Nuclear matter and its role in supernovae, neutron stars and compact object binary mergers
Top Cited Papers
- 26 June 2000
- journal article
- other
- Published by Elsevier in Physics Reports
- Vol. 333-334, 121-146
- https://doi.org/10.1016/s0370-1573(00)00019-3
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This publication has 44 references indexed in Scilit:
- Physical acceptability of isolated, static, spherically symmetric, perfect fluid solutions of Einstein's equationsPublished by Elsevier ,1999
- Asymmetric Nuclear Matter and Neutron Star PropertiesPhysical Review Letters, 1994
- Tidal interactions of inspiraling compact binariesThe Astrophysical Journal, 1992
- Coalescing binary neutron starsThe Astrophysical Journal, 1992
- The incompressibility of nuclear matter and the breathing modePhysics Letters B, 1991
- Reconciliation of neutron-star masses and binding of the Λ in hypernucleiPhysical Review Letters, 1991
- The nuclear symmetry energy in relativistic Brueckner-Hartree-Fock calculationsPhysics Letters B, 1987
- Type II supernova energeticsThe Astrophysical Journal, 1985
- Volume and surface symmetry energy coefficients from photoabsorption cross sectionsPhysics Letters B, 1982
- Static Solutions of Einstein's Field Equations for Spheres of FluidPhysical Review B, 1939