COSMOLOGICAL IMPLICATIONS OF AXINOS

被引:221
作者
RAJAGOPAL, K
TURNER, MS
WILCZEK, F
机构
[1] UNIV CHICAGO,ENRICO FERMI INST,DEPT PHYS & ASTRON,CHICAGO,IL 60637
[2] UNIV CHICAGO,ENRICO FERMI INST,DEPT ASTROPHYS,CHICAGO,IL 60637
[3] INST ADV STUDY,SCH NAT SCI,PRINCETON,NJ 08540
基金
加拿大自然科学与工程研究理事会;
关键词
D O I
10.1016/0550-3213(91)90355-2
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
Axinos are the supersymmetric partners of axions. They arise in models incorporating both low-energy supersymmetry and the axion solution of the strong CP problem. In the present state of knowledge several of the key properties of axinos, which control their cosmological consequences, are poorly determined. But generically there are very significant cosmological consequences, and we attempt to survey the possibilities here. In a wide variety of models the axino is the lightest R-odd particle, and destabilizes the more conventional candidates for this title (photino. higgsino,...) on cosmological time scales. While this consideration perhaps casts some shadow over an important class of dark matter candidates, it turns out that in a large class of models the axino itself becomes a plausible dark matter candidate. In other models the axino is heavy, and unstable. Even then axinos are of cosmological interest, because their decay can be the dominant mechanism for production of the lightest R-odd particle.
引用
收藏
页码:447 / 470
页数:24
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