Zobrazeno 1 - 10
of 80
pro vyhledávání: '"Leo C Stein"'
Autor:
William A. Clark, Mario W. Gomes, Arnaldo Rodriguez-Gonzalez, Leo C. Stein, Steven H. Strogatz
Publikováno v:
SIAM Review. 65:291-315
We revisit a textbook example of a singularly perturbed nonlinear boundary-value problem. Unexpectedly, it shows a wealth of phenomena that seem to have been overlooked previously, including a pitchfork bifurcation in the number of solutions as one v
Autor:
Keefe Mitman, Macarena Lagos, Leo C. Stein, Sizheng Ma, Lam Hui, Yanbei Chen, Nils Deppe, François Hébert, Lawrence E. Kidder, Jordan Moxon, Mark A. Scheel, Saul A. Teukolsky, William Throwe, Nils L. Vu
Publikováno v:
Physical Review Letters
The gravitational wave strain emitted by a perturbed black hole (BH) ringing down is typically modeled analytically using first-order BH perturbation theory. In this Letter we show that second-order effects are necessary for modeling ringdowns from B
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3d97847464f33234574ff7323985c23d
http://arxiv.org/abs/2208.07380
http://arxiv.org/abs/2208.07380
Autor:
Keefe Mitman, Leo C. Stein, Michael Boyle, Nils Deppe, François Hébert, Lawrence E. Kidder, Jordan Moxon, Mark A. Scheel, Saul A. Teukolsky, William Throwe, Nils L. Vu
Publikováno v:
Physical Review D
The Bondi-van der Burg-Metzner-Sachs (BMS) group, which uniquely describes the symmetries of asymptotic infinity and therefore of the gravitational waves that propagate there, has become increasingly important for accurate modeling of waveforms. In p
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4ff369b03e1c545599a5032a52fb64c5
http://arxiv.org/abs/2208.04356
http://arxiv.org/abs/2208.04356
Autor:
Vijay Varma, Scott E. Field, Mark A. Scheel, Jonathan Blackman, Davide Gerosa, Leo C. Stein, Lawrence E. Kidder, Harald P. Pfeiffer
Publikováno v:
Physical Review Research, Vol 1, Iss 3, p 033015 (2019)
Only numerical relativity simulations can capture the full complexities of binary black hole mergers. These simulations, however, are prohibitively expensive for direct data analysis applications such as parameter estimation. We present two fast and
Externí odkaz:
https://doaj.org/article/e3cabaf341a04d9cb4b660be5f7434a2
Autor:
K. G. Arun, Enis Belgacem, Robert Benkel, Laura Bernard, Emanuele Berti, Gianfranco Bertone, Marc Besancon, Diego Blas, Christian G. Böhmer, Richard Brito, Gianluca Calcagni, Alejandro Cardenas-Avendaño, Katy Clough, Marco Crisostomi, Valerio De Luca, Daniela Doneva, Stephanie Escoffier, José María Ezquiaga, Pedro G. Ferreira, Pierre Fleury, Stefano Foffa, Gabriele Franciolini, Noemi Frusciante, Juan García-Bellido, Carlos Herdeiro, Thomas Hertog, Tanja Hinderer, Philippe Jetzer, Lucas Lombriser, Elisa Maggio, Michele Maggiore, Michele Mancarella, Andrea Maselli, Sourabh Nampalliwar, David Nichols, Maria Okounkova, Paolo Pani, Vasileios Paschalidis, Alvise Raccanelli, Lisa Randall, Sébastien Renaux-Petel, Antonio Riotto, Milton Ruiz, Alexander Saffer, Mairi Sakellariadou, Ippocratis D. Saltas, B. S. Sathyaprakash, Lijing Shao, Carlos F. Sopuerta, Thomas P. Sotiriou, Nikolaos Stergioulas, Nicola Tamanini, Filippo Vernizzi, Helvi Witek, Kinwah Wu, Kent Yagi, Stoytcho Yazadjiev, Nicolás Yunes, Miguel Zilhão, Niayesh Afshordi, Marie-Christine Angonin, Vishal Baibhav, Enrico Barausse, Tiago Barreiro, Nicola Bartolo, Nicola Bellomo, Ido Ben-Dayan, Eric A. Bergshoeff, Sebastiano Bernuzzi, Daniele Bertacca, Swetha Bhagwat, Béatrice Bonga, Lior M. Burko, Geoffrey Compére, Giulia Cusin, Antonio da Silva, Saurya Das, Claudia de Rham, Kyriakos Destounis, Ema Dimastrogiovanni, Francisco Duque, Richard Easther, Hontas Farmer, Matteo Fasiello, Stanislav Fisenko, Kwinten Fransen, Jörg Frauendiener, Jonathan Gair, László Árpád Gergely, Davide Gerosa, Leonardo Gualtieri, Wen-Biao Han, Aurelien Hees, Thomas Helfer, Jörg Hennig, Alexander C. Jenkins, Eric Kajfasz, Nemanja Kaloper, Vladimír Karas, Bradley J. Kavanagh, Sergei A. Klioner, Savvas M. Koushiappas, Macarena Lagos, Christophe Le Poncin-Lafitte, Francisco S. N. Lobo, Charalampos Markakis, Prado Martín-Moruno, C. J. A. P. Martins, Sabino Matarrese, Daniel R. Mayerson, José P. Mimoso, Johannes Noller, Nelson J. Nunes, Roberto Oliveri, Giorgio Orlando, George Pappas, Igor Pikovski, Luigi Pilo, Jiří Podolský, Geraint Pratten, Tomislav Prokopec, Hong Qi, Saeed Rastgoo, Angelo Ricciardone, Rocco Rollo, Diego Rubiera-Garcia, Olga Sergijenko, Stuart Shapiro, Deirdre Shoemaker, Alessandro Spallicci, Oleksandr Stashko, Leo C. Stein, Gianmassimo Tasinato, Andrew J. Tolley, Elias C. Vagenas, Stefan Vandoren, Daniele Vernieri, Rodrigo Vicente, Toby Wiseman, Valery I. Zhdanov, Miguel Zumalacárregui
Publikováno v:
Living Reviews in Relativity, 25(1), 1. Albert Einstein Institut
Living Reviews in Relativity
Living Rev.Rel.
