High-Speed Cylindrical Collapse of Perfect Fluid
arXiv:gr-qc/0409042 · doi:10.1143/PTP.113.73
Abstract
The gravitational collapse of cylindrically distributed perfect fluid is studied. We assume the collapsing speed of fluid is very large and investigate such a situation by recently proposed high-speed approximation scheme. We show that if the value of the pressure divided by the energy density is bounded below by some positive value, the high-speed collapse is necessarily halted. This suggests that the collapsing perfect fluid of realistic ideal gas experiences the pressure bounce. However even in the case of mono-atomic ideal gas, arbitrarily large tidal force for freely falling observers are realizable by setting the initial collapsing velocity exceedingly large. In order that the high-speed collapse of cylindrical perfect fluid forms spacetime singularity, the equation of state should be very soft.
15pages, 1figure, PTPTex
Cited by in corpus (11)
- Cylindrical Systems in General Relativity
- High-Speed Cylindrical Collapse of Two Perfect Fluids
- Axially Symmetric Null dust Spacetime, Naked Singularity and Cosmic Time Machine
- Nonlinear evolution of cylindrical gravitational waves: numerical method and physical aspects
- Gravitational Radiation from Cylindrical Naked Singularity
- Cylindrical symmetric, non-rotating and non-static or static black hole solutions and the naked singularities
- Cylindrically symmetric models of gravitational collapse to black holes: a short review
- Visible borders of spacetime generated by high-energy collisions
- High-Speed Collapse of a Hollow Sphere of Type I Matter
- Axial symmetry Type N space-time with a naked curvature singularity and Closed Time-like Curves
- Black holes/naked singularities in four-dimensional non-static space-time and the energy-momentum distributions