This is the writeup of the talk I gave at the Yukawa International Symposium at Kyoto, Japan on June 29, 1999. The talk summarizes the present status of the close limit approximation for colliding black holes
The computation of gravitational radiation generated by the coalescence of inspiralling binary black...
There exists an upper limit on the mass of black holes when the cosmological constant Λ is positive....
We present the first results in a new program intended to make the best use of all available technol...
We calculate an estimate of the gravitational radiation emitted when two equal mass black holes coal...
We calculate an estimate of the gravitational radiation emitted when two equal mass black holes coal...
We study the head-on collision of two equal-mass momentarily stationary black holes, using black hol...
The computation of gravitational radiation generated by the coalescence of inspiralling binary black...
Using approximate techniques we study the final moments of the collision of two (individually non-sp...
International audienceThe ringdown phase of a black hole formed from the merger of two orbiting blac...
We study the radiation from a collision of black holes with equal and opposite linear momenta. Resul...
We study the head-on collision of two equal-mass momentarily stationary black holes, using black hol...
Abstract. The ringdown phase of a black hole formed from the merger of two orbiting black holes is d...
We develop a close-limit approximation to the head-on collision of two neutron stars similar to that...
The ability to model the evolution of compact binaries from the inspiral to coalescence is central t...
The computation of gravitational radiation generated by the coalescence of inspiralling binary black...
The computation of gravitational radiation generated by the coalescence of inspiralling binary black...
There exists an upper limit on the mass of black holes when the cosmological constant Λ is positive....
We present the first results in a new program intended to make the best use of all available technol...
We calculate an estimate of the gravitational radiation emitted when two equal mass black holes coal...
We calculate an estimate of the gravitational radiation emitted when two equal mass black holes coal...
We study the head-on collision of two equal-mass momentarily stationary black holes, using black hol...
The computation of gravitational radiation generated by the coalescence of inspiralling binary black...
Using approximate techniques we study the final moments of the collision of two (individually non-sp...
International audienceThe ringdown phase of a black hole formed from the merger of two orbiting blac...
We study the radiation from a collision of black holes with equal and opposite linear momenta. Resul...
We study the head-on collision of two equal-mass momentarily stationary black holes, using black hol...
Abstract. The ringdown phase of a black hole formed from the merger of two orbiting black holes is d...
We develop a close-limit approximation to the head-on collision of two neutron stars similar to that...
The ability to model the evolution of compact binaries from the inspiral to coalescence is central t...
The computation of gravitational radiation generated by the coalescence of inspiralling binary black...
The computation of gravitational radiation generated by the coalescence of inspiralling binary black...
There exists an upper limit on the mass of black holes when the cosmological constant Λ is positive....
We present the first results in a new program intended to make the best use of all available technol...