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		<title>Universe after PLANCK - Revision history</title>
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		<updated>2026-05-13T04:03:02Z</updated>
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		<id>http://universeinproblems.com/index.php?title=Universe_after_PLANCK&amp;diff=2020&amp;oldid=prev</id>
		<title>Cosmo All: Created page with &quot;3 __TOC__  According to the &quot;PLANCK&quot; data the Universe's composition is the following: $4,89 \%$ of usual (baryon) matter (the previous es...&quot;</title>
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				<updated>2014-04-01T03:07:55Z</updated>
		
		<summary type="html">&lt;p&gt;Created page with &amp;quot;&lt;a href=&quot;/index.php/Category:Observational_Cosmology&quot; title=&quot;Category:Observational Cosmology&quot;&gt;3&lt;/a&gt; __TOC__  According to the &amp;quot;PLANCK&amp;quot; data the Universe&amp;#039;s composition is the following: $4,89 \%$ of usual (baryon) matter (the previous es...&amp;quot;&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;[[Category:Observational Cosmology|3]]&lt;br /&gt;
__TOC__&lt;br /&gt;
&lt;br /&gt;
According to the &amp;quot;PLANCK&amp;quot; data the Universe's composition is the following: $4,89 \%$ of usual (baryon) matter (the previous estimate according to WMAP data was $4,6 \%$), $26.9 \%$ of dark matter (instead of previous $22,7 \%$) and $68.25 \%$ (instead of $73\%$) of dark energy. The Hubble constant was also corrected; the new value is $ H_0 = 67.11 km\ s^{-1}\ Mpc^{-1}$ (the previous estimate was $70 km\ s^{-1}\ Mpc^{-1}$).&lt;br /&gt;
&lt;br /&gt;
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&amp;lt;div id=&amp;quot;&amp;quot;&amp;gt;&amp;lt;/div&amp;gt;&lt;br /&gt;
&amp;lt;div style=&amp;quot;border: 1px solid #AAA; padding:5px;&amp;quot;&amp;gt;&lt;br /&gt;
=== Problem 1 ===&lt;br /&gt;
&amp;lt;p style= &amp;quot;color: #999;font-size: 11px&amp;quot;&amp;gt;problem id: &amp;lt;/p&amp;gt;&lt;br /&gt;
Compare estimates of the age of Universe according to the &amp;quot;PLANCK&amp;quot; data and that of WMAP.&lt;br /&gt;
&amp;lt;div class=&amp;quot;NavFrame collapsed&amp;quot;&amp;gt;&lt;br /&gt;
  &amp;lt;div class=&amp;quot;NavHead&amp;quot;&amp;gt;solution&amp;lt;/div&amp;gt;&lt;br /&gt;
  &amp;lt;div style=&amp;quot;width:100%;&amp;quot; class=&amp;quot;NavContent&amp;quot;&amp;gt;&lt;br /&gt;
    &amp;lt;p style=&amp;quot;text-align: left;&amp;quot;&amp;gt;\[a(t)=a_0\left(\frac{\Omega_{m0}}{\Omega_{\Lambda0}}\right)^{1/3} \left[sh\left(\frac32\sqrt{\Omega_{\Lambda0}}H_0t\right)\right]^{2/3};\]&lt;br /&gt;
&lt;br /&gt;
\[t_0=\frac23H_0^{-1}\Omega_{\Lambda0}^{-1/2}arsh\sqrt{\frac{\Omega_{\Lambda0}}{\Omega_{m0}}} =t_{\Lambda}arsh\sqrt{\frac{\Omega_{\Lambda0}}{\Omega_{m0}}} =t_{\Lambda}arcth\sqrt{\Omega_{\Lambda0}}.\]&lt;br /&gt;
&lt;br /&gt;
According to the WMAP data&lt;br /&gt;
&lt;br /&gt;
\[t_{\Lambda}\equiv\frac23H_0^{-1}(\Omega_{\Lambda0})^{-1/2}\simeq10.768\times10^9\ years\]&lt;br /&gt;
and \[t_0=13.7\ Gyr.\]&lt;br /&gt;
