PROTON DECAY AND NEUTRINO MASSES IN SO(10)

被引:23
作者
ACAMPORA, F
AMELINO-CAMELIA, G
BUCCELLA, F
PISANTI, O
ROSA, L
TUZI, T
机构
[1] DIPARTIMENTO SCI FIS, I-80125 NAPLES, ITALY
[2] INFN, I-80125 NAPLES, ITALY
[3] MIT, DEPT PHYS, CAMBRIDGE, MA 02139 USA
[4] MIT, CTR THEORET PHYS, NUCL SCI LAB, CAMBRIDGE, MA 02139 USA
来源
NUOVO CIMENTO DELLA SOCIETA ITALIANA DI FISICA A-NUCLEI PARTICLES AND FIELDS | 1995年 / 108卷 / 03期
关键词
D O I
10.1007/BF02787063
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
In the last few years physicists have been looking at SO(10) GUT models with renewed attention because it has been realized that the SU(5) minimal model cannot unify the strong, electromagnetic and weak interactions in a way consistent with the experimental values of alpha(M(Z)), sin2theta(w)(M(Z)) and alpha(S)(M(Z)). In this paper we derive lower limits on neutrino masses, relevant for cosmology and for the solar-neutrino problem, from necessary consistency conditions on a class of SO(10) models with SU(4)ps x SU(2)L x SU(2)R or SU(3)c x SU(2)L x SU(2)R x U(1)B-L intermediate gauge symmetry.
引用
收藏
页码:375 / 400
页数:26
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