collaborators

1 paper

gr-qc2019

Comparison of post-Newtonian mode amplitudes with numerical relativity simulations of binary black holes

Ssohrab Borhanian, K. G. Arun, Harald P. Pfeiffer +1

Gravitational waves from the coalescence of two black holes carry the signature of the strong field dynamics of binary black holes. In this work we have used numerical relativity s…