Are Post-Newtonian templates faithful and effectual in detecting gravitational signals from neutron star binaries?
arXiv:gr-qc/0208011 · doi:10.1103/PhysRevD.66.064013
Abstract
We compute the overlap function between Post-Newtonian (PN) templates and gravitational signals emitted by binary systems composed of one neutron star and one point mass, obtained by a perturbative approach. The calculations are performed for different stellar models and for different detectors, to estimate how effectual and faithful the PN templates are, and to establish whether effects related to the internal structure of neutron stars may possibly be extracted by the matched filtering technique.
arXiv comment14 pages, 3 figures, accepted for publication in Phys. Rev. D
References in corpus (15)
- Neutron Star Structure and the Equation of State
- Gravitational Waves from Mergin Compact Binaries: How Accurately Can One Extract the Binary's Parameters from the Inspiral Waveform?
- A Comprehensive Study of Binary Compact Objects as Gravitational Wave Sources: Evolutionary Channels, Rates, and Physical Properties
- Towards gravitational-wave asteroseismology
- Improved filters for gravitational waves from inspiralling compact binaries
- A Comparison of search templates for gravitational waves from binary inspiral
- Gravitational Radiation from Post-Newtonian Sources and Inspiralling Compact Binaries
- Gravitational Wave Astronomy: in Anticipation of First Sources to be Detected
- Resonant Tidal Excitations of Rotating Neutron Stars in Coalescing Binaries
- Gravitational Waves by a Particle in Circular Orbits around a Schwarzschild black hole -5.5 Post-Newtonian Formula-
- Energy and angular momentum flow into a black hole in a binary
- Prospects for gravitational-wave observations of neutron-star tidal disruption in neutron-star/black-hole binaries
- Gravitational signals emitted by a point mass orbiting a neutron star: effects of stellar structure
- Gravitational signals emitted by a point mass orbiting a neutron star: a perturbative approach
- Mother templates for gravitational wave chirps
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