Peculiarities of Thermodynamics in Early Universe - Revision history

Cosmo All at 10:06, 9 October 2012

2012-10-09T10:06:12Z

2012-10-01T22:48:04Z

‎Problem 12

2012-10-01T22:47:51Z

‎Problem 9

2012-10-01T22:47:28Z

2012-09-30T17:19:45Z

2012-09-30T17:17:42Z

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[[Category:Thermodynamics of Universe|(5)]]

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 === Problem 10 ===
 Estimate the baryon-antibaryon asymmetry $A\equiv(n_b-n_{\bar{b}})/n_{\bar{b}}$ in the early Universe.
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 === Problem 12 ===
- At what temperature and time does the contribution of
+At what temperature and time does the contribution of
 monopoles into the Universe energy density become comparable to the
 contribution of photons?

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 === Problem 9 ===
- Show that in the epoch when the energy density of the Universe was determined by ultra-relativistic matter and effective number of internal degrees of freedom did not change, held $\dot{T}/T\propto
+Show that in the epoch when the energy density of the Universe was determined by ultra-relativistic matter and effective number of internal degrees of freedom did not change, held $\dot{T}/T\propto
 -T^2$.
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 === Problem 10 ===
 Estimate the baryon-antibaryon asymmetry $A\equiv(n_b-n_{\bar{b}})/n_{\bar{b}}$ in the early Universe.

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