Computational Relativity in Bondi-Sachs formalism

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9783639702811: Computational Relativity in Bondi-Sachs formalism
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The remainder of the last century has seen compact objects been the centre study of general relativist astrophysics especially black hole-black hole, black hole-neutron star and neutron star-neutron binaries which are said to be the main sources of gravitational radiation in our universe. Convincing major research results have been obtained thus far prompting the development of gravitational wave astronomy. In the distant future, gravitational wave detectors which are being build will detect gravitational wave signals from compact relativistic binaries sources and also from relativistic collapsing sources. In order to theoretically study these sources in this book, we specifically linearize gravity within a Schwarzschild geometry using the Bondi-Sach formalism and we study the resulting perturbations , and for the first time, we obtain quasi-normal modes of a Schwarzschild white hole. We then apply these perturbations to study the emitted gravitational radiation at null infinity from a relativistic system consisting of a point particle in close orbit around a stationary Schwarzschild black hole.

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L'autore:

Dr. Amos Soweto Kubeba has the following degrees; BSc(Mathematics and Physics) and BScHons(Physics) both from the University of Natal (UP), and MSc (Applied Mathematics)(Cum-Laude), PhD (Applied Mathematics) both from the University of South Africa (UNISA). He is currecntly a senior lecturer in the department of mathematical sciences at UNISA.

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Kubeka Amos
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ISBN 10: 3639702816 ISBN 13: 9783639702811
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Descrizione libro Scholars' Press 2013-11-08, 2013. paperback. Condizione: New. Codice articolo 9783639702811

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Descrizione libro Condizione: New. Publisher/Verlag: Scholar's Press | The remainder of the last century has seen compact objects been the centre study of general relativist astrophysics especially black hole-black hole, black hole-neutron star and neutron star-neutron binaries which are said to be the main sources of gravitational radiation in our universe. Convincing major research results have been obtained thus far prompting the development of gravitational wave astronomy. In the distant future, gravitational wave detectors which are being build will detect gravitational wave signals from compact relativistic binaries sources and also from relativistic collapsing sources. In order to theoretically study these sources in this book, we specifically linearize gravity within a Schwarzschild geometry using the Bondi-Sach formalism and we study the resulting perturbations , and for the first time, we obtain quasi-normal modes of a Schwarzschild white hole. We then apply these perturbations to study the emitted gravitational radiation at null infinity from a relativistic system consisting of a point particle in close orbit around a stationary Schwarzschild black hole. | Format: Paperback | Language/Sprache: english | 188 pp. Codice articolo K9783639702811

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Descrizione libro Scholars' Press, 2013. PAP. Condizione: New. New Book. Delivered from our UK warehouse in 4 to 14 business days. THIS BOOK IS PRINTED ON DEMAND. Established seller since 2000. Codice articolo LQ-9783639702811

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Descrizione libro SPS Nov 2013, 2013. Taschenbuch. Condizione: Neu. This item is printed on demand - Print on Demand Neuware - The remainder of the last century has seen compact objects been the centre study of general relativist astrophysics especially black hole-black hole, black hole-neutron star and neutron star-neutron binaries which are said to be the main sources of gravitational radiation in our universe. Convincing major research results have been obtained thus far prompting the development of gravitational wave astronomy. In the distant future, gravitational wave detectors which are being build will detect gravitational wave signals from compact relativistic binaries sources and also from relativistic collapsing sources. In order to theoretically study these sources in this book, we specifically linearize gravity within a Schwarzschild geometry using the Bondi-Sach formalism and we study the resulting perturbations , and for the first time, we obtain quasi-normal modes of a Schwarzschild white hole. We then apply these perturbations to study the emitted gravitational radiation at null infinity from a relativistic system consisting of a point particle in close orbit around a stationary Schwarzschild black hole. 188 pp. Englisch. Codice articolo 9783639702811

