valign="middle" >67.85</td><td align="center" valign="middle" >1.35</td><td align="center" valign="middle" >68.37</td><td align="center" valign="middle" >1.63</td></tr><tr><td align="center" valign="middle" >0.5017</td><td align="center" valign="middle" >42.279</td><td align="center" valign="middle" >1902</td><td align="center" valign="middle" >1855</td><td align="center" valign="middle" >−0.0344</td><td align="center" valign="middle" >0.5361</td><td align="center" valign="middle" >69.38</td><td align="center" valign="middle" >−0.18</td><td align="center" valign="middle" >70.24</td><td align="center" valign="middle" >−0.24</td></tr><tr><td align="center" valign="middle" >0.5427</td><td align="center" valign="middle" >42.440</td><td align="center" valign="middle" >1994</td><td align="center" valign="middle" >1941</td><td align="center" valign="middle" >−0.0366</td><td align="center" valign="middle" >0.5793</td><td align="center" valign="middle" >70.60</td><td align="center" valign="middle" >−1.40</td><td align="center" valign="middle" >71.73</td><td align="center" valign="middle" >−1.73</td></tr><tr><td align="center" valign="middle" >0.5895</td><td align="center" valign="middle" >42.712</td><td align="center" valign="middle" >2194</td><td align="center" valign="middle" >2126</td><td align="center" valign="middle" >−0.0413</td><td align="center" valign="middle" >0.6308</td><td align="center" valign="middle" >68.97</td><td align="center" valign="middle" >0.23</td><td align="center" valign="middle" >69.98</td><td align="center" valign="middle" >0.02</td></tr><tr><td align="center" valign="middle" >0.6302</td><td align="center" valign="middle" >42.860</td><td align="center" valign="middle" >2289</td><td align="center" valign="middle" >2214</td><td align="center" valign="middle" >−0.0436</td><td align="center" valign="middle" >0.6737</td><td align="center" valign="middle" >69.74</td><td align="center" valign="middle" >−0.54</td><td align="center" valign="middle" >70.94</td><td align="center" valign="middle" >−0.94</td></tr><tr><td align="center" valign="middle" >0.7080</td><td align="center" valign="middle" >43.180</td><td align="center" valign="middle" >2533</td><td align="center" valign="middle" >2437</td><td align="center" valign="middle" >−0.0493</td><td align="center" valign="middle" >0.7573</td><td align="center" valign="middle" >69.36</td><td align="center" valign="middle" >−0.16</td><td align="center" valign="middle" >70.62</td><td align="center" valign="middle" >−0.62</td></tr><tr><td align="center" valign="middle" >0.8011</td><td align="center" valign="middle" >43.624</td><td align="center" valign="middle" >2946</td><td align="center" valign="middle" >2810</td><td align="center" valign="middle" >−0.0591</td><td align="center" valign="middle" >0.8602</td><td align="center" valign="middle" >66.21</td><td align="center" valign="middle" >2.99</td><td align="center" valign="middle" >67.06</td><td align="center" valign="middle" >2.94</td></tr><tr><td align="center" valign="middle" >0.8799</td><td align="center" valign="middle" >43.722</td><td align="center" valign="middle" >2953</td><td align="center" valign="middle" >2817</td><td align="center" valign="middle" >−0.0593</td><td align="center" valign="middle" >0.9391</td><td align="center" valign="middle" >70.49</td><td align="center" valign="middle" >−1.29</td><td align="center" valign="middle" >72.01</td><td align="center" valign="middle" >−2.01</td></tr><tr><td align="center" valign="middle" >1.0060</td><td align="center" valign="middle" >44.130</td><td align="center" valign="middle" >3340</td><td align="center" valign="middle" >3160</td><td align="center" valign="middle" >−0.0684</td><td align="center" valign="middle" >1.0745</td><td align="center" valign="middle" >69.22</td><td align="center" valign="middle" >−0.02</td><td align="center" valign="middle" >70.49</td><td align="center" valign="middle" >−0.49</td></tr><tr><td align="center" valign="middle" >1.2559</td><td align="center" valign="middle" >44.763</td><td align="center" valign="middle" >3974</td><td align="center" valign="middle" >3712</td><td align="center" valign="middle" >−0.0835</td><td align="center" valign="middle" >1.3394</td><td align="center" valign="middle" >68.64</td><td align="center" valign="middle" >0.56</td><td align="center" valign="middle" >69.45</td><td align="center" valign="middle" >0.55</td></tr></tbody></table></table-wrap><p>(1) weighted bin average redshift; (2) weighted bin average distance modulus; (3) initial proper distance-Equations (3) &amp; (4); (4) photon travel distance Equation (6); (5) cosmic blueshift If d<sub>o</sub> &lt; 450 then z<sub>c</sub> = 0 else z<sub>c</sub> = (−7.6/c) &#180; (d<sub>o</sub> − 450); (6) tired light redshift z<sub>tl</sub> = z − z<sub>c</sub>; (7) H = (c/d) &#180; ln(1 + z<sub>tl</sub>); (8) resid = 69.2 − H; (9) Equation (8) Ω<sub>M</sub> = 0.278; (10) resid = 70.0 − H<sub>o</sub>.</p><p>weighted dm residual = 0.266. These residuals are identical to the residuals from the TLCU model. There is also a close correlation between the un-weightd dm residuals for the ΛCDM model and those for the TLCU model as seen in <xref ref-type="fig" rid="fig3">Figure 3</xref>. Thus the fit of the TLCU model to the Union2.1 data is nearly identical to the fit of the ΛCDM model to the same data.