Resonant neutrino spin-flavor precession and supernova shock revival

被引：19

作者：

Akhmedov, EK

Lanza, A

Petcov, ST

Sciama, DW

机构：

[1] SCUOLA INT SUPER STUDI AVANZATI, I-34014 TRIESTE, ITALY

[2] IST NAZL FIS NUCL, TRIESTE, ITALY

[3] BULGARIAN ACAD SCI, INST NUCL RES & NUCL ENERGY, BG-1784 SOFIA, BULGARIA

[4] INT CTR THEORET PHYS, I-34100 TRIESTE, ITALY

来源：

PHYSICAL REVIEW D | 1997年 / 55卷 / 02期

关键词：

D O I：

10.1103/PhysRevD.55.515

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

A new mechanism of supernova shock revival is proposed which involves the resonant spin-flavor precession of neutrinos with a transition magnetic moment in the magnetic field of the supernova. The mechanism can be operative id supernovae for transition magnetic moments as small as 10(-14)mu(B) provided the neutrino mass squared difference is in the range Delta m(2) similar to(3 eV)(2)-(600 eV)(2). it is shown that this mechanism can increase the neutrino-induced shock reheating energy by about 60%.

引用

页码：515 / 522

页数：8

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