skip to main content

DOE PAGESDOE PAGES

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

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:
OSTI Identifier:
1327859
Grant/Contract Number:
SC0006417
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)
Research Org:
North Carolina State Univ., Raleigh, NC (United States)
Sponsoring Org:
USDOE Office of Science (SC), Nuclear Physics (NP) (SC-26)
Country of Publication:
United States
Language:
English
Subject:
73 NUCLEAR PHYSICS AND RADIATION PHYSICS; 79 ASTRONOMY AND ASTROPHYSICS neutrino; supernova