EXACT AND QUASI-EXACT MODELS OF STRANGE STARS

DOI10.1142/S0218271810018128zbMath1204.85020arXiv1006.4629MaRDI QIDQ3067228

J. E. Horvath, M. G. B. de Avellar

Publication date: 20 January 2011

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

Full work available at URL: https://arxiv.org/abs/1006.4629

zbMATH Keywords

exact solutionscompact objectsstrange stars

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) Exact solutions to problems in general relativity and gravitational theory (83C15)

Related Items (3)

Entropy, complexity and disequilibrium in compact stars ⋮ Exact solutions for compact stars with CFL quark matter ⋮ Information theoretical methods as discerning quantifiers of the equations of state of neutron stars

Cites Work

• Unnamed Item
• Physical acceptability of isolated, static, spherically symmetric, perfect fluid solutions of Einstein's equations
• General Relativistic Fluid Spheres
• Anisotropic stars in general relativity
• Static Solutions of Einstein's Field Equations for Spheres of Fluid

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