Cosmological Constraints on the Scale of Supersymmetry Breaking

Cosmological Constraints on the Scale of Supersymmetry Breaking
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DOI:
10.1103/physrevlett.48.1303
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发表时间:
1982-05
影响因子:
8.6
通讯作者:
S. Weinberg
S. Weinberg
中科院分区:
物理与天体物理1区
文献类型:
--
作者:
S. Weinberg

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引力伴子必须足够轻,这样周围的引力伴子就不会产生太大的宇宙减速,或者足够重,这样几乎所有的引力伴子都会在氦合成之前衰变。第二种选择是允许超对称性破缺尺度高于模型相关的下限10/sup 11/至10/sup 16/ GeV。
The gravitino must be either light enough so that ambient gravitinos would not produce too large a cosmic deceleration, or heavy enough so that almost all gravitinos would have decayed before the time of helium synthesis. The second alternative is shown to allow supersymmetry breaking scales above a model-dependent lower bound of 10/sup 11/ to 10/sup 16/ GeV.