Post-1-Newtonian tidal effects in the gravitational waveform from binary inspirals
Abstract
The gravitational wave signal from an inspiralling binary neutron star system will contain detailed information about tidal coupling in the system, and thus, about the internal physics of the neutron stars. To extract this information will require highly accurate models for the gravitational waveform. We present here a calculation of the gravitational wave signal from a binary with quadrupolar tidal interactions which includes all post-1-Newtonian–order effects in both the conservative dynamics and wave generation. We consider stars with adiabatically induced quadrupoles moving in circular orbits, and work to linear order in the stars' quadrupole moments. We find that post-1-Newtonian corrections increase the tidal signal by approximately 20% at gravitational wave frequencies of 400 Hz.
Additional Information
© 2011 American Physical Society. Received 12 January 2011; published 28 April 2011. This research was supported at Cornell by NSF Grant No. PHY-0757735, and at Caltech by the Sherman Fairchild Foundation.Attached Files
Published - Vines2011p13891Phys_Rev_D.pdf
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Additional details
- Eprint ID
- 23790
- Resolver ID
- CaltechAUTHORS:20110525-091559488
- PHY-0757735
- NSF
- Sherman Fairchild Foundation
- Created
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2011-06-20Created from EPrint's datestamp field
- Updated
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2021-11-09Created from EPrint's last_modified field