paper

Observation of critical phenomena and self-similarity in the gravitational collapse of radiation fluid

arXiv:gr-qc/9402041 · doi:10.1103/PhysRevLett.72.1782

Abstract

We observe critical phenomena in spherical collapse of radiation fluid. A sequence of spacetimes is numerically computed, containing models () that adiabatically disperse and models () that form a black hole. Near the critical point (), evolutions develop a self-similar region within which collapse is balanced by a strong, inward-moving rarefaction wave that holds constant as a function of a self-similar coordinate . The self-similar solution is known and we show near-critical evolutions asymptotically approaching it. A critical exponent is found for supercritical () models.

10 pages (LaTeX) (to appear in Phys. Rev. Lett.), TAR-039-UNC

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