TY - JOUR
AU - Amalberti, Loris
AU - Yang, Zixin
AU - Porto Pereira, Rafael Alejandro
TI - Gravitational radiation from inspiralling compact binaries to N3LO in the effective field theory approach
JO - Physical review / D
VL - 110
IS - 4
SN - 2470-0010
CY - Ridge, NY
PB - American Physical Society
M1 - PUBDB-2024-05728
M1 - arXiv:2406.03457
M1 - DESY-24-084
SP - 044046
PY - 2024
N1 - 18 pages, 9 figures, 1 computer-readable ancillary file. v2: typos corrected, ancillary file updated, published version preprint:607514
AB - Within the context of the effective field theory (EFT) framework to gravitational dynamics, we compute the Hamiltonian, source quadrupole moment, and gravitational-wave energy flux for (nonspinning) inspiralling compact binaries at next-to-next-to-next-to leading order (N3LO) in the post-Newtonian (PN) expansion. We use the recently developed d-dimensional multipole-expanded effective theory, and explicitly perform the matching to the (pseudo) stress-energy tensor. The calculation involves Feynman integrals up to three- (conservative) and two-loop (radiative) orders, evaluated within dimensional regularization. Our (ambiguity-free) results confirm (for the first time) the value of the gravitational-wave flux for quasicircular orbits at 3PN order, while paving the way forward to the inclusion of spin effects as well as higher-order computations.
KW - binary: compact (INSPIRE)
KW - tensor: energy-momentum (INSPIRE)
KW - gravitational radiation: energy (INSPIRE)
KW - energy: flux (INSPIRE)
KW - regularization: dimensional (INSPIRE)
KW - spin: effect (INSPIRE)
KW - gravitational radiation: flux (INSPIRE)
KW - higher-order: 2 (INSPIRE)
KW - effective field theory (INSPIRE)
KW - gravitation (INSPIRE)
KW - Hamiltonian (INSPIRE)
KW - Feynman graph (INSPIRE)
KW - orbit: circle (INSPIRE)
KW - moment: multipole (INSPIRE)
KW - conservation law (INSPIRE)
KW - binary: coalescence (INSPIRE)
KW - asymptotic expansion (INSPIRE)
KW - expansion: multipole (INSPIRE)
KW - expansion: higher-order (INSPIRE)
KW - any-dimensional (INSPIRE)
KW - loop integral (INSPIRE)
LB - PUB:(DE-HGF)16
UR - <Go to ISI:>//WOS:001301034700013
DO - DOI:10.1103/PhysRevD.110.044046
UR - https://bib-pubdb1.desy.de/record/614027
ER -