Living Rev.Rel., 2022, 25 (1), pp.4. ⟨10.1007/s41114-022-00036-9⟩
E-Prints Complutense. Archivo Institucional de la UCM
instname
Arun, K. G. Ruiz Meneses, Milton Javier 2022 New horizons for fundamental physics with LISA Living Reviews In Relativity 25 4
Living Reviews in Relativity, 25, 1-148
Living Reviews in Relativity, 25(1):4. Albert Einstein Institut
Living Reviews in Relativity, 25, 1, pp. 1-148
Living Reviews in Relativity
Living Rev.Rel.
Living Rev.Rel., 2022, 25 (1), pp.4. ⟨10.1007/s41114-022-00036-9⟩
E-Prints Complutense. Archivo Institucional de la UCM
instname
Arun, K. G. Ruiz Meneses, Milton Javier 2022 New horizons for fundamental physics with LISA Living Reviews In Relativity 25 4
Living Reviews in Relativity, 25, 1-148
Living Reviews in Relativity, 25(1):4. Albert Einstein Institut
Living Reviews in Relativity, 25, 1, pp. 1-148
K. G. Arun et al.
The Laser Interferometer Space Antenna (LISA) has the potential to reveal wonders about the fundamental theory of nature at play in the extreme gravity regime, where the gravitational interaction is both strong and dynamical. I
The Laser Interferometer Space Antenna (LISA) has the potential to reveal wonders about the fundamental theory of nature at play in the extreme gravity regime, where the gravitational interaction is both strong and dynamical. I
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6ee753d4ce141fae6dca78bfdba343d8
https://orca.cardiff.ac.uk/id/eprint/150937/1/41114_2022_Article_36.pdf
https://orca.cardiff.ac.uk/id/eprint/150937/1/41114_2022_Article_36.pdf
Autor:
Lorena Magaña Zertuche, Keefe Mitman, Neev Khera, Leo C. Stein, Michael Boyle, Nils Deppe, François Hébert, Dante A. B. Iozzo, Lawrence E. Kidder, Jordan Moxon, Harald P. Pfeiffer, Mark A. Scheel, Saul A. Teukolsky, William Throwe, Nils Vu
Publikováno v:
Physical Review D
Quasi-normal mode (QNM) modeling is an invaluable tool for characterizing remnant black holes, studying strong gravity, and testing GR. Only recently have QNM studies begun to focus on multimode fitting to numerical relativity (NR) strain waveforms.
Autor:
José T. Gálvez Ghersi, Leo C. Stein
Publikováno v:
Physical review. E. 104(3-1)
Perturbation theory is a crucial tool for many physical systems, when exact solutions are not available, or nonperturbative numerical solutions are intractable. Naive perturbation theory often fails on long timescales, leading to secularly growing so
Autor:
Michael Boyle, Lawrence E. Kidder, Dante A. B. Iozzo, Harald P. Pfeiffer, Jordan Moxon, Leo C. Stein, William Throwe, Keefe Mitman, Saul A. Teukolsky, Neev Khera, Nils Deppe, François Hébert, Mark A. Scheel
Publikováno v:
Physical Review D
We present a new study of remnant black hole properties from 13 binary black hole systems, numerically evolved using the Spectral Einstein Code. The mass, spin, and recoil velocity of each remnant were determined quasi-locally from apparent horizon d
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::438d9dfec00b8854a2f92ae13b100022
https://resolver.caltech.edu/CaltechAUTHORS:20210623-155717011
https://resolver.caltech.edu/CaltechAUTHORS:20210623-155717011
Autor:
William Throwe, Mark A. Scheel, Dante A. B. Iozzo, Nils Deppe, Leo C. Stein, Keefe Mitman, Jordan Moxon, Lawrence E. Kidder, Michael Boyle, Harald P. Pfeiffer, Saul A. Teukolsky, Neev Khera
Publikováno v:
Physical Review D
Understanding the Bondi-Metzner-Sachs (BMS) frame of the gravitational waves produced by numerical relativity is crucial for ensuring that analyses on such waveforms are performed properly. It is also important that models are built from waveforms in
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d9cbc4b26d9e10c3d3c7816d5d4b9e89
http://arxiv.org/abs/2105.02300
http://arxiv.org/abs/2105.02300
We perform a new test of general relativity (GR) with signals from GWTC-2, the LIGO and Virgo catalog of gravitational wave detections. We search for the presence of amplitude birefringence, in which left versus right circularly polarized modes of gr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::529a06874449ce83dc835a9f9edaf9f4
http://arxiv.org/abs/2101.11153
http://arxiv.org/abs/2101.11153