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2019ApJ...878...25N - Astrophys. J., 878, 25-25 (2019/June-2)
Cooling timescale for protoneutron stars and properties of nuclear matter: effective mass and symmetry energy at high densities.
NAKAZATO K. and SUZUKI H.
Abstract (from CDS):
Abstract Copyright: © 2019. The American Astronomical Society. All rights reserved.
Journal keyword(s): dense matter - equation of state - neutrinos - stars: neutron - supernovae: general
Simbad objects: 3
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