Prospects for distinguishing dynamical tides in inspiralling binary neutron stars with third generation gravitational-wave detectors (2022)
Attributed to:
Gravitational wave science at the University of Birmingham
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1103/physrevd.105.123032
Publication URI: http://dx.doi.org/10.1103/physrevd.105.123032
Type: Journal Article/Review
Parent Publication: Physical Review D
Issue: 12