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2014

Ultra-high-energy debris from the collisional Penrose process

Berti, Emanuele, Brito, Richard, Cardoso, Vitor

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Soon after the discovery of the Kerr metric, Penrose realized that superradiance can be exploited to extract energy from black holes.

The original idea (involving the breakup of a single particle) yields only modest energy gains.
A variant of the Penrose process consists of particle collisions in the ergoregion.
The collisional Penrose process has been explored recently in the context of dark matter searches, with the conclusion that the ratio $\eta$ between the energy of post-collision particles detected at infinity and the energy of the colliding particles should be modest ($\eta \lesssim 1.5$).

Ultra-high-energy debris from the collisional Penrose process · Around

Built on

R. P. Kerr, Phys. Rev. Lett. 11
1963
Earlier work this paper cites.
M. Schmidt, Nature 197
1963
Earlier work this paper cites.
R. Penrose, Nuovo Cimento.J. Serie 1
1969
Earlier work this paper cites.
J. M. Bardeen, W. H. Press, and S. A. Teukolsky, Astrophys.J. 178
1972
Earlier work this paper cites.
R. M. Wald, Astrophys.J. 191
1974
Earlier work this paper cites.
K. S. Thorne, Astrophys.J. 191
1974
Earlier work this paper cites.
T. Piran, J. Shaham, and J. Katz, Astrophys.J. 196
1975
Earlier work this paper cites.
T. Piran and J. Shaham, Phys.Rev. D16
1977
Earlier work this paper cites.
S. Wagh, S. Dhurandhar, and N. Dadhich, Astrophys.J. 290
1985
Earlier work this paper cites.
S. M. Wagh, S. V. Dhurandhar, and N. Dadhich, Astrophys.J. 301
1986
Earlier work this paper cites.

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