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Gravitational Wave Data Analysis: Computing Challenges in the 3G Era

Cyber infrastructure will be a critical consideration in the development of next generation gravitational-wave detectors. The demand for data analysis computing in the 3G era will be driven by the high number of detections as well as the expanded search parameter space for compact astrophysical obje...

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Autores principales: Couvares, Peter, Bird, Ian, Porter, Edward, Bagnasco, Stefano, Lovelace, Geoffrey, Punturo, Michele, Reitze, David, Katsanevas, Stavros, Kajita, Takaaki, Kalogera, Vicky, Lueck, Harald, McClelland, David, Rowan, Sheila, Sanders, Gary, Sathyaprakash, B.S., Shoemaker, David, Brand, Jo van den
Lenguaje:eng
Publicado: 2021
Materias:
Acceso en línea:http://cds.cern.ch/record/2791843
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author Couvares, Peter
Bird, Ian
Porter, Edward
Bagnasco, Stefano
Lovelace, Geoffrey
Punturo, Michele
Reitze, David
Katsanevas, Stavros
Kajita, Takaaki
Kalogera, Vicky
Lueck, Harald
McClelland, David
Rowan, Sheila
Sanders, Gary
Sathyaprakash, B.S.
Shoemaker, David
Brand, Jo van den
author_facet Couvares, Peter
Bird, Ian
Porter, Edward
Bagnasco, Stefano
Lovelace, Geoffrey
Punturo, Michele
Reitze, David
Katsanevas, Stavros
Kajita, Takaaki
Kalogera, Vicky
Lueck, Harald
McClelland, David
Rowan, Sheila
Sanders, Gary
Sathyaprakash, B.S.
Shoemaker, David
Brand, Jo van den
author_sort Couvares, Peter
collection CERN
description Cyber infrastructure will be a critical consideration in the development of next generation gravitational-wave detectors. The demand for data analysis computing in the 3G era will be driven by the high number of detections as well as the expanded search parameter space for compact astrophysical objects and the subsequent parameter estimation follow-up required to extract the nature of the sources. Additionally, there will be an increased need to develop appropriate and scalable computing cyberinfrastructure, including data access and transfer protocols, and storage and management of software tools, that have sustainable development, support, and management processes. This report identifies the major challenges and opportunities facing 3G gravitational-wave observatories and presents recommendations for addressing them. This report is the fourth in a six part series of reports by the GWIC 3G Subcommittee: i) Expanding the Reach of Gravitational Wave Observatories to the Edge of the Universe, ii) The Next Generation Global Gravitational Wave Observatory: The Science Book, iii) 3G R&D: R&D for the Next Generation of Ground-based Gravitational Wave Detectors, iv) Gravitational Wave Data Analysis: Computing Challenges in the 3G Era (this report), v) Future Ground-based Gravitational-wave Observatories: Synergies with Other Scientific Communities, and vi) An Exploration of Possible Governance Models for the Future Global Gravitational-Wave Observatory Network.
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institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2021
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spelling cern-27918432023-01-31T10:46:14Zhttp://cds.cern.ch/record/2791843engCouvares, PeterBird, IanPorter, EdwardBagnasco, StefanoLovelace, GeoffreyPunturo, MicheleReitze, DavidKatsanevas, StavrosKajita, TakaakiKalogera, VickyLueck, HaraldMcClelland, DavidRowan, SheilaSanders, GarySathyaprakash, B.S.Shoemaker, DavidBrand, Jo van denGravitational Wave Data Analysis: Computing Challenges in the 3G Eraastro-ph.IMAstrophysics and Astronomyastro-ph.HEAstrophysics and Astronomygr-qcGeneral Relativity and CosmologyCyber infrastructure will be a critical consideration in the development of next generation gravitational-wave detectors. The demand for data analysis computing in the 3G era will be driven by the high number of detections as well as the expanded search parameter space for compact astrophysical objects and the subsequent parameter estimation follow-up required to extract the nature of the sources. Additionally, there will be an increased need to develop appropriate and scalable computing cyberinfrastructure, including data access and transfer protocols, and storage and management of software tools, that have sustainable development, support, and management processes. This report identifies the major challenges and opportunities facing 3G gravitational-wave observatories and presents recommendations for addressing them. This report is the fourth in a six part series of reports by the GWIC 3G Subcommittee: i) Expanding the Reach of Gravitational Wave Observatories to the Edge of the Universe, ii) The Next Generation Global Gravitational Wave Observatory: The Science Book, iii) 3G R&D: R&D for the Next Generation of Ground-based Gravitational Wave Detectors, iv) Gravitational Wave Data Analysis: Computing Challenges in the 3G Era (this report), v) Future Ground-based Gravitational-wave Observatories: Synergies with Other Scientific Communities, and vi) An Exploration of Possible Governance Models for the Future Global Gravitational-Wave Observatory Network.arXiv:2111.06987oai:cds.cern.ch:27918432021-11-12
spellingShingle astro-ph.IM
Astrophysics and Astronomy
astro-ph.HE
Astrophysics and Astronomy
gr-qc
General Relativity and Cosmology
Couvares, Peter
Bird, Ian
Porter, Edward
Bagnasco, Stefano
Lovelace, Geoffrey
Punturo, Michele
Reitze, David
Katsanevas, Stavros
Kajita, Takaaki
Kalogera, Vicky
Lueck, Harald
McClelland, David
Rowan, Sheila
Sanders, Gary
Sathyaprakash, B.S.
Shoemaker, David
Brand, Jo van den
Gravitational Wave Data Analysis: Computing Challenges in the 3G Era
title Gravitational Wave Data Analysis: Computing Challenges in the 3G Era
title_full Gravitational Wave Data Analysis: Computing Challenges in the 3G Era
title_fullStr Gravitational Wave Data Analysis: Computing Challenges in the 3G Era
title_full_unstemmed Gravitational Wave Data Analysis: Computing Challenges in the 3G Era
title_short Gravitational Wave Data Analysis: Computing Challenges in the 3G Era
title_sort gravitational wave data analysis: computing challenges in the 3g era
topic astro-ph.IM
Astrophysics and Astronomy
astro-ph.HE
Astrophysics and Astronomy
gr-qc
General Relativity and Cosmology
url http://cds.cern.ch/record/2791843
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