Evolution of Universe - Revision history

Cosmo All at 00:50, 29 April 2014

2014-04-29T00:50:25Z

2014-03-11T10:07:55Z

2014-03-11T10:07:12Z

2014-03-11T09:54:14Z

‎Problem 9

2014-03-11T09:49:17Z

‎Problem 8

2014-03-11T09:47:45Z

‎Problem 7

2014-03-11T09:47:16Z

‎Problem 5

2014-03-11T09:46:42Z

‎Problem 2

2014-03-11T09:46:16Z

‎Problem 1

2014-03-11T09:45:13Z

‎Problem 1

@@ Line 1,561: / Line 1,561: @@
 \end{equation}
 	</p>
    </div>
 </div></div>

@@ Line 1,531: / Line 1,531: @@
 	\[r=2q^2+q,\, s=\frac23(q+1).\]
 We note that $r=1,\, s=0$ for $q=-1$. Thus the power law cosmology mimics SCM model with $q=-1$.</p>
    </div>
 </div></div>

@@ Line 195: / Line 195: @@
 {j_0} = 1;\\
 {s_0} = 1 - \frac{9}{2}{\Omega _m};\\
-{l_0} = 1 + 3{\Omega _m} + \frac{{27}}{2}\Omega _m^2
+{l_0} = 1 + 3{\Omega _m} + \frac{27}{2}\Omega _m^2
 \end{array}\]
 	</p>
@@ Line 205: / Line 205: @@
 <div id="SCM10"></div>
 <div style="border: 1px solid #AAA; padding:5px;">
 === Problem 10 ===
 Photons with $z=0.1,\ 1,\ 100,\

@@ Line 171: / Line 171: @@
   + \frac{1 - \Omega _m}{4}\left[ 489 + 9(82 - 21\Omega _m)w_a \right]w_0 + \\
   + \frac{9}{2}\left( 1 - \Omega _m \right)\left[ 67 - 21\Omega _m + \frac{3}{2}(23 - 11\Omega _m)w_a \right]w_0^2 + \\
-  + \frac{{27}}{4}\left( {1 - {\Omega _m}} \right)(47 - 24{\Omega _m})w_0^3 + \\
+  + \frac{27}{4}\left( {1 - {\Omega _m}} \right)(47 - 24{\Omega _m})w_0^3 + \\
   + \frac{81}{2}\left( 1 - \Omega _m \right)(3 - 2\Omega _m)w_0^4
 \end{array}\]
@@ Line 182: / Line 182: @@
 <div id="SCM16"></div>
 <div style="border: 1px solid #AAA; padding:5px;">
 === Problem 9 ===
 Show that the results of the previous problem applied to SCM coincide with

@@ Line 129: / Line 129: @@
 elementary functions of the deceleration parameter $q$ or the
 density parameter \[\Omega_m=\frac23(1+q).\]
-<div class="NavFrame collapsed">
+<!--<div class="NavFrame collapsed">
    <div class="NavHead">solution</div>
    <div style="width:100%;" class="NavContent">
      <p style="text-align: left;"></p>
    </div>
-</div></div>
+</div>--></div>
@@ Line 140: / Line 140: @@
 <div id="SCM15"></div>
 <div style="border: 1px solid #AAA; padding:5px;">
 === Problem 8 ===
 Consider the case of flat Universe filled by non-relativistic matter and dark