Zobrazeno 1 - 3
of 3
pro vyhledávání: '"Gabriel S. Bonilla"'
Autor:
Nils L Vu, Samuel Rodriguez, Tom Włodarczyk, Geoffrey Lovelace, Harald P Pfeiffer, Gabriel S Bonilla, Nils Deppe, François Hébert, Lawrence E Kidder, Jordan Moxon, William Throwe
Publikováno v:
Classical and Quantum Gravity
Brownian coating thermal noise in detector test masses is limiting the sensitivity of current gravitational-wave detectors on Earth. Therefore, accurate numerical models can inform the ongoing effort to minimize Brownian coating thermal noise in curr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4a775510dae33ddb08447f33e94d14fb
https://hdl.handle.net/21.11116/0000-000A-BBFC-821.11116/0000-000A-BBFE-621.11116/0000-000C-8377-A
https://hdl.handle.net/21.11116/0000-000A-BBFC-821.11116/0000-000A-BBFE-621.11116/0000-000C-8377-A
Autor:
Nils Deppe, François Hébert, Lawrence E. Kidder, William Throwe, Isha Anantpurkar, Cristóbal Armaza, Gabriel S. Bonilla, Michael Boyle, Himanshu Chaudhary, Matthew D. Duez, Nils L. Vu, Francois Foucart, Matthew Giesler, Jason S. Guo, Yoonsoo Kim, Prayush Kumar, Isaac Legred, Dongjun Li, Geoffrey Lovelace, Sizheng Ma, Alexandra Macedo, Denyz Melchor, Marlo Morales, Jordan Moxon, Kyle C. Nelli, Eamonn O’Shea, Harald P. Pfeiffer, Teresita Ramirez, Hannes R. Rüter, Jennifer Sanchez, Mark A. Scheel, Sierra Thomas, Daniel Vieira, Nikolas A. Wittek, Tom Wlodarczyk, Saul A. Teukolsky
Publikováno v:
Physical Review D
Discontinuous Galerkin methods are popular because they can achieve high order where the solution is smooth, because they can capture shocks while needing only nearest-neighbor communication, and because they are relatively easy to formulate on compl
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3ced9495facdff4d71900557cb45902b
https://resolver.caltech.edu/CaltechAUTHORS:20220715-332513000
https://resolver.caltech.edu/CaltechAUTHORS:20220715-332513000
Autor:
Nils L. Vu, Harald P. Pfeiffer, Gabriel S. Bonilla, Nils Deppe, François Hébert, Lawrence E. Kidder, Geoffrey Lovelace, Jordan Moxon, Mark A. Scheel, Saul A. Teukolsky, William Throwe, Nikolas A. Wittek, Tom Włodarczyk
Publikováno v:
Physical Review D
Elliptic partial differential equations must be solved numerically for many problems in numerical relativity, such as initial data for every simulation of merging black holes and neutron stars. Existing elliptic solvers can take multiple days to solv
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bffb08152adde8a19f24cdd4d7a4db9e
https://hdl.handle.net/21.11116/0000-000A-7B19-121.11116/0000-000A-7B2C-C21.11116/0000-000A-7B1B-F
https://hdl.handle.net/21.11116/0000-000A-7B19-121.11116/0000-000A-7B2C-C21.11116/0000-000A-7B1B-F