Physics potential of future supernova neutrino observations

被引：28

作者：

Dighe, Amol ^{[1
]}

机构：

[1] Tata Inst Fundamental Res, Bombay 400005, Maharashtra, India

来源：

XXIII CONFERENCE ON NEUTRINO PHYSICS AND ASTROPHYSICS | 2008年 / 136卷

关键词：

D O I：

10.1088/1742-6596/136/2/022041

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We point out possible features of neutrino spectra from a future galactic core collapse supernova that will enhance our understanding of neutrino mixing as well as supernova astrophysics. We describe the neutrino flavor conversions inside the star, emphasizing the role of "collective effects" that has been appreciated and understood only very recently. These collective effects change the traditional predictions of flavor conversion substantially, and enable the identification of neutrino mixing scenarios through signatures like Earth matter effects.

引用

页数：7

共 77 条

[71] Earth effects on supernova neutrinos and their implications for neutrino parameters [J].

Takahashi, K ;

Sato, K .

PHYSICAL REVIEW D, 2002, 66 (03)

[72] THE NONLINEAR MSW EQUATION [J].

THOMSON, MJ ;

MCKELLAR, BHJ .

PHYSICS LETTERS B, 1991, 259 (1-2) :113-118

[73] Neutrino signatures of supernova forward and reverse shock propagation -: art. no. 015 [J].

Tomàs, R ;

Kachelriess, M ;

Raffelt, G ;

Dighe, A ;

Janka, HT ;

Scheck, L .

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, 2004, (09) :237-258

[74] Supernova pointing with low- and high-energy neutrino detectors -: art. no. 093013 [J].

Tomàs, R ;

Semikoz, D ;

Raffelt, GG ;

Kachelriess, M ;

Dighe, AS .

PHYSICAL REVIEW D, 2003, 68 (09)

[75] Future detection of supernova neutrino burst and explosion mechanism [J].

Totani, T ;

Sato, K ;

Dalhed, HE ;

Wilson, JR .

ASTROPHYSICAL JOURNAL, 1998, 496 (01) :216-225

[76]

Wong YYY, 2003, AIP CONF PROC, V655, P240, DOI 10.1063/1.1543503

[77]

Wurm M, 2007, AIP CONF PROC, V944, P82, DOI 10.1063/1.2818554

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