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pro vyhledávání: '"Ceja, Andrea"'
Autor:
Lovelace, Geoffrey, Nelli, Kyle C., Deppe, Nils, Vu, Nils L., Throwe, William, Bonilla, Marceline S., Carpenter, Alexander, Kidder, Lawrence E., Macedo, Alexandra, Scheel, Mark A., Afram, Azer, Boyle, Michael, Ceja, Andrea, Giesler, Matthew, Habib, Sarah, Jones, Ken Z., Kumar, Prayush, Lara, Guillermo, Melchor, Denyz, Mendes, Iago B., Mitman, Keefe, Morales, Marlo, Moxon, Jordan, O'Shea, Eamonn, Pannone, Kyle, Pfeiffer, Harald P., Ramirez-Aguilar, Teresita, Sanchez, Jennifer, Tellez, Daniel, Teukolsky, Saul A., Wittek, Nikolas A.
Binary black holes are the most abundant source of gravitational-wave observations. Gravitational-wave observatories in the next decade will require tremendous increases in the accuracy of numerical waveforms modeling binary black holes, compared to
Externí odkaz:
http://arxiv.org/abs/2410.00265
Autor:
Boschini, Matteo, Gerosa, Davide, Varma, Vijay, Armaza, Cristobal, Boyle, Michael, Bonilla, Marceline S., Ceja, Andrea, Chen, Yitian, Deppe, Nils, Giesler, Matthew, Kidder, Lawrence E., Kumar, Prayush, Lara, Guillermo, Long, Oliver, Ma, Sizheng, Mitman, Keefe, Nee, Peter James, Pfeiffer, Harald P., Ramos-Buades, Antoni, Scheel, Mark A., Vu, Nils L., Yoo, Jooheon
Publikováno v:
Phys.Rev.D 108 (2023) 8, 084015
Numerical-relativity surrogate models for both black-hole merger waveforms and remnants have emerged as important tools in gravitational-wave astronomy. While producing very accurate predictions, their applicability is limited to the region of the pa
Externí odkaz:
http://arxiv.org/abs/2307.03435