EQUATION OF STATE FOR DENSE SUPERNOVA MATTER

DOI10.1142/S0218271809015023zbMath1181.85036arXiv0811.4232MaRDI QIDQ3401075

Ch. C. Moustakidis

Publication date: 28 January 2010

Published in: International Journal of Modern Physics D (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/0811.4232

zbMATH Keywords

supernovaequation of stateeffective interactionneutron starnuclear symmetry energyhot nuclear matterproton fraction

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15)

Related Items (2)

Thermal effects on tidal deformability in the last orbits of an inspiraling binary neutron star system ⋮ ROLE OF DISTRIBUTION FUNCTION ON CHARACTERISTIC PROPERTIES OF SUPERNOVA MATTER

Cites Work

• NUCLEAR SYMMETRY ENERGY EFFECTS ON NEUTRON STARS PROPERTIES
• Protoneutron stars within the Brueckner-Bethe-Goldstone theory

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