ON COMPRESSED NUCLEAR MATTER: FROM NUCLEI TO NEUTRON STARS

DOI10.1142/S0218271811019864zbMath1263.85027MaRDI QIDQ4914554

Michael Rotondo, Remo Ruffini, Jorge A. Rueda, She-Sheng Xue

Publication date: 15 April 2013

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

zbMATH Keywords

Thomas-Fermi modelneutron star crustgeneral relativistic Thomas-Fermi treatmentneutron star corerelativistic Thomas-Fermi model

Mathematics Subject Classification ID

Strong interaction, including quantum chromodynamics (81V05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15)

Related Items (1)

Gravitational and electric energies in the collapse of a spherical thin-shell capacitor

Cites Work

• On the Thermodynamical Equilibrium of Fluids in Gravitational Fields
• Equations of State of Elements Based on the Generalized Fermi-Thomas Theory

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