output
20022026
most citedAdvanced capabilities for materials modelling with Quantum ESPRESSO

7.7k citations

Showing 2014 · gr-qcShow all

10 papers · 2 filters

gr-qc2014111 cited

Improved methods for simulating nearly extremal binary black holes

Mark A. Scheel, Matthew Giesler, Daniel A. Hemberger +5

Astrophysical black holes could be nearly extremal (that is, rotating nearly as fast as possible); therefore, nearly extremal black holes could be among the binaries that current a…

gr-qc201450 cited

Nearly extremal apparent horizons in simulations of merging black holes

Geoffrey Lovelace, Mark A. Scheel, Robert Owen +9

The spin angular momentum of an isolated Kerr black hole is bounded by the surface area of its apparent horizon: , with equality for extremal black holes. In thi…

gr-qc2014108 cited

What does a binary black hole merger look like?

Andy Bohn, William Throwe, François Hébert +4

We present a method of calculating the strong-field gravitational lensing caused by many analytic and numerical spacetimes. We use this procedure to calculate the distortion caused…

gr-qc2014180 cited

The Kerr Metric

Saul A. Teukolsky

This review describes the events leading up to the discovery of the Kerr metric in 1963 and the enormous impact the discovery has had in the subsequent 50 years. The review discuss…

gr-qc201460 cited

Rapidly rotating black holes in dynamical Chern-Simons gravity: Decoupling limit solutions and breakdown

Leo C. Stein

Rapidly rotating black holes are a prime arena for understanding corrections to Einstein's theory of general relativity (GR). We construct solutions for rapidly rotating black hole…

gr-qc201436 cited

Geodesic deviation at higher orders via covariant bitensors

Justin Vines

We review a simple but instructive application of the formalism of covariant bitensors, to use a deviation vector field along a fiducial geodesic to describe a neighboring worldlin…