A Comparison of search templates for gravitational waves from binary inspiral
By T. Damour, B. Iyer, B. Sathyaprakash. 2001
188 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Oceanography
View Paper: https://www.semanticscholar.org/paper/e91935354fa1ea144f46e33a33c9b573cb1c9290
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In Astronomy and Astrophysics
- Hans-Thomas Janka
- Andreas Marek
- Bernhard Müller
- Bernard F. Schutz
- Adam Burrows
- R. Oechslin
- K. Kotake
- B. Sathyaprakash
In Oceanography
Citations in the corpus
- Physics, Astrophysics and Cosmology with Gravitational Waves (2009, methodology): “The foregoing evolution equations for the orbital phase can be solved in several equivalent ways [134], each correct to the required post-Newtonian order, but numerically different from one another.”
- Relativistic neutron star merger simulations with non-zero temperature equations of state. I. Variation of binary parameters and equation of state (2006, methodology): “Thisin- Send offprint requests to: R. Oechslin spiral phase lasts millions of years and can be very accurately modelled in the post-Newtonian framework (e.g. Damour et al. 2001, 2002).”