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New gravitational waveform model for precessing binary neutron stars with double-spin effects (2025)

First Author: Colleoni M

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.111.064025

Publication URI: http://dx.doi.org/10.1103/physrevd.111.064025

Type: Journal Article/Review

Parent Publication: Physical Review D

Issue: 6