Unified TeV scale picture of baryogenesis and dark matter

被引:48
作者
Babu, K. S. [1 ]
Mohapatra, R. N.
Nasri, Salah
机构
[1] Oklahoma State Univ, Dept Phys, Stillwater, OK 74078 USA
[2] Univ Maryland, Dept Phys, College Pk, MD 20742 USA
[3] Univ Florida, Dept Phys, Gainesville, FL 32611 USA
关键词
D O I
10.1103/PhysRevLett.98.161301
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We present a simple extension of the minimal supersymmetric standard model which provides a unified picture of cosmological baryon asymmetry and dark matter. Our model introduces a gauge singlet field N and a color triplet field X which couple to the right-handed quark fields. The out-of-equilibrium decay of the Majorana fermion N mediated by the exchange of the scalar field X generates adequate baryon asymmetry for M-N similar to 100 GeV and M-X similar to TeV. The scalar partner of N (denoted N-1) is naturally the lightest SUSY particle as it has no gauge interactions and plays the role of dark matter. The model is experimentally testable in (i) neutron-antineutron oscillations with a transition time estimated to be around 10(10)sec, (ii) discovery of colored particles X at LHC with mass of order TeV, and (iii) direct dark matter detection with a predicted cross section in the observable range.
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