activity
20172023
most citedEccentric, nonspinning, inspiral, Gaussian-process merger approximant for the detection and characterization of eccentric binary black hole mergers

156 citations · 372 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.HE2023★ 4 cited

Effect of magnetic fields on the dynamics and gravitational wave emission of PPI-saturated self-gravitating accretion disks: simulations in full GR

Erik Wessel, Vasileios Paschalidis, Antonios Tsokaros +2

We explore the effect magnetic fields have on self-gravitating accretion disks around spinning black holes via numerical evolutions in full dynamical magnetohydrodynamic spacetimes…

astro-ph.HE2020★ 17 cited

Gravitational Waves from Disks Around Spinning Black Holes: Simulations in Full General Relativity

Erik Wessel, Vasileios Paschalidis, Antonios Tsokaros +2

We present fully general-relativistic numerical evolutions of self-gravitating tori around spinning black holes with dimensionless spin parallel or anti-parallel to the…

astro-ph.HE2019★ 149 cited

All-sky search for continuous gravitational waves from isolated neutron stars using Advanced LIGO O2 data

The LIGO Scientific Collaboration, the Virgo Collaboration, B. P. Abbott +1130

We present results of an all-sky search for continuous gravitational waves (CWs), which can be produced by fast-spinning neutron stars with an asymmetry around their rotation axis,…

gr-qc2019★ 46 cited

Physics of eccentric binary black hole mergers: A numerical relativity perspective

E. A. Huerta, Roland Haas, Sarah Habib +9

Gravitational wave observations of eccentric binary black hole mergers will provide unequivocal evidence for the formation of these systems through dynamical assembly in dense stel…

gr-qc2017★ 156 cited

Eccentric, nonspinning, inspiral, Gaussian-process merger approximant for the detection and characterization of eccentric binary black hole mergers

E. A. Huerta, C. J. Moore, Prayush Kumar +10

We present , a time domain, inspiral-merger-ringdown waveform model that describes non-spinning binary black holes systems that evolve on moderately eccentric orbi…