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25 April 2024
 
  » arxiv » astro-ph/9601027

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Future Cosmic Microwave Background Constraints to the Baryon Density
Marc Kamionkowski ; Gerard Jungman ; Arthur Kosowsky ; David N. Spergel ;
Date 8 Dec 1995
Subject astro-ph
AffiliationColumbia), Gerard Jungman (Syracuse), Arthur Kosowsky (Harvard), and David N. Spergel (Princeton and Maryland
AbstractWe discuss what can be learned about the baryon density from an all-sky map of the cosmic microwave background (CMB) with sub-degree angular resolution. With only minimal assumptions about the primordial spectrum of density perturbations and the values of other cosmological parameters, such a CMB map should be able to distinguish between a Universe with a baryon density near 0.1 and a baryon-dominated Universe. With additional reasonable assumptions, it is conceivable that such measurements will constrain the baryon density to an accuracy similar to that obtained from BBN calculations.
Source arXiv, astro-ph/9601027
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