activity
19942003
most citedFormation of Supermassive Black Holes: Simulations in General Relativity

4 citations · 4 across the 1 of their papers we have counts for

collaborators

7 papers

astro-ph20034 cited

Formation of Supermassive Black Holes: Simulations in General Relativity

Stuart L. Shapiro

There is compelling evidence that supermassive black holes exist. Yet the origin of these objects, or their seeds, is still unknown. We discuss several plausible scenarios for form…

astro-ph2002

Collapse of a Rotating Supermassive Star to a Supermassive Black Hole: Post-Newtonian Simulations

Motoyuki Saijo, Thomas W. Baumgarte, Stuart L. Shapiro +1

We study the gravitational collapse of a rotating supermassive star (SMS) by means of a (3+1) hydrodynamical simulation in a post-Newtonian (PN) approxi- mation of general relativi…

gr-qc2001

Dynamical Bar Instability in Relativistic Rotating Stars

Motoyuki Saijo, Masaru Shibata, Thomas W. Baumgarte +1

We study by computational means the dynamical stability against bar-mode deformation of rapidly and differentially rotating stars in a post-Newtonian approximation of general relat…

gr-qc1999

Brief Comments on ``The Shapiro Conjecture, Prompt or Delayed Collapse ?'' by Miller, Suen and Tobias

Stuart L. Shapiro

Recent numerical simulations address a conjecture by Shapiro that when two neutron stars collide head-on from rest at infinity, sufficient thermal pressure may be generated to supp…

gr-qc1998

Hot, Rotating Disks In General Relativity: Collisionless Equilibrium Models

A. Katrin Schenk, Stuart L. Shapiro, Saul A. Teukolsky

We present a method for constructing equilibrium disks with net angular momentum in general relativity. The method solves the relativistic Vlasov equation coupled to Einstein's equ…

gr-qc1997

Binary Neutron Stars in Quasi-Equilibrium Circular Orbit: A Fully Relativistic Treatment

Thomas W. Baumgarte, Stuart L. Shapiro, Gregory B. Cook +2

We present a numerical scheme that solves the initial value problem in full general relativity for a binary neutron star in quasi-equilibrium. While Newtonian gravity allows for a…