Zobrazeno 1 - 5
of 5
pro vyhledávání: '"Sashwat Tanay"'
Publikováno v:
Phys. Rev. D
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
https://bib-pubdb1.desy.de/record/474335
Accurate and efficient modeling of the dynamics of binary black holes (BBHs) is crucial to their detection and parameter estimation through gravitational waves, both with LIGO/Virgo and LISA. General BBH configurations will have misaligned spins and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::dd4fbe9852fe5d7c21a0eaa0832e9a54
Publikováno v:
Phys.Rev.D
Phys.Rev.D, 2019, 100 (6), pp.064006. ⟨10.1103/PhysRevD.100.064006⟩
Physical Review D
Physical Review D, American Physical Society, 2019, 100 (6), pp.064006. ⟨10.1103/PhysRevD.100.064006⟩
Phys.Rev.D, 2019, 100 (6), pp.064006. ⟨10.1103/PhysRevD.100.064006⟩
Physical Review D
Physical Review D, American Physical Society, 2019, 100 (6), pp.064006. ⟨10.1103/PhysRevD.100.064006⟩
The space-based detector LISA may observe gravitational waves from the early inspiral of stellar-mass black hole binaries, some of which could have significant eccentricity. Current gravitational waveform templates are only valid for small orbital ve
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0c61d9e5c463657150ba327954ec7a77
http://arxiv.org/abs/1905.08811
http://arxiv.org/abs/1905.08811
Publikováno v:
Physical review / D 105(6), 064010 (2022). doi:10.1103/PhysRevD.105.064010
Physical review / D 105(6), 064010 (2022). doi:10.1103/PhysRevD.105.064010
We derive fourth post-Newtonian (4PN) contributions to the Keplerian type parametric solution associated with the conservative dynamics of eccentric, nonspinning compact
We derive fourth post-Newtonian (4PN) contributions to the Keplerian type parametric solution associated with the conservative dynamics of eccentric, nonspinning compact