<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article  PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd"><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article"><front><journal-meta><journal-id journal-id-type="publisher-id">JHEPGC</journal-id><journal-title-group><journal-title>Journal of High Energy Physics, Gravitation and Cosmology</journal-title></journal-title-group><issn pub-type="epub">2380-4327</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/jhepgc.2019.53048</article-id><article-id pub-id-type="publisher-id">JHEPGC-94065</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>
 
 
  The Age of the Universe Predicted by a Time-Varying &lt;i&gt;G&lt;/i&gt; Model?
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Christopher</surname><given-names>Pilot</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>Physics Department, Gonzaga University, Spokane, WA, USA</addr-line></aff><pub-date pub-type="epub"><day>08</day><month>05</month><year>2019</year></pub-date><volume>05</volume><issue>03</issue><fpage>928</fpage><lpage>934</lpage><history><date date-type="received"><day>18,</day>	<month>June</month>	<year>2019</year></date><date date-type="rev-recd"><day>28,</day>	<month>July</month>	<year>2019</year>	</date><date date-type="accepted"><day>31,</day>	<month>July</month>	<year>2019</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>
 
 
  Based on previous work, it is shown how a time varying gravitational constant can account for the apparent tension between Hubble’s constant and a newly predicted age of the universe. The rate of expansion, about nine percent greater than previously estimated, can be accommodated by two specific models, treating the gravitational constant as an order parameter. The deviations from ∧CDM are slight except in the very early universe, and the two time varying parametrizations for 
  G lead to precisely the standard cosmological model in the limit where, 
  <inline-formula><inline-graphic xlink:href="dit_72cdc9c8-1d3f-42a5-ada6-b7322239295f.png" xlink:type="simple"/></inline-formula> , as well as offering a possible explanation for the observed tension. It is estimated that in the current epoch, 
  <inline-formula><inline-graphic xlink:href="dit_619f1edf-be1b-477f-8aab-e9439f4561d4.png" xlink:type="simple"/></inline-formula> , where 
  H<sub>0</sub> is Hubble’s parameter, a value within current observational bounds.
 
</p></abstract><kwd-group><kwd>Universe</kwd><kwd> Gravitational Constant</kwd><kwd> Hubble’s Constant</kwd><kwd> Standard Cosmological Model</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>Conflicts of Interest</title><p>The author declares no conflicts of interest regarding the publication of this paper.</p></sec><sec id="s2"><title>Cite this paper</title><p>Pilot, C. (2019) The Age of the Universe Predicted by a Time-Varying G Model? Journal of High Energy Physics, Gravitation and Cosmology, 5, 928-934. https://doi.org/10.4236/jhepgc.2019.53048</p></sec></body><back><ref-list><title>References</title><ref id="scirp.94065-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Riess, A.G., Casertano, S., Yuan, W., Macri, L.M. and Scolnic, D. (2018) Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond ΛCDM. 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