Multi-messenger astrophysics with THESEUS in the 2030s

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

doi:10.1007/s10686-021-09795-9

Multi-messenger astrophysics with THESEUS in the 2030s

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

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19 Citations (Scopus)

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.

Original language	English
Pages (from-to)	245-275
Number of pages	31
Journal	Experimental Astronomy
Volume	52
Issue number	3
DOIs	https://doi.org/10.1007/s10686-021-09795-9
Publication status	Published - Dec 2021

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10.1007/s10686-021-09795-9Licence: CC BY

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Ciolfi, R., Stratta, G., Branchesi, M., Gendre, B., Grimm, S., Harms, J., Lamb, G. P., Martin-Carrillo, A., McCann, A., Oganesyan, G., Palazzi, E., Ronchini, S., Rossi, A., Salafia, O. S., Salmon, L., Ascenzi, S., Capone, A., Celli, S., Dall’Osso, S., ... Zhang, B. (2021). Multi-messenger astrophysics with THESEUS in the 2030s. Experimental Astronomy, 52(3), 245-275. https://doi.org/10.1007/s10686-021-09795-9

@article{2d5be9c2b79d4283832687cde6a4e8d0,

title = "Multi-messenger astrophysics with THESEUS in the 2030s",

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.",

keywords = "Compact binary merger, Gamma-ray burst, Kilonova, Multi-messenger astrophysics, Neutrino sources, X-ray sources",

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

note = "Funding Information: We acknowledge support from the ASI-INAF agreement n. 2018-29-HH.0. MB and RH acknowledge the support of the European Union{\textquoteright}s Horizon 2020 Programme under the AHEAD2020 Project grant agreement 871158. Part of this research was conducted by the Australian Research Council Centre of Excellence for Gravitational Wave Discovery (OzGrav), through project number CE170100004. EH also acknowledges support from an Australian Research Council DECRA Fellowship (DE170100891). AR acknowledges support from the project Supporto Arizona & Italia. LSal acknowledges support from the Irish Research Council under grant GOIPG/2017/1525. LH acknowledges support from Science Foundation Ireland under grant 19/FFP/6777 and from the EU AHEAD2020 project (grant agreement 871158). PDA acknowledges funding from the Italian Space Agency, contract ASI/INAF n. I/004/11/4. MB, PDA, and EP acknowledge support from PRIN-MIUR 2017 (grant 20179ZF5KS). MDP acknowledges support for this work by the Scientific and Technological Research Council of Turkey (T{\"U}BITAK), Grant No: MFAG-119F073. Funding Information: Open access funding provided by Istituto Nazionale di Astrofisica within the CRUI-CARE Agreement. Publisher Copyright: {\textcopyright} 2021, The Author(s).",

year = "2021",

month = dec,

doi = "10.1007/s10686-021-09795-9",

language = "English",

volume = "52",

pages = "245--275",

journal = "Experimental Astronomy",

issn = "0922-6435",

publisher = "Springer",

number = "3",

}

Ciolfi, R, Stratta, G, Branchesi, M, Gendre, B, Grimm, S, Harms, J, Lamb, GP, Martin-Carrillo, A, McCann, A, Oganesyan, G, Palazzi, E, Ronchini, S, Rossi, A, Salafia, OS, Salmon, L, Ascenzi, S, Capone, A, Celli, S, Dall’Osso, S, Di Palma, I, Fasano, M, Fermani, P, Guetta, D, Hanlon, L, Howell, E, Paltani, S, Rezzolla, L, Vinciguerra, S, Zegarelli, A, Amati, L, Blain, A, Bozzo, E, Chaty, S, D’Avanzo, P, De Pasquale, FM, Dereli-Bégué, H, Ghirlanda, G, Gomboc, A, Götz, D, Horvath, I, Hudec, R, Izzo, L, Le Floch, E, Li, L, Longo, F, Komossa, S, Kong, AKH, Mereghetti, S, Mignani, R, Nathanail, A, O’Brien, PT, Osborne, JP, Pe’er, A, Piranomonte, S, Rosati, P, Savaglio, S, Schüssler, F, Sergijenko, O, Shao, L, Tanvir, N, Turriziani, S, Urata, Y, van Putten, M, Vergani, S, Zane, S & Zhang, B 2021, 'Multi-messenger astrophysics with THESEUS in the 2030s', Experimental Astronomy, vol. 52, no. 3, pp. 245-275. https://doi.org/10.1007/s10686-021-09795-9

