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How Black Holes Form in High Energy Collisions

Authors
  • Kaloper, Nemanja
  • Terning, John
Type
Published Article
Publication Date
May 03, 2007
Submission Date
May 03, 2007
Identifiers
DOI: 10.1007/s10714-007-0468-5
Source
arXiv
License
Unknown
External links

Abstract

We elucidate how black holes form in trans-Planckian collisions. In the rest frame of one of the incident particles, the gravitational field of the other, which is rapidly moving, looks like a gravitational shock wave. The shock wave focuses the target particle down to a much smaller impact parameter. In turn, the gravitational field of the target particle captures the projectile when the resultant impact parameter is smaller than its own Schwarzschild radius, forming a black hole. One can deduce this by referring to the original argument of escape velocities exceeding the speed of light, which Michell and Laplace used to discover the existence of black holes.

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