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David Marsh
Joined: 03 Feb 2011 Posts: 6 Affiliation: University of Oxford
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Posted: January 19 2012 |
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I have looked at initial conditions in both the CAMB notes, and the referenced paper. There is a correction to δγ in CAMB not present in the paper, which goes as omtau. Is this a higher order correction? If so, why is it necessary, and where is it derived?
I also cannot see the definition of πr. I presume it is some multiple of σr (σν in the reference), but it isn't obvious. The same is true of G3. The definitions also seem absent from arXiv:astro-ph/0203507 on a first glance.
Many thanks in advance to all who can offer help. |
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Antony Lewis
Joined: 23 Sep 2004 Posts: 673 Affiliation: University of Sussex
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Posted: January 19 2012 |
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The omtau terms allow for the effect of matter, as opposed assuming pure radiation domination.
You can find maple derivations at
http://camb.info/theory.html
Also somewhat more generally in mathematica at http://camb.info/jrs/
πr is the (scalar or tensor part of the) neutrino anisotropic stress; scalar definitions should be consistent with the appendix of arXiv:astro-ph/0203507 I think. |
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David Marsh
Joined: 03 Feb 2011 Posts: 6 Affiliation: University of Oxford
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Posted: January 20 2012 |
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| Thank you so much! I think the mathematica and maple notebooks will be most helpfull. |
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