Upper Limit of Radiation from Coalescence of Rotating Hayward Black Holes

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Abstract

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.

Original languageEnglish
Article number09002
JournalEPJ Web of Conferences
Volume168
DOIs
StatePublished - 9 Jan 2018
Event13th International Conference on Gravitation, Astrophysics, and Cosmology. ICGAC 2017 and the 15th Italian-Korean Joint Symposium on Relativistic Astrophysics, IK 2017 - Seoul, Korea, Republic of
Duration: 3 Jul 20177 Jul 2017

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