activity
20012026
most citedTotal recoil: the maximum kick from nonspinning black-hole binary inspiral

487 citations · 4.7k across the 48 of their papers we have counts for

collaborators
Showing 2007 · gr-qcShow all

11 papers · 2 filters

gr-qc2007★ 58 cited

Multipolar analysis of spinning binaries

E. Berti, V. Cardoso, J. A. Gonzalez +2

We present a preliminary study of the multipolar structure of gravitational radiation from spinning black hole binary mergers. We consider three different spinning binary configura…

gr-qc2007★ 113 cited

Eccentric binary black-hole mergers: The transition from inspiral to plunge in general relativity

U. Sperhake, E. Berti, V. Cardoso +3

We study the transition from inspiral to plunge in general relativity by computing gravitational waveforms of non-spinning, equal-mass black-hole binaries. We consider three sequen…

gr-qc2007★ 203 cited

Exploring black hole superkicks

Bernd Bruegmann, Jose Gonzalez, Mark Hannam +2

Recent calculations of the recoil velocity in black-hole binary mergers have found kick velocities of km/s for equal-mass binaries with anti-aligned initial spins in…

gr-qc2007★ 108 cited

Reducing eccentricity in black-hole binary evolutions with initial parameters from post-Newtonian inspiral

Sascha Husa, Mark Hannam, Jose A. Gonzalez +2

Standard choices of quasi-circular orbit parameters for black-hole binary evolutions result in eccentric inspiral. We introduce a conceptually simple method, which is to integrate…

gr-qc2007★ 149 cited

Reducing phase error in long numerical binary black hole evolutions with sixth order finite differencing

Sascha Husa, Jose A. Gonzalez, Mark Hannam +2

We describe a modification of a fourth-order accurate ``moving puncture'' evolution code, where by replacing spatial fourth-order accurate differencing operators in the bulk of the…

gr-qc2007★ 179 cited

Where post-Newtonian and numerical-relativity waveforms meet

Mark Hannam, Sascha Husa, Jose A. Gonzalez +2

We analyze numerical-relativity (NR) waveforms that cover nine orbits (18 gravitational-wave cycles) before merger of an equal-mass system with low eccentricity, with numerical unc…