Multi-messenger astrophysics with THESEUS in the 2030s
Yazar
Pe'er, Asaf
Gomboc, Andreja
Gotz, Diego
Horvath, Istvan
Hudec, Rene
Izzo, Luca
Le Floch, Emeric
Li, Liang
Longo, Francesco
Komossa, S.
Kong, Albert K. H.
Mereghetti, Sandro
Mignani, Roberto
Nathanail, Antonios
O'Brien, Paul T.
Osborne, Julian P.
Piranomonte, Silvia
Rosati, Piero
Savaglio, Sandra
Schussler, Fabian
Sergijenko, Olga
Shao, Lijing
Tanvir, Nial
Turriziani, Sara
Urata, Yuji
van Putten, Maurice
Vergani, Susanna
Zane, Silvia
Zhang, Bing
Ciolfi, Riccardo
Stratta, Giulia
Branchesi, Marica
Gendre, Bruce
Grimm, Stefan
Harms, Jan
Lamb, Gavin Paul
Martin-Carrillo, Antonio
McCann, Ayden
Oganesyan, Gor
Palazzi, Eliana
Ronchini, Samuele
Rossi, Andrea
Salafia, Om Sharan
Salmon, Lana
Ascenzi, Stefano
Capone, Antonio
Celli, Silvia
Dall'Osso, Simone
Di Palma, Irene
Fasano, Michela
Fermani, Paolo
Guetta, Dafne
Hanlon, Lorraine
Howell, Eric
Paltani, Stephane
Rezzolla, Luciano
Vinciguerra, Serena
Zegarelli, Angela
Amati, Lorenzo
Blain, Andrew
Bozzo, Enrico
Chaty, Sylvain
D'Avanzo, Paolo
De Pasquale, FnmMassimiliano
Dereli-Begue, Husne
Ghirlanda, Giancarlo
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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.
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