Please use this identifier to cite or link to this item: http://dspace.mediu.edu.my:8181/xmlui/handle/123456789/8672
Title: Quasi-Normal Modes of Stars and Black Holes
Keywords: Relativity in Astrophysics
Issue Date: 1-Jun-2013
Publisher: Albert Einstein Institut, Max-Planck Institute for Gravitati
Description: Perturbations of stars and black holes have been one of the main topics of relativistic astrophysics for the last few decades. They are of particular importance today, because of their relevance to gravitational wave astronomy. In this review we present the theory of quasi-normal modes of compact objects from both the mathematical and astrophysical points of view. The discussion includes perturbations of black holes (Schwarzschild, Reissner-Nordström, Kerr and Kerr-Newman) and relativistic stars (non-rotating and slowly-rotating). The properties of the various families of quasi-normal modes are described, and numerical techniques for calculating quasi-normal modes reviewed. The successes, as well as the limits, of perturbation theory are presented, and its role in the emerging era of numerical relativity and supercomputers is discussed.
URI: http://koha.mediu.edu.my:8181/jspui/handle/123456789/8672
Other Identifiers: http://www.livingreviews.org/lrr-1999-2
http://www.doaj.org/doaj?func=openurl&genre=article&issn=14338351&date=1999&volume=2&issue=&spage=2
Appears in Collections:Physics and Astronomy

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