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Gravity in binary systems at the fifth and sixth post-Newtonian order

Autor: Blümlein, J., Maier, A., Marquard, P., Schäfer, G.

Publikováno v: Proceedings of Science / International School for Advanced Studies (LL2022), 012 (2022). doi:10.3204/PUBDB-2022-04146
Loops and Legs in Quantum Field Theory, LL2022, Ettal, Germany, 2022-04-25-2022-04-30

Binary sources of gravitational waves in the early inspiral phase are accurately described by a post-Newtonian expansion in small velocity and weak interaction. We compute the conservative dynamics to fifth and partial sixth order using a non-relativ

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e040c387a4f9e361671b312a9f6dc7ac

Gravitational radiation from inspiralling compact objects: Spin effects to the fourth post-Newtonian order

Autor: Porto Pereira, Rafael Alejandro, Yang, Zixin, Cho, Gihyuk

Publikováno v: Physical review / D 106(10), L101501 (2022). doi:10.1103/PhysRevD.106.L101501

Physical review / D 106(10), L101501 (2022). doi:10.1103/PhysRevD.106.L101501
The linear- and quadratic-in-spin contributions to the binding potential and gravitational-wave flux from binary systems are derived to next-to-next-to-leading order i

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e45ef5cdf1d6e377151713dc2f3250eb

Action-angle variables of a binary black-hole with arbitrary eccentricity, spins, and masses at 1.5 post-Newtonian order

Autor: Sashwat Tanay, Leo C. Stein, Gihyuk Cho

Publikováno v: INSPIRE-HEP

Accurate and efficient modeling of the dynamics of binary black holes (BBHs) is crucial to their detection through gravitational waves (GWs), with LIGO/Virgo/KAGRA, and LISA in the future. Solving the dynamics of a BBH system with arbitrary parameter

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2b458f897ff736dd58aa110626690360
https://bib-pubdb1.desy.de/record/474335

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