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		<id>http://universeinproblems.com/index.php?action=history&amp;feed=atom&amp;title=Play_with_Numbers_after_Sivaram</id>
		<title>Play with Numbers after Sivaram - Revision history</title>
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		<updated>2026-05-15T10:43:24Z</updated>
		<subtitle>Revision history for this page on the wiki</subtitle>
		<generator>MediaWiki 1.26.2</generator>

	<entry>
		<id>http://universeinproblems.com/index.php?title=Play_with_Numbers_after_Sivaram&amp;diff=2076&amp;oldid=prev</id>
		<title>Cosmo All at 01:30, 23 May 2014</title>
		<link rel="alternate" type="text/html" href="http://universeinproblems.com/index.php?title=Play_with_Numbers_after_Sivaram&amp;diff=2076&amp;oldid=prev"/>
				<updated>2014-05-23T01:30:38Z</updated>
		
		<summary type="html">&lt;p&gt;&lt;/p&gt;
&lt;table class='diff diff-contentalign-left'&gt;
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				&lt;td colspan='2' style=&quot;background-color: white; color:black; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan='2' style=&quot;background-color: white; color:black; text-align: center;&quot;&gt;Revision as of 01:30, 23 May 2014&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l1&quot; &gt;Line 1:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 1:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;[[Category:Cosmo warm-up|&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;10&lt;/del&gt;]]&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;[[Category:Cosmo warm-up|&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;A&lt;/ins&gt;]]&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&amp;lt;div id=&amp;quot;Siv_1&amp;quot;&amp;gt;&amp;lt;/div&amp;gt;&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&amp;lt;div id=&amp;quot;Siv_1&amp;quot;&amp;gt;&amp;lt;/div&amp;gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Cosmo All</name></author>	</entry>

	<entry>
		<id>http://universeinproblems.com/index.php?title=Play_with_Numbers_after_Sivaram&amp;diff=2068&amp;oldid=prev</id>
		<title>Cosmo All: Created page with &quot;10  &lt;div id=&quot;Siv_1&quot;&gt;&lt;/div&gt; &lt;div style=&quot;border: 1px solid #AAA; padding:5px;&quot;&gt; === Problem 1 === &lt;p style= &quot;color: #999;font-size: 11px&quot;&gt;problem id: ...&quot;</title>
		<link rel="alternate" type="text/html" href="http://universeinproblems.com/index.php?title=Play_with_Numbers_after_Sivaram&amp;diff=2068&amp;oldid=prev"/>
				<updated>2014-05-23T01:07:24Z</updated>
		
