Difference between revisions of "The Power-Law Cosmology"
(Created page with "10 <div id="PWL_1"></div> <div style="border: 1px solid #AAA; padding:5px;"> === Problem 1 === <p style= "color: #999;font-size: 11px">problem id: PW...") |
|||
Line 1: | Line 1: | ||
− | [[Category:Dark Energy| | + | [[Category:Dark Energy|A]] |
<div id="PWL_1"></div> | <div id="PWL_1"></div> |
Latest revision as of 01:22, 23 May 2014
Problem 1
problem id: PWL_1
Show that for power law $a(t)\propto t^n$ expansion slow-roll inflation occurs when $n\gg1$.
Slow-roll inflation corresponds to \[\varepsilon\equiv-\frac{\dot H}{H}\ll1.\] For power law expansion $H=n/t$ so that $\varepsilon=n^{-1}$. Consequently, slow-roll inflation occurs when $n\gg1$.
Problem 2
problem id: PWL_2
Show that in the power-law cosmology the scale factor evolution $a\propto\eta^q$ in conformal time transforms into $a\propto t^p$ in physical (cosmic) time with \[p=\frac{q}{1+q}.\]
Problem 3
problem id: PWL_3
Show that if $a\propto\eta^q$ then the state parameter $w$ is related to the index $q$ by the following \[w=\frac{2-q}{3q}=const.\]
\[\bar H=\frac q t,\quad \bar H'=-\frac q{t^2}.\] Using \[\bar H'=-\frac{1+3w}{2}\bar H^2,\] one obtains \[w=\frac{2-q}{3q}.\]