Add to ORKGAbstract. Coalescing compact binaries with neutron star or black hole components provide the most promising sources of gravitational radiation for detection by the LIGO/VIRGO/GEO/TAMA laser interferometers now under construction. This fact has motivated several different theoretical studies of the inspiral and hydrodynamic merging of compact binaries. Analytic analyses of the inspiral waveforms have been performed in the post-Newtonian approximation. Analytic and numerical treatments of the coalescence waveforms from binary neutron stars have been performed using Newtonian hydrodynamics and the quadrupole radiation approximation. Numerical simulations of coalescing black hole and neutron star binaries are also underway in full general relat...
We develop a close-limit approximation to the head-on collision of two neutron stars similar to that...
After the first direct observations of gravitational waves generated by the coalescence of binary bl...
Emission of strong gravitational waves is expected in the last three milliseconds of coales-cence of...
Angular momentum loss via the emission of gravitational waves must eventually drive compact binaries...
Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Physics, 2001.Includes bibliographi...
We review the current status of general relativistic studies for the coalescence of black hole– neut...
The inspiral and merger of binary neutron stars (BNS) is one of the most promising potential sources...
Abstract. Using our Post-Newtonian SPH (smoothed particle hydrodynamics) code, we study the final co...
We present the first results from our Post-Newtonian (PN) Smoothed Particle Hydrodynamics (SPH) code...
Gravitational waves emitted from the coalescence of neutron star binaries open a new window to probe...
This paper reviews the current understanding of double neutron star and neutron star black hole bina...
Abstract: Gravitational waves (GWs) are one of the key predictions of Einstein’s theory of gen-eral ...
We have performed numerical simulations of coalescence of binary neutron stars using a Newtonian hyd...
We develop a semianalytical approach, based on the post-Newtonian expansion and on the affine approx...
On September 14th, 2015 the Laser Interferometer Gravitational-Wave Observatory (LIGO) detected grav...
We develop a close-limit approximation to the head-on collision of two neutron stars similar to that...
After the first direct observations of gravitational waves generated by the coalescence of binary bl...
Emission of strong gravitational waves is expected in the last three milliseconds of coales-cence of...
Angular momentum loss via the emission of gravitational waves must eventually drive compact binaries...
Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Physics, 2001.Includes bibliographi...
We review the current status of general relativistic studies for the coalescence of black hole– neut...
The inspiral and merger of binary neutron stars (BNS) is one of the most promising potential sources...
Abstract. Using our Post-Newtonian SPH (smoothed particle hydrodynamics) code, we study the final co...
We present the first results from our Post-Newtonian (PN) Smoothed Particle Hydrodynamics (SPH) code...
Gravitational waves emitted from the coalescence of neutron star binaries open a new window to probe...
This paper reviews the current understanding of double neutron star and neutron star black hole bina...
Abstract: Gravitational waves (GWs) are one of the key predictions of Einstein’s theory of gen-eral ...
We have performed numerical simulations of coalescence of binary neutron stars using a Newtonian hyd...
We develop a semianalytical approach, based on the post-Newtonian expansion and on the affine approx...
On September 14th, 2015 the Laser Interferometer Gravitational-Wave Observatory (LIGO) detected grav...
We develop a close-limit approximation to the head-on collision of two neutron stars similar to that...
After the first direct observations of gravitational waves generated by the coalescence of binary bl...
Emission of strong gravitational waves is expected in the last three milliseconds of coales-cence of...