Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- California Institute of TechnologyUS2.6k papers
- Centre National de la Recherche ScientifiqueFR2k papers
- Massachusetts Institute of TechnologyUS1.9k papers
- University of FloridaUS1.8k papers
- Carnegie Mellon UniversityUS1.7k papers
- Princeton UniversityUS1.7k papers
- University of RochesterUS1.7k papers
- Purdue University West LafayetteUS1.6k papers
- Johns Hopkins UniversityUS1.6k papers
- University of Maryland, College ParkUS1.6k papers
- The Ohio State UniversityUS1.6k papers
- University of California, Santa BarbaraUS1.6k papers
6 papers · 2 filters
Collapse to Black Holes in Brans-Dicke Theory: II. Comparison with General Relativity
Mark A. Scheel, Stuart L. Shapiro, Saul A. Teukolsky
We discuss a number of long-standing theoretical questions about collapse to black holes in the Brans-Dicke theory of gravitation. Using a new numerical code, we show that Oppenhei…
Collapse to Black Holes in Brans-Dicke Theory: I. Horizon Boundary Conditions for Dynamical Spacetimes
Mark A. Scheel, Stuart L. Shapiro, Saul A. Teukolsky
We present a new numerical code that evolves a spherically symmetric configuration of collisionless matter in the Brans-Dicke theory of gravitation. In this theory the spacetime is…
Calculation of gravitational wave forms from black hole collisions and disk collapse: Applying perturbation theory to numerical spacetimes
Andrew M. Abrahams, Stuart L. Shapiro, Saul A. Teukolsky
Many simulations of gravitational collapse to black holes become inaccurate before the total emitted gravitational radiation can be determined. The main difficulty is that a signif…
Collisions of boosted black holes: perturbation theory prediction of gravitational radiation
Andrew M. Abrahams, Gregory B. Cook
We consider general relativistic Cauchy data representing two nonspinning, equal-mass black holes boosted toward each other. When the black holes are close enough to each other and…
Disk collapse in general relativity
Andrew M. Abrahams, Stuart L. Shapiro, Saul A. Teukolsky
The radial collapse of a homogeneous disk of collisionless particles can be solved analytically in Newtonian gravitation. To solve the problem in general relativity, however, requi…
Three-dimensional initial data for the collision of two black holes II: Quasi-circular orbits for equal-mass black holes
Gregory B. Cook
The construction of initial-data sets representing binary black-hole configurations in quasi-circular orbits is studied in the context of the conformal-imaging formalism. An effect…