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

作　　者：Andrew Beckwith Andrew Beckwith(Physics Department, College of Physics, Chongqing University, Chongqing, China)

机构地区：[1]Physics Department, College of Physics, Chongqing University, Chongqing, China

出　　处：《Journal of High Energy Physics, Gravitation and Cosmology》2021年第4期1255-1263,共9页高能物理（英文）

摘　　要：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—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 7^th and 8^th equations of our presentation.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—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 7^th and 8^th equations of our presentation.

关 键 词：GW Signals Quark Star-Black Hole Binary New Physics 

分 类 号：O57[理学—粒子物理与原子核物理]