The swallowing of a quark star by a black hole
arXiv:astro-ph/0206511 · doi:10.1046/j.1365-8711.2002.05819.x
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.
Minor changes in wording of abstract and introduction to match published version. Conclusions unchanged
References in corpus (1)
Cited by in corpus (36)
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