File Download

There are no files associated with this item.

  Links for fulltext
     (May Require Subscription)
Supplementary

Article: Multi-messenger astrophysics with THESEUS in the 2030s

TitleMulti-messenger astrophysics with THESEUS in the 2030s
Authors
KeywordsCompact binary merger
Gamma-ray burst
Kilonova
Multi-messenger astrophysics
Neutrino sources
X-ray sources
Issue Date2021
Citation
Experimental Astronomy, 2021, v. 52, n. 3, p. 245-275 How to Cite?
AbstractMulti-messenger astrophysics is becoming a major avenue to explore the Universe, with the potential to span a vast range of redshifts. The growing synergies between different probes is opening new frontiers, which promise profound insights into several aspects of fundamental physics and cosmology. In this context, THESEUS will play a central role during the 2030s in detecting and localizing the electromagnetic counterparts of gravitational wave and neutrino sources that the unprecedented sensitivity of next generation detectors will discover at much higher rates than the present. Here, we review the most important target signals from multi-messenger sources that THESEUS will be able to detect and characterize, discussing detection rate expectations and scientific impact.
Persistent Identifierhttp://hdl.handle.net/10722/361618
ISSN
2023 Impact Factor: 2.7
2023 SCImago Journal Rankings: 0.894

 

DC FieldValueLanguage
dc.contributor.authorCiolfi, Riccardo-
dc.contributor.authorStratta, Giulia-
dc.contributor.authorBranchesi, Marica-
dc.contributor.authorGendre, Bruce-
dc.contributor.authorGrimm, Stefan-
dc.contributor.authorHarms, Jan-
dc.contributor.authorLamb, Gavin Paul-
dc.contributor.authorMartin-Carrillo, Antonio-
dc.contributor.authorMcCann, Ayden-
dc.contributor.authorOganesyan, Gor-
dc.contributor.authorPalazzi, Eliana-
dc.contributor.authorRonchini, Samuele-
dc.contributor.authorRossi, Andrea-
dc.contributor.authorSalafia, Om Sharan-
dc.contributor.authorSalmon, Lana-
dc.contributor.authorAscenzi, Stefano-
dc.contributor.authorCapone, Antonio-
dc.contributor.authorCelli, Silvia-
dc.contributor.authorDall’Osso, Simone-
dc.contributor.authorDi Palma, Irene-
dc.contributor.authorFasano, Michela-
dc.contributor.authorFermani, Paolo-
dc.contributor.authorGuetta, Dafne-
dc.contributor.authorHanlon, Lorraine-
dc.contributor.authorHowell, Eric-
dc.contributor.authorPaltani, Stephane-
dc.contributor.authorRezzolla, Luciano-
dc.contributor.authorVinciguerra, Serena-
dc.contributor.authorZegarelli, Angela-
dc.contributor.authorAmati, Lorenzo-
dc.contributor.authorBlain, Andrew-
dc.contributor.authorBozzo, Enrico-
dc.contributor.authorChaty, Sylvain-
dc.contributor.authorD’Avanzo, Paolo-
dc.contributor.authorDe Pasquale, fnm Massimiliano-
dc.contributor.authorDereli-Bégué, Hüsne-
dc.contributor.authorGhirlanda, Giancarlo-
dc.contributor.authorGomboc, Andreja-
dc.contributor.authorGötz, Diego-
dc.contributor.authorHorvath, Istvan-
dc.contributor.authorHudec, Rene-
dc.contributor.authorIzzo, Luca-
dc.contributor.authorLe Floch, Emeric-
dc.contributor.authorLi, Liang-
dc.contributor.authorLongo, Francesco-
dc.contributor.authorKomossa, S.-
dc.contributor.authorKong, Albert K.H.-
dc.contributor.authorMereghetti, Sandro-
dc.contributor.authorMignani, Roberto-
dc.contributor.authorNathanail, Antonios-
dc.contributor.authorO’Brien, Paul T.-
dc.contributor.authorOsborne, Julian P.-
dc.contributor.authorPe’er, Asaf-
dc.contributor.authorPiranomonte, Silvia-
dc.contributor.authorRosati, Piero-
dc.contributor.authorSavaglio, Sandra-
dc.contributor.authorSchüssler, Fabian-
dc.contributor.authorSergijenko, Olga-
dc.contributor.authorShao, Lijing-
dc.contributor.authorTanvir, Nial-
dc.contributor.authorTurriziani, Sara-
dc.contributor.authorUrata, Yuji-
dc.contributor.authorvan Putten, Maurice-
dc.contributor.authorVergani, Susanna-
dc.contributor.authorZane, Silvia-
dc.contributor.authorZhang, Bing-
dc.date.accessioned2025-09-16T04:18:12Z-
dc.date.available2025-09-16T04:18:12Z-
dc.date.issued2021-
dc.identifier.citationExperimental Astronomy, 2021, v. 52, n. 3, p. 245-275-
dc.identifier.issn0922-6435-
dc.identifier.urihttp://hdl.handle.net/10722/361618-
dc.description.abstractMulti-messenger astrophysics is becoming a major avenue to explore the Universe, with the potential to span a vast range of redshifts. The growing synergies between different probes is opening new frontiers, which promise profound insights into several aspects of fundamental physics and cosmology. In this context, THESEUS will play a central role during the 2030s in detecting and localizing the electromagnetic counterparts of gravitational wave and neutrino sources that the unprecedented sensitivity of next generation detectors will discover at much higher rates than the present. Here, we review the most important target signals from multi-messenger sources that THESEUS will be able to detect and characterize, discussing detection rate expectations and scientific impact.-
dc.languageeng-
dc.relation.ispartofExperimental Astronomy-
dc.subjectCompact binary merger-
dc.subjectGamma-ray burst-
dc.subjectKilonova-
dc.subjectMulti-messenger astrophysics-
dc.subjectNeutrino sources-
dc.subjectX-ray sources-
dc.titleMulti-messenger astrophysics with THESEUS in the 2030s-
dc.typeArticle-
dc.description.naturelink_to_subscribed_fulltext-
dc.identifier.doi10.1007/s10686-021-09795-9-
dc.identifier.scopuseid_2-s2.0-85117111956-
dc.identifier.volume52-
dc.identifier.issue3-
dc.identifier.spage245-
dc.identifier.epage275-
dc.identifier.eissn1572-9508-

Export via OAI-PMH Interface in XML Formats


OR


Export to Other Non-XML Formats