</p><fig id="fig2"  position="float"><label><xref ref-type="fig" rid="fig2">Figure 2</xref></label><caption><title> <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x53.png" xlink:type="simple"/></inline-formula>from the binned Union2.1 data (see text) for the TLCU model with <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x53.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x54.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x53.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x54.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x55.png" xlink:type="simple"/></inline-formula></title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-7503044x52.png"/></fig><fig id="fig3"  position="float"><label><xref ref-type="fig" rid="fig3">Figure 3</xref></label><caption><title> dm residuals for ΛCDM and TLCU models using Union2.1 supernovae data</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-7503044x56.png"/></fig><p>Fitting the ΛCDM model to the binned data (n = 29) gives <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x57.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x57.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x58.png" xlink:type="simple"/></inline-formula>with a rms residual dm of 0.031 mag. The uncertainties in the Hubble constant and for the calculated dm are slightly greater than those for the TLCU model. The dm residuals for the binned data for both models are shown in <xref ref-type="fig" rid="fig4">Figure 4</xref>.</p><p>The hint of periodicity shown in <xref ref-type="fig" rid="fig2">Figure 2</xref> is repeated in <xref ref-type="fig" rid="fig4">Figure 4</xref> and not only for the TLCU model but also for the ΛCDM model.</p><p>Another method of comparing the models is to fix the minor constants and then to calculate the value of the Hubble constant for each bin of the binned data. This calculation (with <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x59.png" xlink:type="simple"/></inline-formula> for the TLCU model and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x59.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x60.png" xlink:type="simple"/></inline-formula> for the ΛCDM model) gives <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x59.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x60.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x61.png" xlink:type="simple"/></inline-formula> for the TLCU model and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x59.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x60.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x61.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x62.png" xlink:type="simple"/></inline-formula> for the ΛCDM model. The results of these calculations are presented in <xref ref-type="table" rid="table1">Table 1</xref>. The values of the uncertainty in the Hubble constant show that the TLCU model is a better fit to the binned data than is the ΛCDM model.</p></sec><sec id="s4"><title>4. Discussion</title><p>Although the TLCU model only shows a contracting universe it is reasonable to assume that there was a prior expansion which would be consistent with the “periodic world” predicted by Friedman [<xref ref-type="bibr" rid="scirp.74074-ref1">1</xref>] . In this case the linear contraction revealed by the model can be expected to reverse at higher redshifts and eventually show the expanding phase. The periodicity hinted at in <xref ref-type="fig" rid="fig2">Figure 2</xref> and <xref ref-type="fig" rid="fig4">Figure 4</xref> may possibly be harmonics of the fundamental period. More accurate observations at higher redshifts are needed to reveal the truth.</p><p>The reality of the contracting universe depends, of course, on the reality of the tired light effect and although the TLCU model is an excellent fit to the observed data such a fit is no guarantee of the reality of the assumptions on which the model is based. It is also claimed [<xref ref-type="bibr" rid="scirp.74074-ref11">11</xref>] that time dilation falsifies the tired light theory although the assumption that the thirteen high redshift supernovae used are not subject to a Malmquist type bias may not possibly be the case. Never- theless independent evidence for the tired light effect is essential. A possible</p><fig id="fig4"  position="float"><label><xref ref-type="fig" rid="fig4">Figure 4</xref></label><caption><title> dm residuals for ΛCDM and TLCU models using binned data (see text)</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-7503044x63.png"/></fig><p>mechanism for the tired light process and a terrestrial experiment to test this mechanism are discussed in Appendix 2.</p></sec><sec id="s5"><title>5. Conclusion</title><p>It is concluded that further experimental work on a possible photon energy loss process would be justified.</p></sec><sec id="s6"><title>Acknowledgements</title><p>I am grateful to Graham P. Gerrard for help with computing and many stimulating discussions. I used TurboBasic for the calculations which were recoded in Python and the results checked by GPG using SageMathCloud (SMC). I am also grateful to the late Roger H. Beresford for a copy of the Nelder &amp; Mead minimisation routine coded in Basic. I used SMC to create the figures and SageTex to prepare the document.