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Title: Heavy nuclei as thermal insulation for protoneutron stars

Journal Article · · Physical Review. C
; ;

Sponsoring Organization:
USDOE Office of Science (SC), Nuclear Physics (NP)
OSTI ID:
1427562
Journal Information:
Physical Review. C, Journal Name: Physical Review. C Vol. 97 Journal Issue: 3; ISSN 2469-9985
Publisher:
American Physical SocietyCopyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 20 works
Citation information provided by
Web of Science

References (32)

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Symmetry Parameter Constraints from a Lower Bound on Neutron-matter Energy journal October 2017
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Neutrino Signal of Electron-Capture Supernovae from Core Collapse to Cooling journal June 2010
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Observation of coherent elastic neutrino-nucleus scattering journal August 2017
Protoneutron Star Cooling with Convection: The Effect of the Symmetry Energy journal February 2012
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Mu‐ and Tau‐Neutrino Spectra Formation in Supernovae journal November 2001
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Coherent effects of a weak neutral current journal March 1974
Evolution of a proto-neutron star with a nuclear many-body equation of state: Neutrino luminosity and gravitational wave frequencies journal August 2017
Application of the nuclear equation of state obtained by the variational method to core-collapse supernovae journal February 2014
Protoneutron star evolution and the neutrino-driven wind in general relativistic neutrino radiation hydrodynamics simulations journal July 2010
Nuclear equation of state for core-collapse supernova simulations with realistic nuclear forces journal May 2017
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Supernova Explosion and Neutral Currents of Weak Interaction journal November 1975
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