Maselli, Andrea, Gualtieri, Leonardo, Ferrari, Valeria and Pannarale Greco, Francesco ![]() |
Official URL: http://dx.doi.org/10.1142/9789814623995_0052
Abstract
We use the post-Newtonian-Affine model to assess the validity of the adiabatic approximation in modeling tidal effects in the phase evolution of compact binary systems. We compute the dynamical evolution of the tidal tensor, which we estimate at the 2PN order, and of the quadrupole tensor, finding that their ratio, i.e. the tidal deformability, increases in the last phases of the inspiral. We derive the gravitational wave phase corrections due to this phenomenon and quantify how they affect gravitational wave detectability.
Item Type: | Conference or Workshop Item (Paper) |
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Date Type: | Publication |
Status: | Published |
Schools: | Physics and Astronomy |
Subjects: | Q Science > QC Physics |
Publisher: | World Scientific |
Last Modified: | 28 Oct 2022 10:38 |
URI: | https://orca.cardiff.ac.uk/id/eprint/79114 |
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