Inhomogeneous big bang nucleosynthesis revisited

被引:29
|
作者
Lara, JF [1 ]
Kajino, T
Mathews, GJ
机构
[1] Clemson Univ, Dept Phys & Astron, Clemson, SC 29631 USA
[2] Natl Astron Observ Japan, Tokyo 1818588, Japan
[3] Grad Univ Adv Studies, Tokyo 1818588, Japan
[4] Univ Tokyo, Grad Sch Sci, Dept Astron, Bunkyo Ku, Tokyo 1130033, Japan
[5] Univ Notre Dame, Ctr Astrophys, Notre Dame, IN 46556 USA
来源
PHYSICAL REVIEW D | 2006年 / 73卷 / 08期
基金
美国国家科学基金会;
关键词
D O I
10.1103/PhysRevD.73.083501
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We reanalyze the allowed parameters for inhomogeneous big bang nucleosynthesis in light of the WMAP constraints on the baryon-to-photon ratio eta and a recent measurement which has set the neutron lifetime to be 878.5 +/- 0.7 +/- 0.3 sec. For a set baryon-to-photon ratio eta the new lifetime reduces the mass fraction of He-4 by 0.0015 but does not significantly change the abundances of other isotopes. This enlarges the region of concordance between He-4 and deuterium in the parameter space of eta and the IBBN distance scale r(i). The Li-7 abundance can be brought into concordance with observed He-4 and deuterium abundances by using depletion factors as high as 9.3. The WMAP constraints, however, severely limit the allowed comoving (T=100 GK) inhomogeneity distance scale to r(i)approximate to(1.3-2.6)x10(5) cm.
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页数:6
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