Black hole-neutron star binaries in general relativity: Quasiequilibrium formulation

We present a new numerical method for the construction of quasiequilibrium models of black hole-neutron star binaries. We solve the constraint equations of general relativity, decomposed in the conformal thin-sandwich formalism, together with the Euler equation for the neutron star matter. We take t...

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Veröffentlicht in:	Physical review. D, Particles and fields Particles and fields, 2004-09, Vol.70 (6), Article 064040
Hauptverfasser:	Baumgarte, Thomas W., Skoge, Monica L., Shapiro, Stuart L.
Format:	Artikel
Sprache:	eng
Schlagworte:	BINARY STARS BLACK HOLES COMPARATIVE EVALUATIONS COSMOLOGY EQUATIONS OF STATE GENERAL RELATIVITY THEORY GRAVITATION NEUTRON STARS NUCLEAR MATTER PHYSICS OF ELEMENTARY PARTICLES AND FIELDS RELATIVISTIC RANGE VECTORS
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