Zobrazeno 1 - 10
of 77
pro vyhledávání: '"R, Galley"'
Autor:
O. Crabeck, R. Galley, B. Delille, B. Else, N.-X. Geilfus, M. Lemes, M. Des Roches, P. Francus, J.-L. Tison, S. Rysgaard
Publikováno v:
The Cryosphere, Vol 10, Iss 3, Pp 1125-1145 (2016)
Although the presence of a gas phase in sea ice creates the potential for gas exchange with the atmosphere, the distribution of gas bubbles and transport of gases within the sea ice are still poorly understood. Currently no straightforward technique
Externí odkaz:
https://doaj.org/article/e962a857b96d496c95c06a9de9b17744
Akademický článek
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Autor:
Harald P. Pfeiffer, Scott E. Field, Lawrence E. Kidder, P. Kumar, Mark A. Scheel, Béla Szilágyi, Michael Boyle, Jonathan Blackman, Saul A. Teukolsky, Chad R. Galley
Publikováno v:
Physical Review D
Gravitational-wave detectors have begun to observe coalescences of heavy black holes at a consistent pace for the past few years. Accurate models of gravitational waveforms are essential for unbiased and precise estimation of source parameters. Recen
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a722a0101ae89deb6cc0df297ed6fd7f
https://resolver.caltech.edu/CaltechAUTHORS:20180830-092941715
https://resolver.caltech.edu/CaltechAUTHORS:20180830-092941715
Publikováno v:
Physical Review Letters. 122
Gravitational-wave data analysis is rapidly absorbing techniques from deep learning, with a focus on convolutional networks and related methods that treat noisy time series as images. We pursue an alternative approach, in which waveforms are first re
Publikováno v:
Physical Review X, Vol 4, Iss 3, p 031006 (2014)
We propose a solution to the problem of quickly and accurately predicting gravitational waveforms within any given physical model. The method is relevant for both real-time applications and more traditional scenarios where the generation of waveforms
Externí odkaz:
https://doaj.org/article/21ea84a2b62f43bfbeb0e858a3ff47de
Publikováno v:
Scopus
Repositório Institucional da UNESP
Universidade Estadual Paulista (UNESP)
instacron:UNESP
Web of Science
Repositório Institucional da UNESP
Universidade Estadual Paulista (UNESP)
instacron:UNESP
Web of Science
We compute the leading Post-Newtonian (PN) contributions at linear order in the spin to the radiation-reaction acceleration and spin evolution for binary systems, which enter at fourth PN order. The calculation is carried out, from first principles,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a45269b019e83171741fa08f82dfd566
http://arxiv.org/abs/1705.07934
http://arxiv.org/abs/1705.07934
Publikováno v:
Scopus
Repositório Institucional da UNESP
Universidade Estadual Paulista (UNESP)
instacron:UNESP
Web of Science
Repositório Institucional da UNESP
Universidade Estadual Paulista (UNESP)
instacron:UNESP
Web of Science
We compute the leading Post-Newtonian (PN) contributions at quadratic order in the spins to the radiation-reaction acceleration and spin evolution for binary systems, entering at four-and-a-half PN order. Our calculation includes the back-reaction fr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8bb50a47756b92fcaf78f5d354bbaf66
http://arxiv.org/abs/1705.07938
http://arxiv.org/abs/1705.07938
A Numerical Relativity Waveform Surrogate Model for Generically Precessing Binary Black Hole Mergers
Autor:
Harald P. Pfeiffer, Michael Boyle, Mark A. Scheel, Christian D. Ott, Lawrence E. Kidder, Béla Szilágyi, Scott E. Field, Chad R. Galley, Jonathan Blackman
A generic, non-eccentric binary black hole (BBH) system emits gravitational waves (GWs) that are completely described by 7 intrinsic parameters: the black hole spin vectors and the ratio of their masses. Simulating a BBH coalescence by solving Einste
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6077f1b523bbc6f9d4e42e0c2d317328
Autor:
Jonathan Blackman, Rory Smith, Daniel A. Hemberger, Chad R. Galley, Scott E. Field, Patricia Schmidt, Mark A. Scheel
We present the first surrogate model for gravitational waveforms from the coalescence of precessing binary black holes. We call this surrogate model NRSur4d2s. Our methodology significantly extends recently introduced reduced-order and surrogate mode
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b2271f3d17c186845e68fe4ecc30a93e
Autor:
Robyn K. Fuchs, Jeffrey S. Richard, Stuart J. Warden, Rick G. Barker, Lydia A. George, Matthew R. Galley, Elizabeth A. Guildenbecher, Andrea L. Hurd
Publikováno v:
Journal of Bone and Mineral Research. 29:1131-1140
Skeletal loading enhances cortical and trabecular bone properties. How long these benefits last after loading cessation remains an unresolved, clinically relevant question. This study investigated long-term maintenance of loading-induced cortical and