Big-bang nucleosynthesis with a long-lived charged massive particle including 4He spallation processes

被引:17
|
作者
Jittoh, Toshifumi [1 ]
Kohri, Kazunori [2 ,3 ]
Koike, Masafumi [1 ]
Sato, Joe [1 ]
Sugai, Kenichi [1 ]
Yamanaka, Masato [2 ,4 ]
Yazaki, Koichi [5 ,6 ]
机构
[1] Saitama Univ, Dept Phys, Sakura Ku, Saitama 3388570, Japan
[2] High Energy Accelerator Org, KEK, Inst Particle & Nucl Studies, Ctr Theory, Tsukuba, Ibaraki 3050801, Japan
[3] Tohoku Univ, Dept Phys, Sendai, Miyagi 9808578, Japan
[4] Kyoto Sangyo Univ, Maskawa Inst Sci & Culture, Kyoto 6038555, Japan
[5] RIKEN, Nishina Accelerator Res Ctr, Hashimoto Math Phys Lab, Wako, Saitama 3510198, Japan
[6] Kyoto Univ, Yukawa Inst Theoret Phys, Kyoto 6068502, Japan
关键词
WMAP OBSERVATIONS; LITHIUM; ABUNDANCE; SCATTERING; STARS;
D O I
10.1103/PhysRevD.84.035008
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We propose helium-4 spallation processes induced by long-lived stau in supersymmetric standard models, and investigate an impact of the processes on light elements abundances. We show that, as long as the phase space of helium-4 spallation processes is open, they are more important than stau-catalyzed fusion and hence constrain the stau property.
引用
收藏
页数:11
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