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- Newsgroups: sci.astro
- Path: sparky!uunet!convex!darwin.sura.net!uvaarpa!concert!samba!usenet
- From: Bruce.Scott@bbs.oit.unc.edu (Bruce Scott)
- Subject: Re: Recombination Temperature Question
- Message-ID: <1992Aug12.162012.8106@samba.oit.unc.edu>
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- Organization: Extended Bulletin Board Service
- References: <1992Aug12.064528.22220@cco.caltech.edu> <1992Aug12.085348.14412@vax5.cit.cornell.edu>
- Distribution: sci
- Date: Wed, 12 Aug 1992 16:20:12 GMT
- Lines: 33
-
- Niel Brandt (niel@jomby.caltech.edu) writes:
-
- >I would like to see or get a reference as to how the T=3000 K at
- >recombination is worked out... I assume this is a fairly complicated
- >plasma physics computation...(which might depend on the geometry of
- >spacetime - although I guess by z=1500 everything was pretty flat)...
- >Also, does the presence of helium have a significant effect - how about
- >nonbaryonic dark matter?
-
- Other constituents do have effects, but since these are all formed
- from the nucleosynthesis in calculable ways, one need only start with
- nucleons, leptons, and photons. The free parameter is the photon to
- baryon ratio. As Joe Lazio pointed out, during the recombination era
- the physics are described by Saha equations (that's right, zero-d).
- All particle units are assumed free ("unit" means free electrons,
- protons, etc, as well as re-combined atoms -- no molecules yet). I
- don't recall how flat space was at z=1500; I suggest reading W
- Rindler, Essential Relativity (1977), for the construction of the
- Robertson-Walker metric, and R Wagoner and D Goldsmith, Cosmic
- Horizons (1983), for the backward extrapolation through which one does
- these calculations. For dark matter, everything is speculative until
- its properties are known.
-
- Gruss,
- Dr Bruce Scott The deadliest bullshit is
- Max-Planck-Institut fuer Plasmaphysik odorless and transparent
- bds at spl6n1.aug.ipp-garching.mpg.de -- W Gibson
-
- --
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