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.
引用
收藏
页数:6
相关论文
共 50 条
  • [41] Big-bang nucleosynthesis
    K. A. Olive
    [J]. The European Physical Journal C - Particles and Fields, 2000, 15 (1-4): : 133 - 135
  • [42] No crisis for big bang nucleosynthesis
    Kernan, PJ
    Sarkar, S
    [J]. PHYSICAL REVIEW D, 1996, 54 (06) : R3681 - R3685
  • [43] BIG-BANG NUCLEOSYNTHESIS
    K.A.Olive
    K.Agashe
    C.Amsler
    M.Antonelli
    J.-F.Arguin
    D.M.Asner
    H.Baer
    H.R.Band
    R.M.Barnett
    T.Basaglia
    C.W.Bauer
    J.J.Beatty
    V.I.Belousov
    J.Beringer
    G.Bernardi
    S.Bethke
    H.Bichsel
    O.Biebe
    E.Blucher
    S.Blusk
    G.Brooijmans
    O.Buchmueller
    V.Burkert
    M.A.Bychkov
    R.N.Cahn
    M.Carena
    A.Ceccucci
    A.Cerr
    D.Chakraborty
    M.-C.Chen
    R.S.Chivukula
    K.Copic
    G.Cowan
    O.Dahl
    G.D’Ambrosio
    T.Damour
    D.de Florian
    A.de Gouvea
    T.DeGrand
    P.de Jong
    G.Dissertor
    B.A.Dobrescu
    M.Doser
    M.Drees
    H.K.Dreiner
    D.A.Edwards
    S.Eidelman
    J.Erler
    V.V.Ezhela
    W.Fetscher
    [J]. Chinese Physics C, 2014, 38 (09) : 339 - 344
  • [44] Neutrinos and Big Bang Nucleosynthesis
    Steigman, Gary
    [J]. ADVANCES IN HIGH ENERGY PHYSICS, 2012, 2012
  • [45] Neutrinos and big bang nucleosynthesis
    Dolgov, AD
    [J]. NUOVO CIMENTO DELLA SOCIETA ITALIANA DI FISICA B-BASIC TOPICS IN PHYSICS, 2002, 117 (9-11): : 1081 - 1088
  • [46] Inhomogeneous big bang nucleosynthesis and the high baryon density suggested by Boomerang and MAXIMA
    Kurki-Suonio, H
    Sihvola, E
    [J]. PHYSICAL REVIEW D, 2001, 63 (08)
  • [47] Multiple main sequence of globular clusters as a result of inhomogeneous big bang nucleosynthesis
    Moriya, Takashi
    Shigeyama, Toshikazu
    [J]. PHYSICAL REVIEW D, 2010, 81 (04):
  • [48] Inhomogeneous big bang nucleosynthesis and mutual ion diffusion -: art. no. 043512
    Keihänen, E
    [J]. PHYSICAL REVIEW D, 2002, 66 (04)
  • [49] NEUTRON-CAPTURE RATES OF LIGHT ISOTOPES FOR INHOMOGENEOUS BIG-BANG NUCLEOSYNTHESIS
    BEER, H
    [J]. ACTA PHYSICA POLONICA B, 1994, 25 (3-4): : 629 - 636
  • [50] Finite temperature effects on cosmological baryon diffusion and inhomogeneous big-bang nucleosynthesis
    Suh, IS
    Mathews, GJ
    [J]. PHYSICAL REVIEW D, 1998, 58 (12)