Abstract
I summarize results from a numerical study of spherically symmetric collapse of a massless scalar field. I consider families of solutions, scrS[p], with the property that a critical parameter value, , separates solutions containing black holes from those which do not. I present evidence in support of conjectures that (1) the strong-field evolution in the p→ limit is universal and generates structure on arbitrarily small spatiotemporal scales and (2) the masses of black holes which form satisfy a power law ∝‖p-, where γ≊0.37 is a universal exponent.
- Received 22 September 1992
DOI:https://doi.org/10.1103/PhysRevLett.70.9
©1993 American Physical Society
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