Numerical Black Hole Dynamics
Numerical, Theoretical, and Astrophysical Relativity (Physics)
This project, under the direction Astronomy of Larry L. Smarr, Department of and physics, is entitled: "Numerical. Theoretical, and Astrophysical Relativity (Physics)."
Gravitational Wave Extraction and Outer Boundary Conditions by Perturbative Matching
Physical Review Letters, 80, 1812 (1998).
Stable characteristic evolution of generic 3-dimensional single-black-hole spacetimes
Physical Review Letters, 80, 3915-3918 (1998).
Boosted three-dimensional black-hole evolutions with singularity excision
Physical Review Letters, 80, 2512-2516 (1998).
When Black Holes Collide
Proceedings of the Sixth Canadian Conference on General Relativity and Relativistic Astrophysics, Fields Institute Communications (1997).
Head-on Collisions of Two Black Holes
Computational Astrophysics; 12th Kingston Meeting on Theoretical Astrophysics; ASP Conference Series #123, edited by D. A. Clarke and M. J. West., p. 314 (1997).
Geometry of a Black Hole Collision – Science Magazine
Richard Matzner, Edward Seidel, Stuart L. Shapiro, Larry Smarr, Wai-Mo Suen, Saul Teukolsky, Jeff Winicuor, Science 270, 941. (1995).
The Head-On Collision Of Two Equal Mass Black Holes
Peter Anninos, David Hobill, Edward Seidel, Larry Smarr, and Wai-Mo Suen. Physical Review D15, 52, 2044. (1995).
Dynamics of Apparent and Event Horizons
P. Anninos, D. Bernstein, S. Brandt, J. Libson, Joan Masso, E. Seidel, L. Smarr, W.-M. Suen, and P. Walker. Physical Review Letters, 74, 630. (1995).
Oscillating Apparent Horizons In Numerically Generated Spacetimes
Peter Anninos, David Bernstein, Steve Brandt, David Hobill, Ed Seidel, Larry Smarr, Australian Journal of Physics, 48, 1027-43 (1995).
Dynamics of Black Hole Apparent Horizons
Peter Anninos, David Bernstein, Steven R. Brandt, David Hobill, Edward Seidel, and Larry Smarr,Physical Review D15, 50, 3801. (1994).
Numerically Generated Black Hole Spacetimes: Interaction with Gravitational Waves
A. Abrahams, D. Bernstein, D. Hobill, E. Seidel, and L. Smarr, Physical Review D15, 45, 3544, (1992).
Numerical Relativistic Gravitational Collapse with Spatial Time Slices
C.R. Evans, L.L. Smarr and J.R. Wilson, in Astrophysical Radiation Hydrodynamics, 481-519, ed. K.-H. Winkler and M. Norman (Reidel: Dordrecht) (1986).
Computational Relativity: Numerical And Algebraic Approaches
In The Proceedings of the 10th International Conference on General Relativity and Gravitation, 163-183, ed. B. Berotti et al. (Reidel: Dordrecht). (1984).
The Structure of General Relativity with a Numerical Illustration: The Collision of Two Black Holes
L. Smarr Ph.D. Dissertation, University of Texas at Austin (1975). Ph.D. Advisor Bryce S. DeWitt (Deceased).The Pre-History of the Two Black Hole Collision Problem
Invited Talk. History of Numerical Relativity Session. American Physical Society. Columbus, OH. April 15, 2018The First 50 Years of the Two Black Hole Collision Problem: 1935 to 1985
Invited Talk at the UCSB Institute of Theoretical Physics Miniprogram on Colliding Black Holes: Mathematical Issues in Numerical Relativity, Santa Barbara, CA January 10, 2000The Collision of Two Black Holes – NCSA Visualization
NCSA Visualization - Peter Anninos, David Hobill, Edward Seidel, Larry Smarr, Wai-Mo Suen, and Mark Bajuk.