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/10.1103/physrevd.101.103008
Publication URI: http://dx.doi.org/10.1103/physrevd.101.103008
Type: Journal Article/Review
Parent Publication: Physical Review D
Issue: 10