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• W1994298022 abstract "We report a second example of critical behavior in gravitational collapse. Collapse of axisymmetric gravitational wave packets is computed numerically for a one-parameter family of initial data. A black hole first appears along the sequence at a critical parameter value ${mathit{p}}^{mathrm{*}}$. As with spherical scalar-field collapse, a power law is found to relate black-hole mass (the order parameter) and critical separation: ${mathit{M}}_{mathrm{BH}}$ensuremath{propto}ensuremath{Vert}p-${mathit{p}}^{mathrm{*}}$${mathrm{ensuremath{Vert}}}^{mathrm{ensuremath{beta}}}$. The critical exponent is ensuremath{beta}ensuremath{simeq}0.37, remarkably close to that observed by Choptuik. Near-critical evolutions produce echoes from the strong-field region which appear to exhibit scaling." @default.
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• W1994298022 date "1993-05-17" @default.
• W1994298022 modified "2023-10-18" @default.
• W1994298022 title "Critical behavior and scaling in vacuum axisymmetric gravitational collapse" @default.
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• W1994298022 doi "https://doi.org/10.1103/physrevlett.70.2980" @default.
• W1994298022 hasPubMedId "https://pubmed.ncbi.nlm.nih.gov/10053745" @default.
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