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Bombaci, I., Parenti, I. and Vidaña, I. (2004) Quark Deconfinement and Implications for the Radius and the Limiting Mass of Compact Stars. The Astrophysical Journal, 614, 314-325. astro-ph/0402404.
https://doi.org/10.1086/423658

has been cited by the following article:

• TITLE: Looking at the Physics of What a Quark Star-Black Hole Binary Would Create in Terms of GW Signals and New Physics

  AUTHORS: Andrew Beckwith

  KEYWORDS: GW Signals, Quark Star-Black Hole Binary, New Physics

  JOURNAL NAME: Journal of High Energy Physics, Gravitation and Cosmology, Vol.7 No.4, August 27, 2021

  ABSTRACT: A quark star, black hole pairing as a would-be Gravitational wave generator is brought up. Quark stars are, anyway, likely to be black holes, above a certain mass limit, whereas a quark star in itself obey thermodynamic “laws” which in certain ways differ from the traditional black hole models. We list some of the probable consequences of such a binary, and make predictions as to certain GW phenomenon which will have observational consequences. i.e., a GW “change in energy” from a black hole—Quark star pair would likely be within 90% of that of comparatively massed black hole—black hole binary pair. The electromagnetic “profile” of the two cases would differ dramatically, and we conclude our inquiry with an open question if a generalized uncertainty principle could play a role in comparing the 7th and 8th equations of our presentation.