Change search
CiteExportLink to record
Permanent link

Direct link
Cite
Citation style
  • apa
  • ieee
  • modern-language-association-8th-edition
  • vancouver
  • Other style
More styles
Language
  • de-DE
  • en-GB
  • en-US
  • fi-FI
  • nn-NO
  • nn-NB
  • sv-SE
  • Other locale
More languages
Output format
  • html
  • text
  • asciidoc
  • rtf
Enabling real-time multi-messenger astrophysics discoveries with deep learning
Show others and affiliations
Number of Authors: 602019 (English)In: Nature reviews physics, ISSN 2522-5820, Vol. 1, no 10, p. 600-608Article, review/survey (Refereed) Published
Abstract [en]

Multi-messenger astrophysics is a fast-growing, interdisciplinary field that combines data, which vary in volume and speed of data processing, from many different instruments that probe the Universe using different cosmic messengers: electromagnetic waves, cosmic rays, gravitational waves and neutrinos. In this Expert Recommendation, we review the key challenges of real-time observations of gravitational wave sources and their electromagnetic and astroparticle counterparts, and make a number of recommendations to maximize their potential for scientific discovery. These recommendations refer to the design of scalable and computationally efficient machine learning algorithms; the cyber-infrastructure to numerically simulate astrophysical sources, and to process and interpret multi-messenger astrophysics data; the management of gravitational wave detections to trigger real-time alerts for electromagnetic and astroparticle follow-ups; a vision to harness future developments of machine learning and cyber-infrastructure resources to cope with the big-data requirements; and the need to build a community of experts to realize the goals of multi-messenger astrophysics. A group of experts suggests ways in which deep learning can be used to enhance the potential for discovery in multi-messenger astrophysics.

Place, publisher, year, edition, pages
2019. Vol. 1, no 10, p. 600-608
National Category
Physical Sciences
Identifiers
URN: urn:nbn:se:su:diva-184006DOI: 10.1038/s42254-019-0097-4ISI: 000542186400005Scopus ID: 2-s2.0-85077465113OAI: oai:DiVA.org:su-184006DiVA, id: diva2:1478635
Available from: 2020-10-22 Created: 2020-10-22 Last updated: 2022-11-02Bibliographically approved

Open Access in DiVA

No full text in DiVA

Other links

Publisher's full textScopusarXiv:1911.11779

Authority records

Huerta, E. A.Biswas, RahulKindratenko, VolodymyrTsokaros, Antonios

Search in DiVA

By author/editor
Huerta, E. A.Biswas, RahulKindratenko, VolodymyrTsokaros, Antonios
By organisation
Department of PhysicsThe Oskar Klein Centre for Cosmo Particle Physics (OKC)
Physical Sciences

Search outside of DiVA

GoogleGoogle Scholar

doi
urn-nbn

Altmetric score

doi
urn-nbn
Total: 22 hits
CiteExportLink to record
Permanent link

Direct link
Cite
Citation style
  • apa
  • ieee
  • modern-language-association-8th-edition
  • vancouver
  • Other style
More styles
Language
  • de-DE
  • en-GB
  • en-US
  • fi-FI
  • nn-NO
  • nn-NB
  • sv-SE
  • Other locale
More languages
Output format
  • html
  • text
  • asciidoc
  • rtf