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      Formation of black hole and emission of gravitational waves

      review-article

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          Abstract

          Numerical simulations were performed for the formation process of rotating black holes. It is suggested that Kerr black holes are formed for wide ranges of initial parameters. The nature of gravitational waves from a test particle falling into a Kerr black hole as well as the development of 3D numerical relativity for the coalescing binary neutron stars are discussed.

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          • Record: found
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          Gravitational-wave emission from rotating gravitational collapse.

          (1985)
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            The large scale structure of space time

            S. Hawking, G. Ellis, SW Hawking … (1973)
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              Phys. Rev. Lett

              R Gowdy (1971)
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                Author and article information

                Journal
                Journal ID (nlm-ta): Proc Jpn Acad Ser B Phys Biol Sci
                Journal ID (iso-abbrev): Proc. Jpn. Acad., Ser. B, Phys. Biol. Sci
                Journal ID (publisher-id): PJAB
                Title: Proceedings of the Japan Academy. Series B, Physical and Biological Sciences
                Publisher: The Japan Academy
                ISSN (Print): 0386-2208
                ISSN (Electronic): 1349-2896
                Publication date (Print): December 2006
                Publication date (Electronic): 12 February 2006
                Volume: 82
                Issue: 9
                Pages: 311-327
                Affiliations
                Department of Physics, Kyoto University, Kyoto, Japan
                Author notes

                (Communicated by Chushiro H ayashi, m.j.a.)

                [*)]

                Recipient of the Japan Academy Prize in 2005.

                [†) ]Department of Physics, Kyoto University, Kitashirakawa Oiwakecho, Sakyo-ku, Kyoto 606-8502, Japan (e-mail: takashi@ 123456tap.scphys.kyoto-u.ac.jp ).
                Article
                Publisher ID: 82_311
                PMC ID: 4338837
                PubMed ID: 25792793
                SO-VID: 1b582b5c-b90c-40fa-a799-5ec11dc731da
                Copyright © © 2006 The Japan Academy
                License:

                This is an open access article distributed under the terms of the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.

                History
                Date received : 25 August 2006
                Date accepted : 19 September 2006
                Categories
                Subject: Review

                ScienceOpen disciplines: Life sciences
                Keywords: black holes,gravitational waves,numerical simulations,perturbation of black holes
                Data availability:
                ScienceOpen disciplines: Life sciences
                Keywords: black holes, gravitational waves, numerical simulations, perturbation of black holes

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