An evolution of adiabatic matter: a case for the quasistatic regime

DOI10.1007/S10714-013-1580-3zbMath1274.83008arXiv1308.0077OpenAlexW3098497883MaRDI QIDQ378861

Mohammad Hasan, H. S. Yoon

Publication date: 12 November 2013

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1308.0077

zbMATH Keywords

matter evolutioncharacteristic formulation for matternonradiating evolution

Mathematics Subject Classification ID

Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Exact solutions to problems in general relativity and gravitational theory (83C15)

Cites Work

• Unnamed Item
• Numerical hydrodynamics and magnetohydrodynamics in general relativity
• Evolution of radiating viscous spheres and gravitational collapse
• Ultrarelativistic fluid dynamics
• RELATIVISTIC GRAVITATIONAL COLLAPSE IN COMOVING COORDINATES: THE POST-QUASISTATIC APPROXIMATION
• Black-hole threshold solutions in stiff fluid collapse
• The contraction of gravitating spheres
• Junction conditions and the propagation of isometries in general relativity
• Static Solutions of Einstein's Field Equations for Spheres of Fluid
• On Massive Neutron Cores
• Bondian frames to couple matter with radiation

This page was built for publication: An evolution of adiabatic matter: a case for the quasistatic regime