Cosmological constraints on an invisibly decaying Higgs

被引:111
作者
Bento, MC
Bertolami, O
Rosenfeld, R
机构
[1] Inst Super Tecn, Dept Fis, P-1049001 Lisbon, Portugal
[2] Univ Estadual Paulista, Inst Fis Teor, BR-01405900 Sao Paulo, Brazil
基金
巴西圣保罗研究基金会;
关键词
D O I
10.1016/S0370-2693(01)01078-4
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Working in the context of a proposal for collisional dark matter, we derive bounds on the Higgs boson coupling g' to a stable light scalar particle, which we refer to as phion (phi), required to solve problems with small scale structure formation which arise in collisionless, dark matter models. We discuss the behaviour of the phion in the early universe for different ranges of its mass. We find that a phion in the mass range of 100 MeV is excluded and that a phion in the mass range of I GeV requires a large coupling constant, g' greater than or similar to 2, and m(h) less than or similar to 130 GeV in order to avoid overabundance, in which case the invisible decay mode of the Higgs boson would be dominant. (C) 2001 Elsevier Science B.V. All rights reserved.
引用
收藏
页码:276 / 281
页数:6
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