Distinguishing high-mass binary neutron stars from binary black holes with second- and third-generation gravitational wave observatories (2020)
Attributed to:
Unveiling the Structure of the Universe
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.2001.11470
Publication URI: https://arxiv.org/abs/2001.11470
Type: Other