ONE POSSIBLE MECHANISM FOR MASSIVE NEUTRON STAR SUPPORTED BY SOFT EOS
From MaRDI portal
Publication:4911491
DOI10.1142/S0218271812500368zbMath1263.85030arXiv1204.3030MaRDI QIDQ4911491
Dehua Wen, Jing Yan, Xue-Mei Liu
Publication date: 15 March 2013
Published in: International Journal of Modern Physics D (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1204.3030
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)
Cites Work
- Viscous cosmological model with variable gravitational and cosmological constants
- Cosmological models with variable \(G\) in \(C\)-field cosmology
- LET'S TALK ABOUT VARYING G
- The fundamental constants and their variation: observational and theoretical status
- Classical Field Theory of Nuclear Forces
- Relativistic Effects in Nuclear Forces
- Mach's Principle and a Relativistic Theory of Gravitation
- The Cosmological Constants
- Static Solutions of Einstein's Field Equations for Spheres of Fluid
- On Massive Neutron Cores