Numerical hydrodynamics in special relativity.
Martí, José Maria, Müller, Ewald (2003)
Living Reviews in Relativity [electronic only]
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Martí, José Maria, Müller, Ewald (2003)
Living Reviews in Relativity [electronic only]
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Anninos, Peter (2001)
Living Reviews in Relativity [electronic only]
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Bisnovatyi-Kogan, G.S. (1999)
Discrete Dynamics in Nature and Society
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Psaltis, Dimitrios (2008)
Living Reviews in Relativity [electronic only]
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Kokkotas, Kostas D., Schmidt, Bernd G. (1999)
Living Reviews in Relativity [electronic only]
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Nicolas Besse, Norbert J. mauser, Eric Sonnendrücker (2007)
International Journal of Applied Mathematics and Computer Science
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We present a new numerical method to solve the Vlasov-Darwin and Vlasov-Poisswell systems which are approximations of the Vlasov-Maxwell equation in the asymptotic limit of the infinite speed of light. These systems model low-frequency electromagnetic phenomena in plasmas, and thus "light waves" are somewhat supressed, which in turn allows thenumerical discretization to dispense with the Courant-Friedrichs-Lewy condition on the time step. We construct a numerical scheme based on semi-Lagrangian...
Kostas Kokkotas (1997)
Banach Center Publications
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Pulsating stars are important sources of information for astrophysics. Nearly every star undergoes some kind of pulsation from the early stages of its formation until the very late ones i.e. the catastrophic creation of a supercompact object (white dwarf, neutron star or black hole). Pulsations of supercompact objects are of great importance for relativistic astrophysics since these pulsations are accompanied by the emission of gravitational radiation. In this review we shall discuss...
Ashtekar, Abhay, Krishnan, Badri (2004)
Living Reviews in Relativity [electronic only]
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Chamel, Nicolas, Haensel, Pawel (2008)
Living Reviews in Relativity [electronic only]
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Sathyaprakash, B.S., Schutz, Bernard F. (2009)
Living Reviews in Relativity [electronic only]
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Misao Sasaki (1997)
Banach Center Publications
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Gravitational radiation from a small mass particle orbiting a massive black hole can be analytically studied to a very high order in the post-Newtonian expansion. Thus it gives us useful information on the evolution of a coalescing compact binary star. In this talk, I report on recent progress made in the black-hole perturbation approach.
Yaremko, Yurij (2005)
SIGMA. Symmetry, Integrability and Geometry: Methods and Applications [electronic only]
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