		<summary type="html">&lt;p&gt;Created page with &amp;quot;&lt;a href=&quot;/index.php/Category:Cosmo_warm-up&quot; title=&quot;Category:Cosmo warm-up&quot;&gt;10&lt;/a&gt;  &amp;lt;div id=&amp;quot;Siv_1&amp;quot;&amp;gt;&amp;lt;/div&amp;gt; &amp;lt;div style=&amp;quot;border: 1px solid #AAA; padding:5px;&amp;quot;&amp;gt; === Problem 1 === &amp;lt;p style= &amp;quot;color: #999;font-size: 11px&amp;quot;&amp;gt;problem id: ...&amp;quot;&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;[[Category:Cosmo warm-up|10]]&lt;br /&gt;
&lt;br /&gt;
&amp;lt;div id=&amp;quot;Siv_1&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: Siv_1&amp;lt;/p&amp;gt;&lt;br /&gt;
(after C.Sivaram, Dark Energy may link the numbers of Rees, arXiv: 0710.4993)&lt;br /&gt;
Given $\Lambda$-dominated Universe, the requirement that for various large scale structures (held together by self gravity) to form a variety of length scales, their gravitational self energy density should at least match the ambient vacuum energy repulsion, as was shown to imply [16. C Sivaram, Astr. Spc. Sci, 219, 135; IJTP, 33, 2407, 1994, 17. C Sivaram, Mod. Phys. Lett., 34, 2463, 1999]&lt;br /&gt;
a scale invariant mass-radius relationship to the form (for the various structures):&lt;br /&gt;
\[\frac M{R^2}\approx\sqrt\Lambda\frac{c^2} G.\]&lt;br /&gt;
This equation  predicts a universality of $M/R^2$ for a large variety of structures. Check this statement for such structures as a galaxy, a globular cluster, a galaxy cluster.&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;For a typical spiral galaxy $M_{gal}\approx10^{12} M_\odot$, $R\approx30kpc$, for globular clusters, $M\approx10^{6} M_\odot$, $R\approx100pc$, for galaxy clusters, $M_C\approx10^{16} M_\odot$, $R_C\approx3Mpc$, so for all these structures the equation holds.&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;
&lt;br /&gt;
&amp;lt;div id=&amp;quot;Siv_2&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: Siv_2&amp;lt;/p&amp;gt;&lt;br /&gt;
(after C.Sivaram, Scaling Relations for self-Similar Structures and the Cosmological Constant, arXiv: 0801.1218)&lt;br /&gt;
In recent papers [13. Sivaram, C.: 1993a, Mod. Phys. Lett. 8,321.; 14. Sivaram, C.: 1993b, Astrophys. Spc. Sci. 207, 317.; 15. Sivaram, C.: 1993c, Astron. Astrophys. 275, 37.; 16. Sivaram, C.: 1994a, Astrophysics. Spc. Sci., 215, 185.; 17. Sivaram, C.: 1994b. Astrphysics .Spc .Sci., 215,191.; 18. Sivaram, C.: 1994c. Int. J. Theor. Phys. 33, 2407.], it was pointed out that the surface gravities of a whole hierarchy&lt;br /&gt;
of astronomical objects (i.e. globular clusters, galaxies, clusters, super clusters,&lt;br /&gt;
GMC's etc.) are more or less given by a universal value $a_0\approx cH_0\approx 10^{-8} cm\ s^{-2}$ a o ƒ° cHo ƒ° 10-8 cms-2. Thus&lt;br /&gt;
\[a=\frac{GM}{R^2}\approx a_0\]&lt;br /&gt;
for all these objects, $M$ being their typical mass and $R$ their typical radius. Also interestingly enough it was also pointed out [4. Sivaram, C.: 1982, Astrophysics. Spc. Sci. 88,507.; 5. Sivaram, C.: 1982, Amer. J. Phy. 50, 279.; 6. Sivaram, C.: 1983, Amer. J. Phys. 51, 277.; 7. Sivaram, C.: 1983, Phys. Lett. 60B, 181.] that the gravitational self energy of a typical elementary particle (hadron) was shown to be&lt;br /&gt;
\[E_G\approx\frac{Gm^3 c}{\hbar}\approx\hbar H_0\]&lt;br /&gt;
implying the same surface gravity value for the particle&lt;br /&gt;
\[a_h=\frac{GM}{r^2}\approx \frac{Gm^3 c}{\hbar}\times\frac c\hbar\approx cH_0\approx a_0.\]&lt;br /&gt;
Calculate actual value of the ratio&lt;br /&gt;
\[\frac M{R^2}\approx\sqrt\Lambda\frac{c^2} G\sim1\]&lt;br /&gt;
for such examples as a galaxy, whole Universe, globular cluster, a GMC, a supercluster, nuclei, an electron, Solar system, planetary nebula.&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;\begin{tabular}{|c|c|}&lt;br /&gt;
   \hline&lt;br /&gt;
   $M/R^2$ ($g/cm^2$) &amp;amp; Object \\&lt;br /&gt;
   \hline&lt;br /&gt;
   $10^{45}/(3\times10^{22})^2\sim1$ &amp;amp; Galaxy \\&lt;br /&gt;
   $10^{56}/(10^{28})^2\sim1$ &amp;amp; Universe \\&lt;br /&gt;
   $10^{38}/(10^{19})^2\sim1$ &amp;amp; globular cluster, GMC, etc. \\&lt;br /&gt;
   $few\times10^{48}/(few\times10^{24})^2\sim1$ &amp;amp; supercluster \\&lt;br /&gt;
   $10^{-23}/(10^{-12})^2\sim1$ &amp;amp; nuclei \\&lt;br /&gt;
   $10^{-27}/(10^{-13})^2\sim1$ &amp;amp; electron \\&lt;br /&gt;
   $10^{33}/(10^{16})^2\sim1$ &amp;amp; Solar system, planetary nebula\\&lt;br /&gt;
   \hline&lt;br /&gt;
 \end{tabular}&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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