Zobrazeno 1 - 10
of 19
pro vyhledávání: '"Laura Sberna"'
Autor:
Lorenzo Speri, Andrea Antonelli, Laura Sberna, Stanislav Babak, Enrico Barausse, Jonathan R. Gair, Michael L. Katz
Publikováno v:
Physical Review X, Vol 13, Iss 2, p 021035 (2023)
Gravitational-wave observations of extreme mass ratio inspirals (EMRIs) offer the opportunity to probe the environments of active galactic nuclei (AGN) through the torques that accretion disks induce on the binary. Within a Bayesian framework, we stu
Externí odkaz:
https://doaj.org/article/6cd45c4f3f19412c8bfc236a205fefc4
Publikováno v:
Physical Review D
We introduce a bilinear form for Weyl scalar perturbations of Kerr. The formis symmetric and conserved, and we show that, when combined with a suitablerenormalization prescription involving complex r integration contours,quasinormal modes are orthogo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::222aae829875601a20e94b331c602f14
https://hdl.handle.net/21.11116/0000-000B-662A-421.11116/0000-000B-662C-221.11116/0000-000C-F2CE-B
https://hdl.handle.net/21.11116/0000-000B-662A-421.11116/0000-000B-662C-221.11116/0000-000C-F2CE-B
Publikováno v:
Physical Review
Physical Review D
Physical Review D
Black-hole superradiance has been used to place very strong bounds on a variety of models of ultralight bosons such as axions, new light scalars, and dark photons. It is common lore to believe that superradiance bounds are broadly model independent a
Autor:
Riccardo Barbieri, Stefano Savastano, Lorenzo Speri, Andrea Antonelli, Laura Sberna, Ollie Burke, Jonathan Gair, Nicola Tamanini
Publikováno v:
Physical Review D
Spaceborne gravitational-wave (GW) detectors observing at milli-Hz and deci-Hz frequencies are expected to detect large numbers of quasi-monochromatic signals. The first and second time-derivative of the GW frequency ($\dot f_0$ and $\ddot f_0$) can
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3759fd5ffc2cab6dd256497b5228f32e
http://arxiv.org/abs/2207.10674
http://arxiv.org/abs/2207.10674
Publikováno v:
Physical Review D
Physical Review D, 105(6):064046. American Institute of Physics
Physical Review D, 105(6):064046. American Institute of Physics
Gravitational-wave observations of black hole ringdowns are commonly used to characterize binary merger remnants and to test general relativity. These analyses assume linear black hole perturbation theory, in particular that the ringdown can be descr
Autor:
Andrés Castillo, Jorge Martin-Camalich, Jorge Terol-Calvo, Diego Blas, Andrea Caputo, Ricardo Tanausú Génova Santos, Laura Sberna, Michael Peel, Jose Alberto Rubiño-Martín
Publikováno v:
Journal of Cosmology and Astroparticle Physics
The polarization of photons emitted by astrophysical sources might be altered as they travel through a dark matter medium composed of ultra light axion-like particles (ALPs). In particular, the coherent oscillations of the ALP background in the galac
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::96033a6bd330567d9b1b82b215335589
http://arxiv.org/abs/2201.03422
http://arxiv.org/abs/2201.03422
Autor:
Laura Sberna, Stanislav Babak, Sylvain Marsat, Andrea Caputo, Giulia Cusin, Alexandre Toubiana, Enrico Barausse, Chiara Caprini, Tito Dal Canton, Alberto Sesana, Nicola Tamanini
Publikováno v:
Phys.Rev.D
Phys.Rev.D, 2022, 106 (6), pp.064056. ⟨10.1103/PhysRevD.106.064056⟩
Physical Review D
Phys.Rev.D, 2022, 106 (6), pp.064056. ⟨10.1103/PhysRevD.106.064056⟩
Physical Review D
Binaries of relatively massive black holes like GW190521 have been proposed to form in dense gas environments, such as the disks of Active Galactic Nuclei (AGNs), and they might be associated with transient electromagnetic counterparts. The interacti
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a2ee88d4d9fd2103b92159558b6b6c24
https://hal.science/hal-03681626
https://hal.science/hal-03681626
Publikováno v:
The Astrophysical Journal
The Astrophysical Journal, American Astronomical Society, 2021, 908 (1), pp.1. ⟨10.3847/1538-4357/abccc7⟩
Astrophys.J.
Astrophys.J., 2021, 908 (1), pp.1. ⟨10.3847/1538-4357/abccc7⟩
The Astrophysical Journal, American Astronomical Society, 2021, 908 (1), pp.1. ⟨10.3847/1538-4357/abccc7⟩
Astrophys.J.
Astrophys.J., 2021, 908 (1), pp.1. ⟨10.3847/1538-4357/abccc7⟩
We study the evolution and gravitational wave emission of white dwarf -- black hole accreting binaries with a semi-analytical model. These systems will evolve across the mHz gravitational wave frequency band and potentially be detected by the Laser I
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::55c81439cd804c89c948be515c66c1e0
https://hal.archives-ouvertes.fr/hal-02981254
https://hal.archives-ouvertes.fr/hal-02981254
Autor:
Giulia Cusin, Paolo Pani, Nicola Tamanini, Andrea Caputo, Chiara Caprini, Alberto Sesana, Enrico Barausse, Alexandre Toubiana, Laura Sberna, Karan Jani, Stanislav Babak, Sylvain Marsat
Publikováno v:
Physical Review Letters
Phys.Rev.Lett.
Phys.Rev.Lett., 2021, 126 (10), pp.101105. ⟨10.1103/PhysRevLett.126.101105⟩
Physical Review Letters, American Physical Society, 2021, 126 (10), pp.101105. ⟨10.1103/PhysRevLett.126.101105⟩
Phys.Rev.Lett.
Phys.Rev.Lett., 2021, 126 (10), pp.101105. ⟨10.1103/PhysRevLett.126.101105⟩
Physical Review Letters, American Physical Society, 2021, 126 (10), pp.101105. ⟨10.1103/PhysRevLett.126.101105⟩
GW190521 is the compact binary with the largest masses observed to date, with at least one in the pair-instability gap. This event has also been claimed to be associated with an optical flare observed by the Zwicky Transient Facility in an Active Gal
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9c1ef816fd5773bd1fd71f42dc3644f8
http://hdl.handle.net/11573/1563236
http://hdl.handle.net/11573/1563236
Publikováno v:
Physical Review D
We investigate the linear dynamics of an electromagnetic field propagating in curved spacetime in the presence of plasma. The dynamical equations are generically more involved and richer than the effective Proca equation adopted as a model in previou
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2dc876c0649a09f740831ebeeca6a058
http://arxiv.org/abs/2012.05114
http://arxiv.org/abs/2012.05114