Natural candidates for superheavy dark matter in string and M theory

被引:121
作者
Benakli, K [1 ]
Ellis, J
Nanopoulos, DV
机构
[1] Texas A&M Univ, Ctr Theoret Phys, Dept Phys, College Stn, TX 77843 USA
[2] CERN, Div Theory, CH-1211 Geneva 23, Switzerland
[3] Houston Adv Res Ctr, Astroparticle Phys Grp, The Woodlands, TX 77381 USA
[4] Acad Athens, Chair Theoret Phys, GR-10679 Athens, Greece
来源
PHYSICAL REVIEW D | 1999年 / 59卷 / 04期
关键词
D O I
10.1103/PhysRevD.59.047301
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We reconsider superheavy dark matter candidates in string and M theory, in view of the possibility that inflation might generate superheavy particles with an abundance close to that required for a near-critical Universe. We argue that cryptons-stable or metastable bound states of matter in the hidden sector-are favored over other possible candidates in string or M theory, such as the Kaluza-Klein states associated with extra dimensions. We exhibit a specific string model that predicts cryptons as hidden-sector bound states weighing similar to 10(12) GeV, and discuss their astrophysical observability. [S0556-2821(98)04824-3].
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页数:4
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