CONSTRAINTS FROM PRIMORDIAL NUCLEOSYNTHESIS ON THE MASS OF THE TAU NEUTRINO

被引:72
作者
KOLB, EW
TURNER, MS
CHAKRAVORTY, A
SCHRAMM, DN
机构
[1] UNIV CHICAGO,ENRICO FERMI INST,DEPT ASTRON & ASTROPHYS,CHICAGO,IL 60637
[2] UNIV CHICAGO,DEPT PHYS,CHICAGO,IL 60637
关键词
D O I
10.1103/PhysRevLett.67.533
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
The familiar nucleosynthesis constraint on the number of neutrino species, N(v) less-than-or-equal-to 3.4, applies to massless neutrino species. An MeV-mass neutrino can have even greater impact, and we show that primordial nucleosynthesis excludes a tau-neutrino mass from 0.3 to 25 MeV (Dirac) and 0.5 to 25 MeV (Majorana) provided that its lifetime tau-v greater-than-or-similar-to sec, and from 0.3 to 30 MeV (Dirac) and 0.5 to 32 MeV (Majorana) for tau-v greater-than-or-similar-to 10(3) sec. A modest improvement in the laboratory mass limit - from 35 to 25 MeV - would imply that the tau-neutrino mass must be less than 0.5 MeV (provided tau-v greater-than-or-similar-to 1 sec).
引用
收藏
页码:533 / 536
页数:4
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