Destruction of 7Be in big bang nucleosynthesis via long-lived sub-strongly interacting massive particles as a solution to the Li problem

被引:22
作者
Kawasaki, Masahiro [1 ,2 ]
Kusakabe, Motohiko [1 ]
机构
[1] Univ Tokyo, Inst Cosm Ray Res, Chiba 2778582, Japan
[2] Univ Tokyo, Inst Phys & Math Universe, Chiba 2778582, Japan
来源
PHYSICAL REVIEW D | 2011年 / 83卷 / 05期
关键词
LATE-DECAYING PARTICLES; MEDIATED SUSY BREAKING; LIGHT-ELEMENTS; PRIMORDIAL NUCLEOSYNTHESIS; LITHIUM ABUNDANCES; WMAP OBSERVATIONS; RADIATIVE DECAY; CROSS-SECTIONS; COSMIC-RAYS; EVOLUTION;
D O I
10.1103/PhysRevD.83.055011
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We identify reactions which destroy Be-7 and Li-7 during big bang nucleosynthesis (BBN) in the scenario of BBN catalyzed by a long-lived sub-strongly-interacting massive particle (sub-SIMP or X particle). The destruction associated with nonradiative X captures of the nuclei can be realized only if the interaction strength between an X particle and a nucleon is properly weaker than that between two nucleons to a degree depending on the mass of X. Binding energies of nuclei to an X particle are estimated taking the mass and the interaction strength to nuclei of the X as input parameters. Nuclear reaction rates associated with the X are estimated naively and adopted in calculating evolutions of nuclear abundances. We suggest that the Li-7 problem, which might be associated with as-yet-unrecognized particle processes operating during BBN, can be solved if the X particle interacts with nuclei strongly enough to drive Be-7 destruction but not strongly enough to form a bound state with He-4 of relative angular momentum L = 1. Justifications of this scenario by rigorous calculations of reaction rates using quantum mechanical many-body models are highly desirable since this result involves many significant uncertainties.
引用
收藏
页数:16
相关论文
共 126 条
[1]   H-3 AND HE-3 ELECTROMAGNETIC FORM-FACTORS [J].
AMROUN, A ;
BRETON, V ;
CAVEDON, JM ;
FROIS, B ;
GOUTTE, D ;
JUSTER, FP ;
LECONTE, P ;
MARTINO, J ;
MIZUNO, Y ;
PHAN, XH ;
PLATCHKOV, SK ;
SICK, I ;
WILLIAMSON, S .
NUCLEAR PHYSICS A, 1994, 579 (3-4) :596-626
[2]   A compilation of charged-particle induced thermonuclear reaction rates [J].
Angulo, C ;
Arnould, M ;
Rayet, M ;
Descouvemont, P ;
Baye, D ;
Leclercq-Willain, C ;
Coc, A ;
Barhoumi, S ;
Aguer, P ;
Rolfs, C ;
Kunz, R ;
Hammer, JW ;
Mayer, A ;
Paradellis, T ;
Kossionides, S ;
Chronidou, C ;
Spyrou, K ;
Degl'Innocenti, S ;
Fiorentini, G ;
Ricci, B ;
Zavatarelli, S ;
Providencia, C ;
Wolters, H ;
Soares, J ;
Grama, C ;
Rahighi, J ;
Shotter, A ;
Rachti, ML .
NUCLEAR PHYSICS A, 1999, 656 (01) :3-183
[3]  
[Anonymous], ARXIV07120647
[4]  
[Anonymous], ARXIV09064373
[5]  
[Anonymous], 2005, J HIGH ENERGY PHYS
[6]   LITHIUM ABUNDANCES OF EXTREMELY METAL-POOR TURNOFF STARS [J].
Aoki, Wako ;
Barklem, Paul S. ;
Beers, Timothy C. ;
Christlieb, Norbert ;
Inoue, Susumu ;
Perez, E. Garcia ;
Norris, John E. ;
Carollo, Daniela .
ASTROPHYSICAL JOURNAL, 2009, 698 (02) :1803-1812
[7]   Aspects of split supersymmetry [J].
Arkani-Hamed, N ;
Dimopoulos, S ;
Giudice, GF ;
Romanino, A .
NUCLEAR PHYSICS B, 2005, 709 (1-2) :3-46
[8]   Lithium isotopic abundances in metal-poor halo stars [J].
Asplund, Martin ;
Lambert, David L. ;
Nissen, Poul Erik ;
Primas, Francesca ;
Smith, Verne V. .
ASTROPHYSICAL JOURNAL, 2006, 644 (01) :229-259
[9]   CONTINUUM-DISCRETIZED COUPLED-CHANNELS CALCULATIONS FOR 3-BODY MODELS OF DEUTERON-NUCLEUS REACTIONS [J].
AUSTERN, N ;
ISERI, Y ;
KAMIMURA, M ;
KAWAI, M ;
RAWITSCHER, G ;
YAHIRO, M .
PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS, 1987, 154 (03) :125-204
[10]   A new approach to systematic uncertainties and self-consistency in helium abundance determinations [J].
Aver, Erik ;
Olive, Keith A. ;
Skillman, Evan D. .
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, 2010, (05)