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
收藏
页数:7
相关论文
共 77 条
[1]   Determining the supernova direction of its neutrinos [J].
Ando, S ;
Sato, K .
PROGRESS OF THEORETICAL PHYSICS, 2002, 107 (05) :957-966
[2]  
AUTIERO A, 2007, J COSMOL ASTROPART P
[3]   Antineutrino spectroscopy with large water Cerenkov detectors [J].
Beacom, JF ;
Vagins, MR .
PHYSICAL REVIEW LETTERS, 2004, 93 (17) :171101-1
[4]   Can a supernova be located by its neutrinos? [J].
Beacom, JF ;
Vogel, P .
PHYSICAL REVIEW D, 1999, 60 (03)
[5]   REVIVAL OF A STALLED SUPERNOVA SHOCK BY NEUTRINO HEATING [J].
BETHE, HA ;
WILSON, JR .
ASTROPHYSICAL JOURNAL, 1985, 295 (01) :14-23
[6]  
BURAS R, 2005, ASTROPH0512189
[7]   THE FUTURE OF SUPERNOVA NEUTRINO DETECTION [J].
BURROWS, A ;
KLEIN, D ;
GANDHI, R .
PHYSICAL REVIEW D, 1992, 45 (10) :3361-3385
[8]  
CHOUBEY S, 2008, UNPUB
[9]   Turbulent supernova shock waves and the sterile neutrino signature in megaton water detectors [J].
Choubey, Sandhya ;
Harries, N. P. ;
Ross, G. G. .
PHYSICAL REVIEW D, 2007, 76 (07)
[10]   Probing neutrino oscillations from supernovae shock waves via the IceCube detector [J].
Choubey, Sandhya ;
Harries, N. P. ;
Ross, G. G. .
PHYSICAL REVIEW D, 2006, 74 (05)