Upper Limit of Radiation from Coalescence of Rotating Hayward Black Holes

We review the upper limit of the gravitational radiation thermally allowed under the collision of two rotating Hayward black holes. The upper limit is dependent on the gravitational spin interaction between black holes and is useful to determine one of the parameters for consistency with Laser Inter...

Full description

Bibliographic Details
Main Author: Gwak Bogeun
Format: Article
Language:English
Published: EDP Sciences 2018-01-01
Series:EPJ Web of Conferences
Online Access:https://doi.org/10.1051/epjconf/201816809002
id doaj-d73964639fa543eba71864047b96ba14
record_format Article
spelling doaj-d73964639fa543eba71864047b96ba142021-08-02T07:10:37ZengEDP SciencesEPJ Web of Conferences2100-014X2018-01-011680900210.1051/epjconf/201816809002epjconf_icgaxiii-ik2018_09002Upper Limit of Radiation from Coalescence of Rotating Hayward Black HolesGwak BogeunWe review the upper limit of the gravitational radiation thermally allowed under the collision of two rotating Hayward black holes. The upper limit is dependent on the gravitational spin interaction between black holes and is useful to determine one of the parameters for consistency with Laser Interferometer Gravitational-Wave Observatory (LIGO) data.https://doi.org/10.1051/epjconf/201816809002
collection DOAJ
language English
format Article
sources DOAJ
author Gwak Bogeun
spellingShingle Gwak Bogeun
Upper Limit of Radiation from Coalescence of Rotating Hayward Black Holes
EPJ Web of Conferences
author_facet Gwak Bogeun
author_sort Gwak Bogeun
title Upper Limit of Radiation from Coalescence of Rotating Hayward Black Holes
title_short Upper Limit of Radiation from Coalescence of Rotating Hayward Black Holes
title_full Upper Limit of Radiation from Coalescence of Rotating Hayward Black Holes
title_fullStr Upper Limit of Radiation from Coalescence of Rotating Hayward Black Holes
title_full_unstemmed Upper Limit of Radiation from Coalescence of Rotating Hayward Black Holes
title_sort upper limit of radiation from coalescence of rotating hayward black holes
publisher EDP Sciences
series EPJ Web of Conferences
issn 2100-014X
publishDate 2018-01-01
description We review the upper limit of the gravitational radiation thermally allowed under the collision of two rotating Hayward black holes. The upper limit is dependent on the gravitational spin interaction between black holes and is useful to determine one of the parameters for consistency with Laser Interferometer Gravitational-Wave Observatory (LIGO) data.
url https://doi.org/10.1051/epjconf/201816809002
work_keys_str_mv AT gwakbogeun upperlimitofradiationfromcoalescenceofrotatinghaywardblackholes
_version_ 1721239609170460672