&lt;br /&gt;
According to the &amp;quot;PLANCK&amp;quot; data&lt;br /&gt;
&lt;br /&gt;
\[t_{\Lambda}=11.74\ Gyr\]&lt;br /&gt;
and \[t_0=13.8\ Gyr.\]&amp;lt;/p&amp;gt;&lt;br /&gt;
  &amp;lt;/div&amp;gt;&lt;br /&gt;
&amp;lt;/div&amp;gt;&amp;lt;/div&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;div id=&amp;quot;&amp;quot;&amp;gt;&amp;lt;/div&amp;gt;&lt;br /&gt;
&amp;lt;div style=&amp;quot;border: 1px solid #AAA; padding:5px;&amp;quot;&amp;gt;&lt;br /&gt;
=== Problem 2 ===&lt;br /&gt;
&amp;lt;p style= &amp;quot;color: #999;font-size: 11px&amp;quot;&amp;gt;problem id: &amp;lt;/p&amp;gt;&lt;br /&gt;
Estimate the age of Universe corresponding to termination of the radiation dominated epoch.&lt;br /&gt;
&amp;lt;div class=&amp;quot;NavFrame collapsed&amp;quot;&amp;gt;&lt;br /&gt;
  &amp;lt;div class=&amp;quot;NavHead&amp;quot;&amp;gt;solution&amp;lt;/div&amp;gt;&lt;br /&gt;
  &amp;lt;div style=&amp;quot;width:100%;&amp;quot; class=&amp;quot;NavContent&amp;quot;&amp;gt;&lt;br /&gt;
    &amp;lt;p style=&amp;quot;text-align: left;&amp;quot;&amp;gt;\[\rho_m=\frac{a_0^3}{a^3}\rho_{m0}=\rho_r;\]&lt;br /&gt;
\[\frac a{a_0}=\frac{\rho_{r0}}{\rho_{m0}}=\frac{\Omega_{r0}}{\Omega_{m0}}=2.9088\times10^{-4};\]&lt;br /&gt;
\[1+z=\frac{a_0}a\to z^*=3436.9;\]&lt;br /&gt;
\[t(z^*)=\frac1{H_0}\int\limits_0^{a/a_0}\frac{dx}x \frac1{\sqrt{\Omega_{\Lambda0}+\Omega_{curv}x^{-2}+\Omega_{m0}x^{-3}+\Omega_{r0}x^{-4}}};\]&lt;br /&gt;
\[t(z^*=3436.9)=50.152\ years.\]&amp;lt;/p&amp;gt;&lt;br /&gt;
  &amp;lt;/div&amp;gt;&lt;br /&gt;
&amp;lt;/div&amp;gt;&amp;lt;/div&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;div id=&amp;quot;&amp;quot;&amp;gt;&amp;lt;/div&amp;gt;&lt;br /&gt;
&amp;lt;div style=&amp;quot;border: 1px solid #AAA; padding:5px;&amp;quot;&amp;gt;&lt;br /&gt;
=== Problem 3 ===&lt;br /&gt;
&amp;lt;p style= &amp;quot;color: #999;font-size: 11px&amp;quot;&amp;gt;problem id: &amp;lt;/p&amp;gt;&lt;br /&gt;
Estimate the age of Universe corresponding to termination of the matter dominated epoch.&lt;br /&gt;
&amp;lt;div class=&amp;quot;NavFrame collapsed&amp;quot;&amp;gt;&lt;br /&gt;
  &amp;lt;div class=&amp;quot;NavHead&amp;quot;&amp;gt;solution&amp;lt;/div&amp;gt;&lt;br /&gt;
  &amp;lt;div style=&amp;quot;width:100%;&amp;quot; class=&amp;quot;NavContent&amp;quot;&amp;gt;&lt;br /&gt;
    &amp;lt;p style=&amp;quot;text-align: left;&amp;quot;&amp;gt;\[\rho_m=\frac{a_0^3}{a^3}\rho_{m0}=\rho_\Lambda;\]&lt;br /&gt;
\[\frac a{a_0}=\left(\frac{\rho_{m0}}{\rho_{\Lambda}}\right)^{1/3}= \left(\frac{\Omega_{m0}}{\Omega_{\Lambda}}\right)^{1/3}=0.7719\times10^{-4};\]&lt;br /&gt;
\[1+z=\frac{a_0}a\to z^*=0.2956;\]&lt;br /&gt;
\[t(z^*)=\frac1{H_0}\int\limits_0^{a/a_0}\frac{dx}x \frac1{\sqrt{\Omega_{\Lambda0}+\Omega_{curv}x^{-2}+\Omega_{m0}x^{-3}+\Omega_{r0}x^{-4}}};\]&lt;br /&gt;
\[t(z^*=0.2956)=10.309\ Gyr\to 3.508\ Gyr \ ago.\]&amp;lt;/p&amp;gt;&lt;br /&gt;
  &amp;lt;/div&amp;gt;&lt;br /&gt;
&amp;lt;/div&amp;gt;&amp;lt;/div&amp;gt;&lt;/div&gt;</summary>
		<author><name>Cosmo All</name></author>	</entry>

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