Critical gravitational collapse with angular momentum: from critical exponents to universal scaling functions

Details Critical gravitational collapse with angular momentum: from critical exponents to universal scaling functions Critical gravitational collapse with angular momentum: from critical exponents to universal scaling functions

2001-10-09

arxiv.org/abs/gr-qc/0110049v1

Phys.Rev. D65 (2002) 064019

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

RevTex, 14 pages, 5 eps figures

Scientific paper

10.1103/PhysRevD.65.064019

We investigate the threshold of gravitational collapse with angular momentum, under the assumption that the critical solution is spherical and self-similar and has two growing modes, namely one spherical mode and one axial dipole mode (threefold degenerate). This assumption holds for perfect fluid matter with the equation of state p=kappa rho if the constant kappa is in the range 0

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