Detecting fundamental fields with LISA observations of gravitational waves from extreme mass-ratio inspirals
Top Cited Papers
- 10 February 2022
- journal article
- letter
- Published by Springer Nature in Nature Astronomy
- Vol. 6 (4) , 464-470
Abstract
No abstract availableKeywords
All Related Versions
This publication has 61 references indexed in Scilit:
- Testing General Relativity with Low-Frequency, Space-Based Gravitational-Wave DetectorsLiving Reviews in Relativity, 2013
- Erratum: Evolution of circular, nonequatorial orbits of Kerr black holes due to gravitational-wave emission [Phys. Rev. D61, 084004 (2000)]Physical Review D, 2001
- Angular resolution of the LISA gravitational wave detectorPhysical Review D, 1998
- Measuring gravitational waves from binary black hole coalescences. II. The waves’ information and its extraction, with and without templatesPhysical Review D, 1998
- Dilatonic black holes in higher curvature string gravityPhysical Review D, 1996
- Gravitational waves from inspiraling compact binaries: Parameter estimation using second-post-Newtonian waveformsPhysical Review D, 1995
- Novel ‘‘no-scalar-hair’’ theorem for black holesPhysical Review D, 1995
- Spin-induced orbital precession and its modulation of the gravitational waveforms from merging binariesPhysical Review D, 1994
- Observable effects of a scalar gravitational field in a binary pulsarThe Astrophysical Journal, 1975
- Black holes in the Brans-DickeCommunications in Mathematical Physics, 1972