Publication Date:
2018-11-08
Description:
Author(s): A. S. Schneider, M. E. Caplan, D. K. Berry, and C. J. Horowitz Nuclear pasta topology is an essential ingredient to determine transport properties in the inner crust of neutron stars. We perform semiclassical molecular dynamics simulations of nuclear pasta for proton fractions Y p = 0.30 and Y p = 0.40 near one-third of nuclear saturation density, n = 0.05 fm − 3 , at a te... [Phys. Rev. C 98, 055801] Published Wed Nov 07, 2018
Keywords:
Nuclear Astrophysics
Print ISSN:
0556-2813
Electronic ISSN:
1089-490X
Topics:
Physics