Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/31588
DC Field | Value | Language |
---|---|---|
dc.contributor.author | CIOLFI, RICCARDO | en_US |
dc.contributor.author | STRATTA, MARIA GIULIANA | en_US |
dc.contributor.author | Branchesi, Marica | en_US |
dc.contributor.author | Gendre, Bruce | en_US |
dc.contributor.author | Grimm, Stefan | en_US |
dc.contributor.author | Harms, Jan | en_US |
dc.contributor.author | Lamb, Gavin Paul | en_US |
dc.contributor.author | Martin-Carrillo, Antonio | en_US |
dc.contributor.author | McCann, Ayden | en_US |
dc.contributor.author | OGANESYAN, GOR | en_US |
dc.contributor.author | PALAZZI, ELIANA | en_US |
dc.contributor.author | RONCHINI, SAMUELE | en_US |
dc.contributor.author | ROSSI, Andrea | en_US |
dc.contributor.author | Salafia, Om Sharan | en_US |
dc.contributor.author | Salmon, Lana | en_US |
dc.contributor.author | ASCENZI, STEFANO | en_US |
dc.contributor.author | Capone, Antonio | en_US |
dc.contributor.author | Celli, Silvia | en_US |
dc.contributor.author | Dall’Osso, Simone | en_US |
dc.contributor.author | Di Palma, Irene | en_US |
dc.contributor.author | Fasano, Michela | en_US |
dc.contributor.author | Fermani, Paolo | en_US |
dc.contributor.author | GUETTA, Dafne | en_US |
dc.contributor.author | Hanlon, Lorraine | en_US |
dc.contributor.author | Howell, Eric | en_US |
dc.contributor.author | Paltani, Stephane | en_US |
dc.contributor.author | Rezzolla, Luciano | en_US |
dc.contributor.author | Vinciguerra, Serena | en_US |
dc.contributor.author | Zegarelli, Angela | en_US |
dc.contributor.author | AMATI, LORENZO | en_US |
dc.contributor.author | Blain, Andrew | en_US |
dc.contributor.author | BOZZO , ENRICO | en_US |
dc.contributor.author | Chaty, Sylvain | en_US |
dc.contributor.author | D'AVANZO, Paolo | en_US |
dc.contributor.author | De Pasquale, fnm Massimiliano | en_US |
dc.contributor.author | Dereli-Bégué, Hüsne | en_US |
dc.contributor.author | GHIRLANDA, Giancarlo | en_US |
dc.contributor.author | Gomboc, Andreja | en_US |
dc.contributor.author | Götz, Diego | en_US |
dc.contributor.author | Horvath, Istvan | en_US |
dc.contributor.author | Hudec, Rene | en_US |
dc.contributor.author | IZZO, LUCA | en_US |
dc.contributor.author | Le Floch, Emeric | en_US |
dc.contributor.author | Li, Liang | en_US |
dc.contributor.author | Longo, Francesco | en_US |
dc.contributor.author | Komossa, S. | en_US |
dc.contributor.author | Kong, Albert K.H. | en_US |
dc.contributor.author | MEREGHETTI, Sandro | en_US |
dc.contributor.author | MIGNANI, Roberto | en_US |
dc.contributor.author | Nathanail, Antonios | en_US |
dc.contributor.author | O’Brien, Paul T. | en_US |
dc.contributor.author | Osborne, Julian P. | en_US |
dc.contributor.author | Pe’er, Asaf | en_US |
dc.contributor.author | PIRANOMONTE, Silvia | en_US |
dc.contributor.author | Rosati, Piero | en_US |
dc.contributor.author | SAVAGLIO, SANDRA | en_US |
dc.contributor.author | Schüssler, Fabian | en_US |
dc.contributor.author | Sergijenko, Olga | en_US |
dc.contributor.author | Shao, Lijing | en_US |
dc.contributor.author | Tanvir, Nial | en_US |
dc.contributor.author | Turriziani, Sara | en_US |
dc.contributor.author | Urata, Yuji | en_US |
dc.contributor.author | van Putten, Maurice | en_US |
dc.contributor.author | VERGANI, SUSANNA | en_US |
dc.contributor.author | Zane, Silvia | en_US |
dc.contributor.author | Zhang, Bing | en_US |
dc.date.accessioned | 2022-03-15T15:01:33Z | - |
dc.date.available | 2022-03-15T15:01:33Z | - |
dc.date.issued | 2021 | en_US |
dc.identifier.issn | 0922-6435 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/31588 | - |
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. | en_US |
dc.language.iso | eng | en_US |
dc.title | Multi-messenger astrophysics with THESEUS in the 2030s | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1007/s10686-021-09795-9 | en_US |
dc.identifier.scopus | 2-s2.0-85117111956 | en_US |
dc.identifier.isi | WOS:000707542600006 | en_US |
dc.identifier.url | https://link.springer.com/article/10.1007/s10686-021-09795-9 | en_US |
dc.identifier.url | https://api.elsevier.com/content/abstract/scopus_id/85117111956 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 52 | en_US |
dc.relation.issue | 3 | en_US |
dc.relation.firstpage | 245 | en_US |
dc.relation.lastpage | 275 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.international | sì | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | EXPERIMENTAL ASTRONOMY | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.relation.ercsector | ERC sectors::Physical Sciences and Engineering::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.openairetype | Article | - |
item.languageiso639-1 | en | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | O.A. Padova | - |
crisitem.author.dept | IAPS Roma | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | O.A. Abruzzo | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | O.A. Brera | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | O.A. Roma | - |
crisitem.author.dept | O.A. Brera | - |
crisitem.author.dept | O.A. Brera | - |
crisitem.author.dept | O.A. Capodimonte | - |
crisitem.author.dept | IASF Milano | - |
crisitem.author.dept | IASF Milano | - |
crisitem.author.dept | O.A. Roma | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | Direzione Scientifica | - |
crisitem.author.dept | O.A. Brera | - |
crisitem.author.orcid | 0000-0003-3140-8933 | - |
crisitem.author.orcid | 0000-0003-1055-7980 | - |
crisitem.author.orcid | 0000-0002-8691-7666 | - |
crisitem.author.orcid | 0000-0002-8860-6538 | - |
crisitem.author.orcid | 0000-0003-4924-7322 | - |
crisitem.author.orcid | 0000-0001-5116-6789 | - |
crisitem.author.orcid | 0000-0002-7349-1109 | - |
crisitem.author.orcid | 0000-0001-5355-7388 | - |
crisitem.author.orcid | 0000-0001-7164-1508 | - |
crisitem.author.orcid | 0000-0001-5876-9259 | - |
crisitem.author.orcid | 0000-0001-9695-8472 | - |
crisitem.author.orcid | 0000-0003-3259-7801 | - |
crisitem.author.orcid | 0000-0002-8685-583x | - |
crisitem.author.orcid | 0000-0002-8875-5453 | - |
crisitem.author.orcid | 0000-0002-6813-0632 | - |
crisitem.journal.journalissn | 0922-6435 | - |
crisitem.journal.ance | E061604 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
Ciolfi2021_Article_Multi-messengerAstrophysicsWit.pdf | Pdf editoriale | 2.44 MB | Adobe PDF | View/Open |
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