70 citations · 259 across the 7 of their papers we have counts for
7 papers
The SXS Collaboration's third catalog of binary black hole simulations
Mark A. Scheel, Michael Boyle, Keefe Mitman +56
We present a major update to the Simulating eXtreme Spacetimes (SXS) Collaboration's catalog of binary black hole simulations. Using highly efficient spectral methods implemented i…
Extending black-hole remnant surrogate models to extreme mass ratios
Matteo Boschini, Davide Gerosa, Vijay Varma +19
Numerical-relativity surrogate models for both black-hole merger waveforms and remnants have emerged as important tools in gravitational-wave astronomy. While producing very accura…
Simulating magnetized neutron stars with discontinuous Galerkin methods
Nils Deppe, François Hébert, Lawrence E. Kidder +33
Discontinuous Galerkin methods are popular because they can achieve high order where the solution is smooth, because they can capture shocks while needing only nearest-neighbor com…
On the Possibility of Non-Geodesic Motion of the Massless Spinning Top
Cristóbal Armaza, Sergio A. Hojman, Benjamin Koch +1
The motion of spinning massless particles in gravitationally curved backgrounds is revisited by considering new types of constraints. Those constraints guarantee zero mass ($P_μP^μ…
Can Schwarzschild Black Holes Be Accelerators of Spinning Massive Particles?
Cristóbal Armaza, Máximo Bañados, Benjamin Koch
It is known that the center-of-mass energy of the collision of two massive particles following geodesics around a black hole presents a maximum. The maximum energy increases when t…
On magnetic equilibria in barotropic stars
C. Armaza, A. Reisenegger, J. A. Valdivia
Upper main sequence stars, white dwarfs and neutron stars are known to possess stable, large-scale magnetic fields. Numerical works have confirmed that stable MHD equilibria can ex…
Hall equilibria with toroidal and poloidal fields: application to neutron stars
K. N. Gourgouliatos, A. Cumming, A. Reisenegger +3
We present solutions for Hall equilibria applicable to neutron star crusts. Such magnetic configurations satisfy a Grad-Shafranov-type equation, which is solved analytically and nu…