Unifying inflation and dark matter with neutrino masses

被引:77
|
作者
Allahverdi, Rouzbeh [1 ,2 ]
Dutta, Bhaskar [3 ]
Mazumdar, Anupam [4 ,5 ,6 ]
机构
[1] Perimeter Inst Theoret Phys, Waterloo, ON N2L 2Y5, Canada
[2] Univ New Mexico, Dept Phys & Astron, Albuquerque, NM 87131 USA
[3] Texas A&M Univ, Dept Phys, College Stn, TX 77843 USA
[4] NORDITA, DK-2100 Copenhagen, Denmark
[5] Niels Bohr Inst, DK-2100 Copenhagen, Denmark
[6] Univ Lancaster, Dept Phys, Lancaster LA1 4YB, England
关键词
D O I
10.1103/PhysRevLett.99.261301
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We propose a simple model where a gauge-invariant inflaton is responsible for cosmic inflation and generates the seed for structure formation, while its relic thermal abundance explains the missing matter of the Universe in the form of cold dark matter. The inflaton self-coupling also explains the observed neutrino masses. All the virtues can be attained in a minimal extension of the standard model gauge group around the TeV scale. We can also unveil these properties of an inflaton in forthcoming space and ground based experiments.
引用
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页数:4
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