Fast-time variations of supernova neutrino fluxes and detection perspectives

被引：0

作者：

Tamborra, I. ^{[1
]}

Hanke, F. ^{[2
]}

Mueller, B. ^{[2
]}

Janka, H. -T. ^{[2
]}

Raffelt, G. G. ^{[1
]}

机构：

[1] Werner Heisenberg Inst, Max Planck Inst Phys, D-80805 Munich, Germany

[2] Max Planck Inst Astrophys, D-85748 Garching, Germany

来源：

13TH INTERNATIONAL CONFERENCE ON TOPICS IN ASTROPARTICLE AND UNDERGROUND PHYSICS, TAUP 2013 | 2015年 / 61卷

关键词：

neutrinos; supernova; hydrodynamical instabilities; CORE-COLLAPSE SUPERNOVAE; ACCRETION SHOCK INSTABILITY; SIMULATIONS; HYDRODYNAMICS; MECHANISMS; TRANSPORT; MODELS;

D O I：

10.1016/j.phpro.2014.12.076

中图分类号：

O59 [应用物理学];

学科分类号：

摘要：

In the delayed explosion scenario of a core-collapse supernova, the accretion phase shows pronounced convective overturns and a low-multipole hydrodynamic instability, the so-called standing accretion shock instability (SASI). Neutrino signal variations from the first full-scale three-dimensional core-collapse supernova simulations with sophisticated neutrino transport are presented as well as their detection perspectives in IceCube and Hyper-Kamiokande. (C) 2015 The Authors. Published by Elsevier B.V.

引用

页码：359 / 365

页数：7

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