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/10.48550/arxiv.2203.00623
Publication URI: https://arxiv.org/abs/2203.00623
Type: Other