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ElaKiri Talk!
Big Bang Theory and Sinhala Buddhist explanation about Big Bang Theory
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<blockquote data-quote="tharinda07" data-source="post: 3578325" data-attributes="member: 21844"><p style="text-align: center"><strong><u><span style="font-size: 18px"><span style="color: RoyalBlue">Other lines of evidence</span></span></u></strong></p> <p style="text-align: center"></p> <p style="text-align: center"><span style="font-size: 10px"><span style="color: Purple"></span></span></p> <p style="text-align: center"><span style="font-size: 10px"><span style="color: Purple"></span></span><span style="font-size: 10px"><span style="color: Purple">After some controversy, the age of universe as estimated from the Hubble expansion and the CMB is now in good agreement with (i.e., slightly larger than) the ages of the oldest stars, both as measured by applying the theory of <a href="http://en.wikipedia.org/wiki/Stellar_evolution" target="_blank">stellar evolution</a> to <a href="http://en.wikipedia.org/wiki/Globular_clusters" target="_blank">globular clusters</a> and through <a href="http://en.wikipedia.org/wiki/Radiometric_dating" target="_blank">radiometric dating</a> of individual <a href="http://en.wikipedia.org/wiki/Population_II" target="_blank">Population II</a> stars.</span></span></p> <p style="text-align: center"><span style="font-size: 10px"><span style="color: Purple">The prediction that the CMB temperature was higher in the past has been experimentally supported by observations of temperature-sensitive emission lines in gas clouds at high redshift. This prediction also implies that the amplitude of the <a href="http://en.wikipedia.org/wiki/Sunyaev-Zel%27dovich_effect" target="_blank">Sunyaev-Zel'dovich effect</a> in <a href="http://en.wikipedia.org/wiki/Clusters_of_galaxies" target="_blank">clusters of galaxies</a> does not depend directly on redshift; this seems to be roughly true, but unfortunately the amplitude does depend on cluster properties which do change substantially over cosmic time, so a precise test is impossible.</span></span></p> <p style="text-align: center"></p> <p style="text-align: center"></p> <p style="text-align: center"></p></blockquote><p></p>
[QUOTE="tharinda07, post: 3578325, member: 21844"] [CENTER][B][U][SIZE=5][COLOR=RoyalBlue]Other lines of evidence[/COLOR][/SIZE][/U][/B] [SIZE=2][COLOR=Purple] [/COLOR][/SIZE][SIZE=2][COLOR=Purple]After some controversy, the age of universe as estimated from the Hubble expansion and the CMB is now in good agreement with (i.e., slightly larger than) the ages of the oldest stars, both as measured by applying the theory of [URL="http://en.wikipedia.org/wiki/Stellar_evolution"]stellar evolution[/URL] to [URL="http://en.wikipedia.org/wiki/Globular_clusters"]globular clusters[/URL] and through [URL="http://en.wikipedia.org/wiki/Radiometric_dating"]radiometric dating[/URL] of individual [URL="http://en.wikipedia.org/wiki/Population_II"]Population II[/URL] stars.[/COLOR][/SIZE] [SIZE=2][COLOR=Purple]The prediction that the CMB temperature was higher in the past has been experimentally supported by observations of temperature-sensitive emission lines in gas clouds at high redshift. This prediction also implies that the amplitude of the [URL="http://en.wikipedia.org/wiki/Sunyaev-Zel%27dovich_effect"]Sunyaev-Zel'dovich effect[/URL] in [URL="http://en.wikipedia.org/wiki/Clusters_of_galaxies"]clusters of galaxies[/URL] does not depend directly on redshift; this seems to be roughly true, but unfortunately the amplitude does depend on cluster properties which do change substantially over cosmic time, so a precise test is impossible.[/COLOR][/SIZE] [/CENTER] [/QUOTE]
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