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DETECTING THE SUPERNOVA BREAKOUT BURST IN TERRESTRIAL NEUTRINO DETECTORS

Journal Article · · Astrophysical Journal
;  [1]
  1. Department of Astrophysical Sciences, Princeton University, Princeton, NJ 08544 (United States)
We calculate the distance-dependent performance of a few representative terrestrial neutrino detectors in detecting and measuring the properties of the ν{sub e} breakout burst light curve in a Galactic core-collapse supernova. The breakout burst is a signature phenomenon of core collapse and offers a probe into the stellar core through collapse and bounce. We examine cases of no neutrino oscillations and oscillations due to normal and inverted neutrino-mass hierarchies. For the normal hierarchy, other neutrino flavors emitted by the supernova overwhelm the ν{sub e} signal, making a detection of the breakout burst difficult. For the inverted hierarchy (IH), some detectors at some distances should be able to see the ν{sub e} breakout burst peak and measure its properties. For the IH, the maximum luminosity of the breakout burst can be measured at 10 kpc to accuracies of ∼30% for Hyper-Kamiokande (Hyper-K) and ∼60% for the Deep Underground Neutrino Experiment (DUNE). Super-Kamiokande (Super-K) and Jiangmen Underground Neutrino Observatory (JUNO) lack the mass needed to make an accurate measurement. For the IH, the time of the maximum luminosity of the breakout burst can be measured in Hyper-K to an accuracy of ∼3 ms at 7 kpc, in DUNE to ∼2 ms at 4 kpc, and JUNO and Super-K can measure the time of maximum luminosity to an accuracy of ∼2 ms at 1 kpc. Detector backgrounds in IceCube render a measurement of the ν{sub e} breakout burst unlikely. For the IH, a measurement of the maximum luminosity of the breakout burst could be used to differentiate between nuclear equations of state.
OSTI ID:
22521603
Journal Information:
Astrophysical Journal, Journal Name: Astrophysical Journal Journal Issue: 2 Vol. 817; ISSN ASJOAB; ISSN 0004-637X
Country of Publication:
United States
Language:
English

Cited By (13)

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A Successful 3D Core-Collapse Supernova Explosion Model text January 2018
Characterizing the Gravitational Wave Signal from Core-collapse Supernovae journal April 2019
Three-Dimensional Supernova Explosion Simulations of 9-, 10-, 11-, 12-, and 13-M$_{\odot}$ Stars text January 2019
Neutrino signals of core-collapse supernovae in underground detectors journal August 2018
Characterizing the Gravitational Wave Signal from Core-Collapse Supernovae text January 2018
Revival of the Fittest: Exploding Core-Collapse Supernovae from 12 to 25 M$_{\odot}$ text January 2018
Fornax: A Flexible Code for Multiphysics Astrophysical Simulations journal February 2019
A successful 3D core-collapse supernova explosion model journal September 2018
Revival of the fittest: exploding core-collapse supernovae from 12 to 25 M⊙ journal March 2018
Global comparison of core-collapse supernova simulations in spherical symmetry text January 2018
Global comparison of core-collapse supernova simulations in spherical symmetry journal September 2018
Three-dimensional supernova explosion simulations of 9-, 10-, 11-, 12-, and 13-M⊙ stars journal February 2019

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