COSMOLOGICAL IMPLICATIONS OF DYNAMICAL SUPERSYMMETRY BREAKING
被引:485
作者:
BANKS, T
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h-index: 0
机构:
UNIV CALIF SAN DIEGO,DEPT PHYS,LA JOLLA,CA 92093UNIV CALIF SAN DIEGO,DEPT PHYS,LA JOLLA,CA 92093
BANKS, T
[1
]
KAPLAN, DB
论文数: 0引用数: 0
h-index: 0
机构:
UNIV CALIF SAN DIEGO,DEPT PHYS,LA JOLLA,CA 92093UNIV CALIF SAN DIEGO,DEPT PHYS,LA JOLLA,CA 92093
KAPLAN, DB
[1
]
NELSON, AE
论文数: 0引用数: 0
h-index: 0
机构:
UNIV CALIF SAN DIEGO,DEPT PHYS,LA JOLLA,CA 92093UNIV CALIF SAN DIEGO,DEPT PHYS,LA JOLLA,CA 92093
NELSON, AE
[1
]
机构:
[1] UNIV CALIF SAN DIEGO,DEPT PHYS,LA JOLLA,CA 92093
来源:
PHYSICAL REVIEW D
|
1994年
/
49卷
/
02期
关键词:
D O I:
10.1103/PhysRevD.49.779
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
We provide a taxonomy of dynamical supersymmetry-breaking theories, and discuss the cosmological implications of the various types of models. Models in which supersymmetry breaking is produced by chiral superfields which only have interactions of gravitational strength (e.g., string theory moduli) are inconsistent with standard big bang nucleosynthesis unless the gravitino mass is greater than similar to 3X10(4) GeV. This problem cannot be solved by inflation. Models in which supersymmetry is dynamically broken by renormalizable interactions in flat space have no such cosmological problems. Supersymmetry can be broken either in a hidden or the visible sector. However, hidden sector models suffer from several naturalness problems and have difficulties in producing an acceptably large gluino mass.