Efficient method for estimating the time evolution of the proto-neutron star mass and radius from a supernova neutrino signal
Author:
Affiliation:
1. Division of Science, National Astronomical Observatory of Japan , 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan
2. Astronomy Department and Theoretical Astrophysics Center, University of California , Berkeley, CA 94720, USA
Abstract
Funder
National Science Foundation
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://academic.oup.com/mnras/article-pdf/512/2/2806/43158747/stac383.pdf
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5. IceCube sensitivity for low-energy neutrinos from nearby supernovae
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