Right-handed neutrino production in dense and hot plasmas

被引:31
|
作者
Ayala, A
D'Olivo, JC
Torres, M
机构
[1] Natl Autonomous Univ Mexico, Inst Ciencias Nucl, Mexico City 04510, DF, Mexico
[2] Univ Nacl Autonoma Mexico, Inst Fis, Mexico City 01000, DF, Mexico
关键词
D O I
10.1016/S0550-3213(99)00642-2
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
For Dirac neutrinos with magnetic moment, we compute the production rate for right-banded neutrinos in a hot and dense QED plasma containing an initial population of left-handed neutrinos thermally distributed. The most important mechanisms for nu(L) depolarization, or production of right-handed neutrinos, are the nu(L) --> nu(R) chirality flip and the plasmon decay to <(nu)over bar>(L) + nu(R). The rates for these processes are computed in terms of a resummed photon propagator which consistently incorporates the background effects to leading order. Applying the results to the cases of supernovae core collapse and the primordial nucleosynthesis in the early universe, we obtain upper Limits on the neutrino magnetic moment. (C) 2000 Elsevier Science B.V. All rights reserved.
引用
收藏
页码:204 / 222
页数:19
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