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Descrizione libro SPS Nov 2013, 2013. Taschenbuch. Condizione: Neu. Neuware - The remainder of the last century has seen compact objects been the centre study of general relativist astrophysics especially black hole-black hole, black hole-neutron star and neutron star-neutron binaries which are said to be the main sources of gravitational radiation in our universe. Convincing major research results have been obtained thus far prompting the development of gravitational wave astronomy. In the distant future, gravitational wave detectors which are being build will detect gravitational wave signals from compact relativistic binaries sources and also from relativistic collapsing sources. In order to theoretically study these sources in this book, we specifically linearize gravity within a Schwarzschild geometry using the Bondi-Sach formalism and we study the resulting perturbations , and for the first time, we obtain quasi-normal modes of a Schwarzschild white hole. We then apply these perturbations to study the emitted gravitational radiation at null infinity from a relativistic system consisting of a point particle in close orbit around a stationary Schwarzschild black hole. 188 pp. Englisch. Codice articolo 9783639702811

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Descrizione libro SPS Nov 2013, 2013. Taschenbuch. Condizione: Neu. Neuware - The remainder of the last century has seen compact objects been the centre study of general relativist astrophysics especially black hole-black hole, black hole-neutron star and neutron star-neutron binaries which are said to be the main sources of gravitational radiation in our universe. Convincing major research results have been obtained thus far prompting the development of gravitational wave astronomy. In the distant future, gravitational wave detectors which are being build will detect gravitational wave signals from compact relativistic binaries sources and also from relativistic collapsing sources. In order to theoretically study these sources in this book, we specifically linearize gravity within a Schwarzschild geometry using the Bondi-Sach formalism and we study the resulting perturbations , and for the first time, we obtain quasi-normal modes of a Schwarzschild white hole. We then apply these perturbations to study the emitted gravitational radiation at null infinity from a relativistic system consisting of a point particle in close orbit around a stationary Schwarzschild black hole. 188 pp. Englisch. Codice articolo 9783639702811

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Descrizione libro Scholars Press, 2013. Paperback. Condizione: New. Language: English . Brand New Book. The remainder of the last century has seen compact objects been the centre study of general relativist astrophysics especially black hole-black hole, black hole-neutron star and neutron star-neutron binaries which are said to be the main sources of gravitational radiation in our universe. Convincing major research results have been obtained thus far prompting the development of gravitational wave astronomy. In the distant future, gravitational wave detectors which are being build will detect gravitational wave signals from compact relativistic binaries sources and also from relativistic collapsing sources. In order to theoretically study these sources in this book, we specifically linearize gravity within a Schwarzschild geometry using the Bondi-Sach formalism and we study the resulting perturbations, and for the first time, we obtain quasi-normal modes of a Schwarzschild white hole. We then apply these perturbations to study the emitted gravitational radiation at null infinity from a relativistic system consisting of a point particle in close orbit around a stationary Schwarzschild black hole. Codice articolo KNV9783639702811

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Descrizione libro Scholars' Press. Paperback. Condizione: New. 188 pages. Dimensions: 8.7in. x 5.9in. x 0.4in.The remainder of the last century has seen compact objects been the centre study of general relativist astrophysics especially black hole-black hole, black hole-neutron star and neutron star-neutron binaries which are said to be the main sources of gravitational radiation in our universe. Convincing major research results have been obtained thus far prompting the development of gravitational wave astronomy. In the distant future, gravitational wave detectors which are being build will detect gravitational wave signals from compact relativistic binaries sources and also from relativistic collapsing sources. In order to theoretically study these sources in this book, we specifically linearize gravity within a Schwarzschild geometry using the Bondi-Sach formalism and we study the resulting perturbations , and for the first time, we obtain quasi-normal modes of a Schwarzschild white hole. We then apply these perturbations to study the emitted gravitational radiation at null infinity from a relativistic system consisting of a point particle in close orbit around a stationary Schwarzschild black hole. This item ships from multiple locations. Your book may arrive from Roseburg,OR, La Vergne,TN. Paperback. Codice articolo 9783639702811

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