Arun, K. G., Iyer, B. R., Qusailah, M. S. S. and Sathyaprakash, Bangalore Suryanarayana ![]() |
Official URL: http://dx.doi.org/10.1088/0264-9381/23/9/L01
Abstract
The Laser Interferometric Space Antenna (LISA) will observe supermassive black hole binary mergers with an amplitude signal-to-noise ratio of several thousand. We investigate the extent to which such observations afford high-precision tests of Einstein's gravity. We show that LISA provides a unique opportunity to probe the nonlinear structure of post-Newtonian theory both in the context of general relativity and its alternatives.
Item Type: | Article |
---|---|
Date Type: | Publication |
Status: | Published |
Schools: | Physics and Astronomy |
Subjects: | Q Science > QB Astronomy |
Publisher: | IOP Publishing |
ISSN: | 0264-9381 |
Last Modified: | 24 Oct 2022 10:40 |
URI: | https://orca.cardiff.ac.uk/id/eprint/45357 |
Citation Data
Cited 105 times in Scopus. View in Scopus. Powered By Scopus® Data
Actions (repository staff only)
![]() |
Edit Item |