Radiative gravitational collapse to black holes in five dimensions

We review recent results about the modelling of radiating gravitational collapse to Schwarzschild-Tangherlini black holes. In particular, we prove that classes of five dimensional collapsing solutions built on Riemannian Bianchi IX spatial metrics can be matched to radiating exteriors given by the B...

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Bibliographic Details
Main Author: Mena, Filipe C. (author)
Format: conferencePaper
Language:eng
Published: 2012
Subjects:
General relativity
Black holes
Spacetime junctions
Gravitational collapse
Gravitational waves
Science & Technology
Online Access:http://hdl.handle.net/1822/24466
Country:Portugal
Oai:oai:repositorium.sdum.uminho.pt:1822/24466
Description
Summary:We review recent results about the modelling of radiating gravitational collapse to Schwarzschild-Tangherlini black holes. In particular, we prove that classes of five dimensional collapsing solutions built on Riemannian Bianchi IX spatial metrics can be matched to radiating exteriors given by the Bizo´n-Chmaj-Schmidt metric. We show that the data at the boundary for the exterior can be chosen to be close to the data for the Schwarzschild-Tangherlini solution which is known to be stable

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