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Title: Fast time variations of supernova neutrino signals from 3-dimensional models

Abstract

Here, we study supernova neutrino flux variations in the IceCube detector, using 3D models based on a simplified neutrino transport scheme. The hemispherically integrated neutrino emission shows significantly smaller variations compared with our previous study of 2D models, largely because of the reduced activity of the standing accretion shock instability in this set of 3D models which we interpret as a pessimistic extreme. For the studied cases, intrinsic flux variations up to about 100 Hz frequencies could still be detected in a supernova closer than about 2 kpc.

Authors:
 [1];  [2];  [2];  [2];  [3]
  1. North Carolina State Univ., Raleigh, NC (United States)
  2. Max-Planck-Institut fur Astrophysik, Garching (Germany)
  3. Max-Planck-Institut fur Physik (Werner-Heisenberg-Institut), Munchen (Germany)
Publication Date:
Research Org.:
North Carolina State University, Raleigh, NC (United States)
Sponsoring Org.:
USDOE Office of Science (SC), Nuclear Physics (NP)
OSTI Identifier:
1327859
Grant/Contract Number:  
SC0006417
Resource Type:
Accepted Manuscript
Journal Name:
Physical Review. D, Particles, Fields, Gravitation and Cosmology
Additional Journal Information:
Journal Volume: 86; Journal Issue: 10; Journal ID: ISSN 1550-7998
Publisher:
American Physical Society (APS)
Country of Publication:
United States
Language:
English
Subject:
73 NUCLEAR PHYSICS AND RADIATION PHYSICS; 79 ASTRONOMY AND ASTROPHYSICS; neutrino; supernova

Citation Formats

Lund, Tina, Wongwathanarat, Annop, Janka, Hans -Thomas, Muller, Ewald, and Raffelt, Georg. Fast time variations of supernova neutrino signals from 3-dimensional models. United States: N. p., 2012. Web. doi:10.1103/PhysRevD.86.105031.
Lund, Tina, Wongwathanarat, Annop, Janka, Hans -Thomas, Muller, Ewald, & Raffelt, Georg. Fast time variations of supernova neutrino signals from 3-dimensional models. United States. https://doi.org/10.1103/PhysRevD.86.105031
Lund, Tina, Wongwathanarat, Annop, Janka, Hans -Thomas, Muller, Ewald, and Raffelt, Georg. Mon . "Fast time variations of supernova neutrino signals from 3-dimensional models". United States. https://doi.org/10.1103/PhysRevD.86.105031. https://www.osti.gov/servlets/purl/1327859.
@article{osti_1327859,
title = {Fast time variations of supernova neutrino signals from 3-dimensional models},
author = {Lund, Tina and Wongwathanarat, Annop and Janka, Hans -Thomas and Muller, Ewald and Raffelt, Georg},
abstractNote = {Here, we study supernova neutrino flux variations in the IceCube detector, using 3D models based on a simplified neutrino transport scheme. The hemispherically integrated neutrino emission shows significantly smaller variations compared with our previous study of 2D models, largely because of the reduced activity of the standing accretion shock instability in this set of 3D models which we interpret as a pessimistic extreme. For the studied cases, intrinsic flux variations up to about 100 Hz frequencies could still be detected in a supernova closer than about 2 kpc.},
doi = {10.1103/PhysRevD.86.105031},
journal = {Physical Review. D, Particles, Fields, Gravitation and Cosmology},
number = 10,
volume = 86,
place = {United States},
year = {Mon Nov 19 00:00:00 EST 2012},
month = {Mon Nov 19 00:00:00 EST 2012}
}

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Cited by: 33 works
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Works referencing / citing this record:

What can be learned from a future supernova neutrino detection?
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Observing Supernova Neutrino Light Curves with Super-Kamiokande: Expected Event Number over 10 s
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