Thermo--inertial bouncing of a relativistic collapsing sphere: A numerical model
arXiv:gr-qc/0512032 · doi:10.1103/PhysRevD.73.024008
Abstract
We present a numerical model of a collapsing radiating sphere, whose boundary surface undergoes bouncing due to a decreasing of its inertial mass density (and, as expected from the equivalence principle, also of the ``gravitational'' force term) produced by the ``inertial'' term of the transport equation. This model exhibits for the first time the consequences of such an effect, and shows that under physically reasonable conditions this decreasing of the gravitational term in the dynamic equation may be large enough as to revert the collapse and produce a bouncing of the boundary surface of the sphere.
arXiv comment14 pages, 6 figures. To appear in Phys. Rev. D
References in corpus (11)
- Dynamics of dissipative gravitational collapse
- Transport processes in anisotropic gravitational collapse
- A causal model of radiating stellar collapse
- Shear-free radiating collapse and conformal flatness
- Radiating Collapse with Vanishing Weyl stresses
- Hyperbolic theories of dissipation: Why and when do we need them?
- Shear-free and homology conditions for self-gravitating dissipative fluids
- Relaxational effects in radiating stellar collapse
- Gravitational collapse: A case for thermal relaxation
- On the effective inertial mass density of a dissipative fluid
- Dissipative Collapse Through the Critical Point
Cited by in corpus (22)
- Dynamics of viscous dissipative gravitational collapse: A full causal approach
- Cylindrically Symmetric Relativistic Fluids: A Study Based on Structure Scalars
- Some analytical models of radiating collapsing spheres
- Tilted Lemaitre-Tolman-Bondi Spacetimes: Hydrodynamic and Thermodynamic Properties
- Dissipative collapse of axially symmetric, general relativistic, sources: A general framework and some applications
- Why Gravitational Contraction Must be Accompanied by Emission of Radiation Both in Newtonian and Einstein Gravity
- The inertia of heat and its role in the dynamics of dissipative collapse
- Quasi-static evolution of axially and reflection symmetric large-scale configuration
- Radiating Shear-Free Gravitational Collapse with Charge
- Likely formation of general relativistic radiation pressure supported stars or "eternally collapsing objects"
- Dynamics of Shearfree Dissipative Collapse in f(G) Gravity
- Radiation Pressure Supported Stars in Einstein Gravity: Eternally Collapsing Objects
- Higher Dimensional Inhomogeneous Perfect Fluid Collapse in \emph{f(R)} Gravity
- Dynamical Instability of Spherical Anisotropic Sources in Gravity
- Dynamics of Charged Bulk Viscous Collapsing Cylindrical Source With Heat Flux
- Models of Collapsing and Expanding Anisotropic Gravitating Source in Theory of Gravity
- Earliest stages of the non-equilibrium in axially symmetric, self-gravitating, dissipative fluids
- Nonadiabatic charged spherical evolution in the postquasistatic approximation
- Dynamics of Charged Viscous Dissipative Cylindrical Collapse With Full Causal Approach
- Shear Viscosity in the Post-quasistatic Approximation
- Dissipative Viscous Cylindrical Collapse in Gravity With Full Causal Approach
- General Relativistic Radiant Shock Waves in the Post-Quasistatic Approximation