The swallowing of a quark star by a black hole

Preprint

30 August 2002

preprint
Published by arXiv in arXiv

https://doi.org/10.48550/arXiv.astro-ph/0206511

Abstract

In 3-d SPH simulations of the coalescence of a quark star with a pseudo-Newtonian black hole all of the quark matter is quickly accreted by the black hole. The Madsen-Caldwell-Friedman argument against the existence of quark stars may need to be re-examined.

Keywords

FRIEDMAN ARGUMENT
NEWTONIAN BLACK
SWALLOWING
BLACK HOLE
QUARK STAR
ACCRETED
STAR

All Related Versions

Version 1, 2002-06-28, ArXiv
Version 2, 2002-08-30, ArXiv
Published version: Monthly Notices of the Royal Astronomical Society, 335 (1), L29.

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