QUANTUM STABILIZATION OF A RELATIVISTIC DEGENERATE STAR BEYOND THE CHANDRASEKHAR MASS LIMIT

DOI10.1142/S0218271804006334zbMath1065.83030MaRDI QIDQ4665627

Mark P. Silverman

Publication date: 11 April 2005

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

Mathematics Subject Classification ID

Gravitational interaction in quantum theory (81V17) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15)

Related Items (3)

Condensates in the cosmos: Quantum stabilization of the collapse of relativistic degenerate stars to black holes ⋮ GRAVITATIONALLY-INDUCED PARTICLE RESORPTION INTO THE VACUUM: A GENERAL SOLUTION TO THE PROBLEM OF BLACK HOLE COLLAPSE ⋮ FERMION CONDENSATION IN A RELATIVISTIC DEGENERATE STAR: ARRESTED COLLAPSE AND MACROSCOPIC EQUILIBRIUM

Cites Work

• Unnamed Item
• Dark matter as a cosmic Bose-Einstein condensate and possible superfluid
• The Large Scale Structure of Space-Time

This page was built for publication: QUANTUM STABILIZATION OF A RELATIVISTIC DEGENERATE STAR BEYOND THE CHANDRASEKHAR MASS LIMIT