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| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | East, William E | - |
| dc.contributor.author | Pretorius, Frans | - |
| dc.date.accessioned | 2018-07-20T15:10:07Z | - |
| dc.date.available | 2018-07-20T15:10:07Z | - |
| dc.date.issued | 2013-03-08 | en_US |
| dc.identifier.citation | East, William E, Pretorius, Frans. (2013). Ultrarelativistic Black Hole Formation. PHYSICAL REVIEW LETTERS, 110 (10.1103/PhysRevLett.110.101101 | en_US |
| dc.identifier.issn | 0031-9007 | - |
| dc.identifier.uri | http://arks.princeton.edu/ark:/88435/pr1vh53 | - |
| dc.description.abstract | We study the head-on collision of fluid particles well within the kinetic energy dominated regime (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: 014 c(5)/G, carrying 16 +/- 2% of the total energy. DOI: 10.1103/PhysRevLett.110.101101 | en_US |
| dc.language.iso | en_US | en_US |
| dc.relation.ispartof | PHYSICAL REVIEW LETTERS | en_US |
| dc.rights | Final published version. Article is made available in OAR by the publisher's permission or policy. | en_US |
| dc.title | Ultrarelativistic Black Hole Formation | en_US |
| dc.type | Journal Article | en_US |
| dc.identifier.doi | doi:10.1103/PhysRevLett.110.101101 | - |
| dc.date.eissued | 2013-03-07 | en_US |
| dc.identifier.eissn | 1079-7114 | - |
| pu.type.symplectic | http://www.symplectic.co.uk/publications/atom-terms/1.0/journal-article | en_US |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| PhysRevLett.110.101101.pdf | 1.57 MB | Adobe PDF | View/Download |
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