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Phenomenological model of gravitational self-force enhanced tides in inspiraling binary neutron stars (2024)

First Author: Williams N

Attributed to: Advanced LIGO Operations Support funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1103/physrevd.110.104013

Publication URI: http://dx.doi.org/10.1103/physrevd.110.104013

Type: Journal Article/Review

Parent Publication: Physical Review D

Issue: 10