Zobrazeno 1 - 5
of 5
pro vyhledávání: '"Zeyuan Xuan"'
Publikováno v:
The Astrophysical Journal, Vol 965, Iss 2, p 148 (2024)
The dynamical formation channels of gravitational wave (GW) sources typically involve a stage when the compact object binary source interacts with the environment, which may excite its eccentricity, yielding efficient GW emission. For the wide eccent
Externí odkaz:
https://doaj.org/article/d1f3c83e12f84599ad1fa255c96262e2
Many gravitational wave (GW) sources in the LISA band are expected to have non-negligible eccentricity. Furthermore, many of them can undergo acceleration because they reside in the presence of a tertiary. Here we develop analytical and numerical met
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d8761f59403aa807e85805f3f62c10bb
http://arxiv.org/abs/2210.03129
http://arxiv.org/abs/2210.03129
Autor:
Xian Chen, A. J. K. Chua, Mara J. B. Rosell, Alejandro Torres-Orjuela, Pau Amaro Seoane, Zeyuan Xuan
Publikováno v:
Physical review letters 127(4), 041102 (2021). doi:10.1103/PhysRevLett.127.041102
Physical review letters 127(4), 041102 (2021). doi:10.1103/PhysRevLett.127.041102
Gravitational waves from a source moving relative to us can suffer from special-relativistic effects such as aberration. The required velocities for these to be si
Gravitational waves from a source moving relative to us can suffer from special-relativistic effects such as aberration. The required velocities for these to be si
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a6b078e9df5bbcaa18fe5dda9781b766
Publikováno v:
27th Chinese Control & Decision Conference (2015 CCDC); 2015, p5155-5159, 5p
Autor:
Torres-Orjuela, Alejandro1,2, Seoane, Pau Amaro2,3,4,5,6, Zeyuan Xuan7, Chua, Alvin J. K.8,9, Rosell, Mara J. B.10, Xian Chen1,2 xian.chen@pku.edu.cn
Publikováno v:
Physical Review Letters. 7/23/2021, Vol. 127 Issue 4, p1-1. 1p.