1.1k citations · 7.4k across the 52 of their papers we have counts for
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gr-qc2011★ 36 cited
Analytical meets numerical relativity - status of complete gravitational waveform models for binary black holes
Frank Ohme
Models of gravitational waveforms from coalescing black-hole binaries play a crucial role in the efforts to detect and interpret the signatures of those binaries in the data of lar…
gr-qc2011★ 52 cited
Reliability of complete gravitational waveform models for compact binary coalescences
Frank Ohme, Mark Hannam, Sascha Husa
With recent advances in post-Newtonian (PN) theory and numerical relativity (NR) it has become possible to construct inspiral-merger-ringdown waveforms by combining both descriptio…
astro-ph.HE2011★ 128 cited
Will black hole-neutron star binary inspirals tell us about the neutron star equation of state?
Francesco Pannarale, Luciano Rezzolla, Frank Ohme +1
The strong tidal forces that arise during the last stages of the life of a black hole-neutron star binary may severely distort, and possibly disrupt, the star. Both phenomena will…