Mass-gap for black hole formation in higher derivative and ghost free gravity
May 3, 20155 pages
Published in:
- Phys.Rev.Lett. 115 (2015) 5, 051102
- Published: Jul 31, 2015
e-Print:
- 1505.00492 [hep-th]
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Abstract: (APS)
We study a spherical gravitational collapse of a small mass in higher-derivative and ghost-free theories of gravity. By boosting a solution of linearized equations for a static point mass in such theories we obtain in the Penrose limit the gravitational field of an ultrarelativistic particle. Taking a superposition of such solutions we construct a metric of a collapsing null shell in the linearized higher-derivative and ghost-free gravity. The latter allows one to find the gravitational field of a thick null shell. By analyzing these solutions we demonstrate that in a wide class of the higher dimensional theories of gravity as well as for the ghost-free gravity there exists a mass gap for mini-black-hole production. We also found conditions when the curvature invariants remain finite at r=0 for the collapse of the thick null shell.Note:
- 4 pages
- 04.70.Bw
- 04.20.Jb
- derivative: high
- gravitation: collapse
- mass: gap
- black hole: production
- black hole: formation
- ghost
- Penrose limit
- curvature
References(19)
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