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Multi-messenger astrophysics with THESEUS in the 2030s

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dc.contributor.author Ciolfi R.
dc.contributor.author Stratta G.
dc.contributor.author Branchesi M.
dc.contributor.author Gendre B.
dc.contributor.author Grimm S.
dc.contributor.author Harms J.
dc.contributor.author Lamb G.P.
dc.contributor.author Martin-Carrillo A.
dc.contributor.author McCann A.
dc.contributor.author Oganesyan G.
dc.contributor.author Palazzi E.
dc.contributor.author Ronchini S.
dc.contributor.author Rossi A.
dc.contributor.author Salafia O.S.
dc.contributor.author Salmon L.
dc.contributor.author Ascenzi S.
dc.contributor.author Capone A.
dc.contributor.author Celli S.
dc.contributor.author Dall’Osso S.
dc.contributor.author Di Palma I.
dc.contributor.author Fasano M.
dc.contributor.author Fermani P.
dc.contributor.author Guetta D.
dc.contributor.author Hanlon L.
dc.contributor.author Howell E.
dc.contributor.author Paltani S.
dc.contributor.author Rezzolla L.
dc.contributor.author Vinciguerra S.
dc.contributor.author Zegarelli A.
dc.contributor.author Amati L.
dc.contributor.author Blain A.
dc.contributor.author Bozzo E.
dc.contributor.author Chaty S.
dc.contributor.author D’Avanzo P.
dc.contributor.author De Pasquale f.M.
dc.contributor.author Dereli-Bégué H.
dc.contributor.author Ghirlanda G.
dc.contributor.author Gomboc A.
dc.contributor.author Götz D.
dc.contributor.author Horvath I.
dc.contributor.author Hudec R.
dc.contributor.author Izzo L.
dc.contributor.author Le Floch E.
dc.contributor.author Li L.
dc.contributor.author Longo F.
dc.contributor.author Komossa S.
dc.contributor.author Kong A.K.H.
dc.contributor.author Mereghetti S.
dc.contributor.author Mignani R.
dc.contributor.author Nathanail A.
dc.contributor.author O’Brien P.T.
dc.contributor.author Osborne J.P.
dc.contributor.author Pe’er A.
dc.contributor.author Piranomonte S.
dc.contributor.author Rosati P.
dc.contributor.author Savaglio S.
dc.contributor.author Schüssler F.
dc.contributor.author Sergijenko O.
dc.contributor.author Shao L.
dc.contributor.author Tanvir N.
dc.contributor.author Turriziani S.
dc.contributor.author Urata Y.
dc.contributor.author van Putten M.
dc.contributor.author Vergani S.
dc.contributor.author Zane S.
dc.contributor.author Zhang B.
dc.date.accessioned 2022-02-09T20:34:28Z
dc.date.available 2022-02-09T20:34:28Z
dc.date.issued 2021
dc.identifier.issn 0922-6435
dc.identifier.uri https://dspace.kpfu.ru/xmlui/handle/net/169121
dc.description.abstract Multi-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.relation.ispartofseries Experimental Astronomy
dc.subject Compact binary merger
dc.subject Gamma-ray burst
dc.subject Kilonova
dc.subject Multi-messenger astrophysics
dc.subject Neutrino sources
dc.subject X-ray sources
dc.title Multi-messenger astrophysics with THESEUS in the 2030s
dc.type Article
dc.collection Публикации сотрудников КФУ
dc.source.id SCOPUS09226435-2021-SID85117111956


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  • Публикации сотрудников КФУ Scopus [24551]
    Коллекция содержит публикации сотрудников Казанского федерального (до 2010 года Казанского государственного) университета, проиндексированные в БД Scopus, начиная с 1970г.

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