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20102026
most citedElectromagnetic Counterparts of Compact Object Mergers Powered by the Radioactive Decay of R-process Nuclei

1.2k citations · 1.5k across the 18 of their papers we have counts for

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7 papers · 1 filter

astro-ph.HE2021★ 45 cited

Estimating outflow masses and velocities in merger simulations: impact of r-process heating and neutrino cooling

Francois Foucart, Philipp Moesta, Teresita Ramirez +3

The determination of the mass, composition, and geometry of matter outflows in black hole-neutron star and neutron star-neutron star binaries is crucial to current efforts to model…

astro-ph.HE2021★ 24 cited

Electromagnetic Signatures from the Tidal Tail of a Black Hole - Neutron Star Merger

Siva Darbha, Daniel Kasen, Francois Foucart +1

Black hole - neutron star (BH-NS) mergers are a major target for ground-based gravitational wave (GW) observatories. A merger can also produce an electromagnetic counterpart (a kil…

astro-ph.HE2020★ 58 cited

Inclination Dependence of Kilonova Light Curves from Globally Aspherical Geometries

Siva Darbha, Daniel Kasen

The merger of two neutron stars (NSs) or a neutron star and a black hole (BH) produces a radioactively-powered transient known as a kilonova, first observed accompanying the gravit…

astro-ph.HE2019★ 16 cited

Ultra-deep tidal disruption events: prompt self-intersections and observables

Siva Darbha, Eric R. Coughlin, Daniel Kasen +1

A star approaching a supermassive black hole (SMBH) can be torn apart in a tidal disruption event (TDE). We examine ultra-deep TDEs, a new regime in which the disrupted debris appr…

astro-ph.HE2018★ 18 cited

Gravitational interactions of stars with supermassive black hole binaries. I. Tidal disruption events

Siva Darbha, Eric R. Coughlin, Daniel Kasen +1

Stars approaching supermassive black holes (SMBHs) in the centers of galaxies can be torn apart by strong tidal forces. We study the physics of tidal disruption by a binary SMBH as…

astro-ph.HE2010★ 77 cited

Nickel-Rich Outflows Produced by the Accretion-Induced Collapse of White Dwarfs: Lightcurves and Spectra

S. Darbha, B. D. Metzger, E. Quataert +3

The accretion-induced collapse (AIC) of a white dwarf to form a neutron star can leave behind a rotationally supported disk with mass of up to ~ 0.1 M_sun. The disk is initially co…

astro-ph.HE2010★ 1.2k cited

Electromagnetic Counterparts of Compact Object Mergers Powered by the Radioactive Decay of R-process Nuclei

B. D. Metzger, G. Martinez-Pinedo, S. Darbha +7

The most promising astrophysical sources of kHz gravitational waves (GWs) are the inspiral and merger of binary neutron star(NS)/black hole systems. Maximizing the scientific retur…