Modified gravitational wave propagation and the binary neutron star mass function
1. June 2022
A.Finke, S. Foffa, F. Iacovelli, M. Maggiore, M. Mancarella, Phys.Dark Univ. 36 (2022) 100994, arXiv: 2108.04065 [gr-qc]
We show how the narrowness of the mass distribution of binary neutron stars can be used to constrain deviations from general relativity at cosmological scales with the observations of gravitational waves from coalescing binary neutron stars, even in absence of a direct redshift measurement.