SUPERSYMMETRY AND LARGE TRANSITION MAGNETIC-MOMENT OF THE NEUTRINO

被引:98
作者
BABU, KS
MOHAPATRA, RN
机构
[1] Department of Physics and Astronomy, University of Maryland, College Park
关键词
D O I
10.1103/PhysRevLett.64.1705
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We show that the most general minimal supersymmetric standard model with le-l symmetry (li=ith lepton number) and a discrete horizontal symmetry between e and families can generate a large transition magnetic moment for the neutrino while leading to a naturally small mass. A magnetic moment of order 0.3×10-10B implies me=m1 eV. The photino, which is expected to be the lightest supersymmetric particle, is unstable in this scheme, decaying dominantly into three-lepton final states (+»e-, e+»-+charge conjugate). © 1990 The American Physical Society.
引用
收藏
页码:1705 / 1708
页数:4
相关论文
共 21 条
[2]  
AULAKH C, 1983, PHYS LETT B, V119, P136
[3]   MODEL FOR LARGE TRANSITION MAGNETIC-MOMENT OF THE ELECTRON NEUTRINO [J].
BABU, KS ;
MOHAPATRA, RN .
PHYSICAL REVIEW LETTERS, 1989, 63 (03) :228-231
[4]  
BACHALL J, 1988, REV MOD PHYS, V60, P297
[5]   LIMIT ON THE MAGNETIC-MOMENT OF THE NEUTRINO FROM SUPERNOVA-1987A OBSERVATIONS [J].
BARBIERI, R ;
MOHAPATRA, RN .
PHYSICAL REVIEW LETTERS, 1988, 61 (01) :27-30
[6]  
CHANG D, PUB8923T FERM REP
[7]   EFFECT OF NEUTRINO MAGNETIC MOMENT ON SOLAR NEUTRINO OBSERVATIONS [J].
CISNEROS, A .
ASTROPHYSICS AND SPACE SCIENCE, 1971, 10 (01) :87-&
[8]  
DAVIS R, IN PRESS 13TH P INT, P518
[9]  
ECKER G, UWTHPH198941 CERNTH5
[10]  
GIUDICE G, 1989, 89167T FERM REP