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- W1715374051 abstract "An analysis of the b → sγ is given in supergravity grand unification using the framework of the radiative breaking of the electro-weak symmetry under three separate sets of constraints: 1) neutralino relic density does not overclose the universe, 2) p-stability constraint, and 3) the combined constraints of p-stability and COBE data. For case 1 it is found that the CLEO II data on the branching ratio already imposes very strong further constraints on dark matter analyses. For case 2 the branching ratio is found to lie in the range (1.5–6.3) × 10−4 and thus the data does not at present significantly limit the analyses with p-stability constraint. It is shown that improvements by a factor of 3 in the p→νK+ lifetime will reduce SUSY effects to less than O(30%) of the Standard Model value. For case 3, the branching ratio lies in the interval (3.1–5.3) × 10−4, and the SUSY effects lie within (−10%, +50%) of the SM value. Thus as experimental bounds on B(b→sγ) improve, one would need in cases 2 and 3 the next-to-leading order QCD corrections to disentangle SUSY effects." @default.
- W1715374051 created "2016-06-24" @default.
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- W1715374051 date "1994-09-01" @default.
- W1715374051 modified "2023-09-27" @default.
- W1715374051 title "b → sγ decay in supergravity grand unification and dark matter" @default.
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- W1715374051 doi "https://doi.org/10.1016/0370-2693(94)90550-9" @default.
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