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Re: [Phys-l] Baryon Acoustic Oscillations




On 2012, Mar 31, , at 00:00, Mark Sylvester wrote:

Looking at http://arxiv.org/abs/1203.6594v1

Have I got this right: there are discernible patterns in the
distribution of galaxies that derive from sound waves in the early
universe, when matter was still dense enough for this. The distance to
these features is accurately known (how is this calibration achieved?)
and thus provides a datum for getting distances to galaxies that lie on
the features.

Mark.


am I understanding this? The early acoustic wave is maintained by mutual gravitational attraction and mass - analogy: intermolecular forces and molecular masses? (solids), etc.

bc thinks rather interesting