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• W2033418923 abstract "We study the head-on collision of fluid particles well within the kinetic energy dominated regime ($ensuremath{gamma}=8$ to 12) by numerically solving the Einstein-hydrodynamic equations. We find that the threshold for black hole formation is lower (by a factor of a few) than simple hoop conjecture estimates, and, moreover, near this threshold two distinct apparent horizons first form postcollision and then merge. We argue that this can be understood in terms of a gravitational focusing effect. The gravitational radiation reaches luminosities of $0.014text{ }{c}^{5}/G$, carrying $16ifmmodepmelsetextpmfi{}2%$ of the total energy." @default.
• W2033418923 created "2016-06-24" @default.
• W2033418923 creator A5019617791 @default.
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• W2033418923 date "2013-03-07" @default.
• W2033418923 modified "2023-10-14" @default.
• W2033418923 title "Ultrarelativistic Black Hole Formation" @default.
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• W2033418923 doi "https://doi.org/10.1103/physrevlett.110.101101" @default.
• W2033418923 hasPubMedId "https://pubmed.ncbi.nlm.nih.gov/23521246" @default.
• W2033418923 hasPublicationYear "2013" @default.
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