25 citations · 83 across the 14 of their papers we have counts for
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Toward 2D Dynamo Models Calibrated by Global 3D Relativistic Accretion Disk Simulations
Matthew D. Duez, Courtney L. Cadenhead, Zachariah B. Etienne +2
Two-dimensional models assuming axisymmetry are an economical way to explore the long-term evolution of black hole accretion disks, but they are only realistic if the feedback of t…
The Dynamics of Debris Disk Creation in Neutron Star Mergers
Yossef Zenati, Julian Krolik, Leonardo Werneck +4
The detection of GW170817/AT2017gfo inaugurated an era of multimessenger astrophysics, in which gravitational wave and multiwavelength photon observations complement one another to…
Bound Debris Expulsion from Neutron Star Merger Remnants
Yossef Zenati, Julian H. Krolik, Leonardo R. Werneck +4
Many studies have found that neutron star mergers leave a fraction of the stars' mass in bound orbits surrounding the resulting massive neutron star or black hole. This mass is a s…
Handing off the outcome of binary neutron star mergers for accurate and long-term post-merger simulations
Federico G. Lopez Armengol, Zachariah B. Etienne, Scott C. Noble +20
We perform binary neutron star (BNS) merger simulations in full dynamical general relativity with IllinoisGRMHD, on a Cartesian grid with adaptive-mesh refinement. After the remnan…
HARM3D+NUC: A new method for simulating the post-merger phase of binary neutron star mergers with GRMHD, tabulated EOS and neutrino leakage
Ariadna Murguia-Berthier, Scott C. Noble, Luke F. Roberts +25
The first binary neutron star merger has already been detected in gravitational waves. The signal was accompanied by an electromagnetic counterpart including a kilonova component p…