</p></sec><sec id="s7"><title>Cite this paper</title><p>Glover, J. (2017) A Tired Light/Contracting Universe Model from the Union2.1 Supernovae Data. Journal of Modern Physics, 8, 147-155. https://doi.org/10.4236/jmp.2017.82013</p></sec><sec id="s8"><title>Appendix 1: Photon Travel Distance (d)</title><p>The initial distance (<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x64.png" xlink:type="simple"/></inline-formula>) is the distance between emitter and observer at the moment a photon is emitted. In an expanding or contracting universe the path traversed by the photon will have expanded or contracted when it reaches the observer so that <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x64.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x65.png" xlink:type="simple"/></inline-formula> although <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x64.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x65.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x66.png" xlink:type="simple"/></inline-formula> for low values of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x64.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x65.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x66.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x67.png" xlink:type="simple"/></inline-formula>. The relationship between d and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x64.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x65.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x66.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x67.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x68.png" xlink:type="simple"/></inline-formula> derived below is based on three assumptions: 1) the universe is flat [i.e. Euclidean], 2) the space velocity is much les than the speed of light, and 3) the space velocity is linearly proportional to distance</p><disp-formula id="scirp.74074-formula31"><label>(9)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-7503044x69.png"  xlink:type="simple"/></disp-formula><p>where x is distance and k is a constant. Integrating Equation (9) between<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x70.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x70.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x71.png" xlink:type="simple"/></inline-formula>and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x70.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x71.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x72.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x70.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x71.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x72.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x73.png" xlink:type="simple"/></inline-formula>(where the photon travel time,<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x70.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x71.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x72.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x73.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x74.png" xlink:type="simple"/></inline-formula>)</p><disp-formula id="scirp.74074-formula32"><label>(10)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-7503044x75.png"  xlink:type="simple"/></disp-formula><p>gives</p><disp-formula id="scirp.74074-formula33"><label>(11)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-7503044x76.png"  xlink:type="simple"/></disp-formula><p>Equation (11) is re-arranged as Equation (6) for use in Section 2.2.</p></sec><sec id="s9"><title>Appendix 2: Tired Light Experiment</title><p>Mechanisms for the tired-light effect which involve photon/photon interactions or photon/baryon interactions would involve deflection and blurring of images which is not observed. However a possible mechanism which avoids the blurring problem is spontaneous photon decay [<xref ref-type="bibr" rid="scirp.74074-ref8">8</xref>] in which it is assumed that a primary photon decays producing secondary photons [<xref ref-type="bibr" rid="scirp.74074-ref12">12</xref>] all continuing to travel in the same direction. It is necessary that the frequency of these secondary photons would be considerably less than the frequency of the primary photon in order to avoid significant linebroadening .</p><p>Spontaneous decay of the primary radiation from the sun would produce secondary photons amounting to about <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-7503044x77.png" xlink:type="simple"/></inline-formula> at the earth. These tired light photons from the sun would need to be in the GHz/MHz range or lower in order to avoid the line broadening effect and so would make a significant contribution to the observed quiet sun radio emission. Thus it may be that tired light secondary photons have already been observed and this raises the possibility of detecting the tired-light effect experimentally.</p><p>It is suggested here that the tired light radio emission which would be produced from a pulsed femtosecond optical laser could be detected in a terrestrial experiment. It would be necessary to conduct the laser beam through an evacuated tube in order to prevent the radio emission which would otherwise result [<xref ref-type="bibr" rid="scirp.74074-ref13">13</xref>] from ionization of the gas through which the laser beam travelled.</p></sec></body><back><ref-list><title>References</title><ref id="scirp.74074-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Friedman, A. 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