Search results from PIRSA
2749 - 2760 of 16102 Results
Format results
-
-
-
A framework for the quasinormal mode shifts of arbitrary spin beyond-kerr black holes.
Asad Hussain The University of Texas at Austin
-
Pseudospectrum and black hole quasi-normal mode (in)stability
Rodrigo Panosso Macedo Queen Mary University of London
-
Efforts on calculating the gravitational sef-force using the Green function method [work in progress]
David Aruquipa Centro Brasileiro de Pesquisas Físicas
-
Progress in Green Function Methods for Extreme Mass Ratio Inspirals
Conor O'Toole National University of Ireland
-
Self-consistent adiabatic inspiral and transition motion
Lorenzo Küchler Université Libre de Bruxelles
-
Flux-balance laws in the Kerr spacetime
Alexander Grant University of Virginia
-
Improving Semi-Analytic Spin Precession with NITs
Michael LaHaye University of Guelph
-
Fast Self-Forced Inspirals into a Rotating Black Hole
Philip Lynch National University of Ireland
-
A multi-mode time-domain surrogate model for gravitational wave signals from comparable to extreme mass-ratio black hole binaries
Tousif Islam University of Massachusetts Dartmouth
-
Kerr self-force via elliptic PDEs: Numerical methods (part 2)
Thomas Osburn State University of New York (SUNY)