%0 Journal Article
%T Looking at the Physics of What a Quark Star-Black Hole Binary Would Create in Terms of GW Signals and New Physics
%A Andrew Beckwith
%J Journal of High Energy Physics, Gravitation and Cosmology
%P 1255-1263
%@ 2380-4335
%D 2021
%I Scientific Research Publishing
%R 10.4236/jhepgc.2021.74075
%X 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>i.e.</i>, a GW ¡°change in energy¡± from a black hole¡ªQuark star pair would likely be within 90% of that of comparatively massed black hole¡ªblack 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 7<sup>th</sup> and 8<sup>th</sup> equations of our presentation.
%K GW Signals
%K Quark Star-Black Hole Binary
%K New Physics
%U http://www.scirp.org/journal/PaperInformation.aspx?PaperID=111522