Erratum: Constraints on Einstein-dilation-Gauss-Bonnet gravity from black hole-neutron star gravitational wave events [Phys. Rev. D <b>105</b>, 064001 (2022)]
Zhenwei Lyu, Nan Jiang, Kent Yagi
Abstract
The correct version of Eqs. A(8, 10-12), which are coefficients of 0PN, 1PN, 1.5PN, and 2PN corrections should be as below. Note that the corrections only occur for s 1 s 2 terms; thus, the calculations and figures given in the paper are not affected. This is because when we study the black hole-neutron star system, these s 1 s 2 terms will vanish due to neutron star's scalar charge reducing to zero.
Topics & Concepts
PhysicsNeutron starEinsteinGravitational waveBlack hole (networking)AstrophysicsEinstein TelescopeStellar black holeMathematical physicsClassical mechanicsComputer scienceComputer networkRouting protocolLink-state routing protocolRouting (electronic design automation)GalaxyPulsars and Gravitational Waves ResearchRelativity and Gravitational TheoryCosmology and Gravitation Theories