Figure 11: Evolution of a highly spinning BH (
) during interaction with different
frequency GW packets, each with initial mass 
. Shown (in units where 
) are the
mass, irreducible mass, and angular momentum of the BH as inferred from AH properties. Image
reproduced with permission from [289], copyright by APS.
) during interaction with different
frequency GW packets, each with initial mass . Shown (in units where ) are the
mass, irreducible mass, and angular momentum of the BH as inferred from AH properties. Image
reproduced with permission from [289], copyright by APS.Vitor Cardoso and Leonardo Gualtieri and Carlos Herdeiro and Ulrich Sperhake, "Exploring New Physics Frontiers Through Numerical
Relativity",
Living Rev. Relativity, 18 (2015), 1, doi:10.1007/lrr-2015-1, URL (accessed <date>): http://www.livingreviews.org/lrr-2015-1.![]()
This work is licensed under a Creative Commons Attribution 4.0 International License.
© The author(s), except where otherwise noted.
Living Rev. Relativity, 18 (2015), 1, doi:10.1007/lrr-2015-1, URL (accessed <date>): http://www.livingreviews.org/lrr-2015-1.