Energy and angular momentum radiated for non head-on binary black hole collisions
classification
🌀 gr-qc
keywords
angularenergymomentumradiatedtotalbinaryblackhole
read the original abstract
We investigate the possible total radiated energy produced by a binary black hole system containing non-vanishing total angular momentum. For the scenearios considered we find that the total radiated energy does not exceed 1%. Additionally we explore the gravitational radiation field and the variation of angular momentum in the process.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.