Ed Seidel

Spectral Methods for Numerical Relativity

The Confrontation between General Relativity and Experiment

Gravitational Radiation from Post-Newtonian Sources and Inspiralling Compact Binaries

Gravitational-Wave Emission from Rotating Gravitational Collapse in Three Dimensions

Testing General Relativity with the Shadow Size of SgrA*

Challenging the Paradigm of Singularity Excision in Gravitational Collapse

Isolated and Dynamical Horizons and Their Applications

Visualizing spacetime curvature via frame-drag vortexes and tidal tendexes. II. Stationary black holes

Merger of binary neutron stars to a black hole: Disk mass, short gamma-ray bursts, and quasinormal mode ringing

Visualizing spacetime curvature via frame-drag vortexes and tidal tendexes. III. Quasinormal pulsations of Schwarzschild and Kerr black holes

Faithful effective-one-body waveforms of small-mass-ratio coalescing black hole binaries

Accurate evolutions of inspiralling neutron-star binaries: Prompt and delayed collapse to a black hole

Dynamical horizons and their properties

Template bank for gravitational waveforms from coalescing binary black holes: Nonspinning binaries

Evolving black hole-neutron star binaries in general relativity using pseudospectral and finite difference methods

Testing SgrA^*with the spectrum of its accretion structure

Merger of binary neutron stars with realistic equations of state in full general relativity

Introduction to dynamical horizons in numerical relativity

Momentum flow in black-hole binaries. I. Post-Newtonian analysis of the inspiral and spin-induced bobbing

Gravitational radiation from collapsing magnetized dust

Quasinormal modes of black holes and black branes

Dynamical evolution of quasicircular binary black hole data

Are moving punctures equivalent to moving black holes?

Oscillating Apparent Horizons in Numerically Generated Spacetimes

Three-dimensional relativistic simulations of rotating neutron-star collapse to a Kerr black hole