Dirac neutrino magnetic moment and possible time evolution of the neutrino signal from a supernova

被引：0

作者：

Anikin, R. A. ^{[1
]}

Kuznetsov, A. V. ^{[1
]}

Mikheev, N. V. ^{[1
]}

机构：

[1] Yaroslavl State Univ, Yaroslavl 150000, Russia

来源：

ASTRONOMY LETTERS-A JOURNAL OF ASTRONOMY AND SPACE ASTROPHYSICS | 2010年 / 36卷 / 09期

关键词：

supernovae; neutrino interactions; GAUGE THEORIES; LEPTON-NUMBER; SN1987A; BURST; STAR; SYMMETRY; DYNAMICS; MODELS; 1987A; FLIP;

D O I：

10.1134/S1063773710090069

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We analyze the influence of neutrino helicity conversion, nu (L) -> nu (R), on the neutrino flux from a supernova attributable to the interaction of the Dirac neutrino magnetic moment with a magnetic field.We show that if the neutrino has a magnetic moment in the interval 10(-13)A mu(B) < A mu(nu) < 10(-12)A mu(B) and provided that a magnetic field of similar to 10(13)-10(14) G exists in the supernova envelope, a peculiar kind of time evolution of the neutrino signal from the supernova attributable to the resonance transition nu (L) -> nu (R) in the magnetic field of the envelope can appear.

引用

页码：680 / 685

页数：6

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