On B and L violation in the laboratory in the light of cosmological and astrophysical constraints

被引:45
作者
Campbell, Bruce A. [1 ,3 ]
Davidson, Sacha [1 ]
Ellis, John [1 ]
Olive, Keith A. [2 ]
机构
[1] CERN, Div Theoret Phys, CH-1211 Geneva 23, Switzerland
[2] Univ Minnesota, Sch Phys & Astron, Minneapolis, MN 55455 USA
[3] Univ Alberta, Dept Phys, Fac Sci, Edmonton, AB T6G 2J1, Canada
基金
加拿大自然科学与工程研究理事会;
关键词
D O I
10.1016/0927-6505(92)90010-W
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We have pointed out previously that the survival of a cosmological baryon asymmetry despite strong non-perturbative electroweak interactions puts severe constraints on extensions of the Standard Model that violate baryon number B and/or lepton number L. After reviewing this argument including numerical factors, and implementing astrophysical constraints, in this paper we discuss the prospects for observing B and/or L violation in laboratory experiments. Modulo loopholes that we mention, we find that even if R parity is violated, the lifetime of the lightest supersymmetric particle must be so long that its decays could not be observed in accelerator experiments, and the L-violating Z decays would have unobservably small branching ratios. The only novel signature for accelerator experiments that survives our analysis is a small window for the lightest supersymmetric particle to be strongly-interacting or charged, with a lifetime that is short on a cosmological time-scale but long enough to appear stable in accelerator experiments. We also find that even if Delta B = 2 interactions exist, the rates they yield for n-(n) over bar oscillations and N-N annihilations in nuclei must be unobservably small.
引用
收藏
页码:77 / 97
页数:21
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