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11 December 2024
 
  » arxiv » astro-ph/0701580

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Revised Primordial Helium Abundance Based on New Atomic Data
M. Peimbert ; V. Luridiana ; A. Peimbert ;
Date 19 Jan 2007
AbstractWe have derived a primordial helium abundance of Yp = 0.2474 +- 0.0028, based on new atomic physics computations of the recombination coefficients of He I and of the collisional excitation of the H I Balmer lines together with observations and photoionization models of metal-poor extragalactic H II regions. The new atomic data increase our previous determination of Yp by 0.0083, a very significant amount. By combining our Yp result with the predictions made by the standard Big Bang nucleosynthesis model, we find a baryon-to-photon ratio, eta, in excellent agreement both with the eta value derived by the primordial deuterium abundance value observed in damped Lyman-alpha systems and with the one obtained from the WMAP observations.
Source arXiv, astro-ph/0701580
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