TY - JOUR

T1 - Multi-messenger astrophysics with THESEUS in the 2030s

AU - Ciolfi, Riccardo

AU - Stratta, Giulia

AU - Branchesi, Marica

AU - Gendre, Bruce

AU - Grimm, Stefan

AU - Harms, Jan

AU - Lamb, Gavin Paul

AU - Martin-Carrillo, Antonio

AU - McCann, Ayden

AU - Oganesyan, Gor

AU - Palazzi, Eliana

AU - Ronchini, Samuele

AU - Rossi, Andrea

AU - Salafia, Om Sharan

AU - Salmon, Lana

AU - Ascenzi, Stefano

AU - Capone, Antonio

AU - Celli, Silvia

AU - Dall’Osso, Simone

AU - Di Palma, Irene

AU - Fasano, Michela

AU - Fermani, Paolo

AU - Guetta, Dafne

AU - Hanlon, Lorraine

AU - Howell, Eric

AU - Paltani, Stephane

AU - Rezzolla, Luciano

AU - Vinciguerra, Serena

AU - Zegarelli, Angela

AU - Amati, Lorenzo

AU - Blain, Andrew

AU - Bozzo, Enrico

AU - Chaty, Sylvain

AU - D’Avanzo, Paolo

AU - De Pasquale, fnm Massimiliano

AU - Dereli-Bégué, Hüsne

AU - Ghirlanda, Giancarlo

AU - Gomboc, Andreja

AU - Götz, Diego

AU - Horvath, Istvan

AU - Hudec, Rene

AU - Izzo, Luca

AU - Le Floch, Emeric

AU - Li, Liang

AU - Longo, Francesco

AU - Komossa, S.

AU - Kong, Albert K.H.

AU - Mereghetti, Sandro

AU - Mignani, Roberto

AU - Nathanail, Antonios

AU - O’Brien, Paul T.

AU - Osborne, Julian P.

AU - Pe’er, Asaf

AU - Piranomonte, Silvia

AU - Rosati, Piero

AU - Savaglio, Sandra

AU - Schüssler, Fabian

AU - Sergijenko, Olga

AU - Shao, Lijing

AU - Tanvir, Nial

AU - Turriziani, Sara

AU - Urata, Yuji

AU - van Putten, Maurice

AU - Vergani, Susanna

AU - Zane, Silvia

AU - Zhang, Bing

N1 - Funding Information: We acknowledge support from the ASI-INAF agreement n. 2018-29-HH.0. MB and RH acknowledge the support of the European Union’s Horizon 2020 Programme under the AHEAD2020 Project grant agreement 871158. Part of this research was conducted by the Australian Research Council Centre of Excellence for Gravitational Wave Discovery (OzGrav), through project number CE170100004. EH also acknowledges support from an Australian Research Council DECRA Fellowship (DE170100891). AR acknowledges support from the project Supporto Arizona & Italia. LSal acknowledges support from the Irish Research Council under grant GOIPG/2017/1525. LH acknowledges support from Science Foundation Ireland under grant 19/FFP/6777 and from the EU AHEAD2020 project (grant agreement 871158). PDA acknowledges funding from the Italian Space Agency, contract ASI/INAF n. I/004/11/4. MB, PDA, and EP acknowledge support from PRIN-MIUR 2017 (grant 20179ZF5KS). MDP acknowledges support for this work by the Scientific and Technological Research Council of Turkey (TÜBITAK), Grant No: MFAG-119F073. Funding Information: Open access funding provided by Istituto Nazionale di Astrofisica within the CRUI-CARE Agreement. Publisher Copyright: © 2021, The Author(s).

PY - 2021/12

Y1 - 2021/12

N2 - 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.

AB - 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.

KW - Compact binary merger

KW - Gamma-ray burst

KW - Kilonova

KW - Multi-messenger astrophysics

KW - Neutrino sources

KW - X-ray sources

UR - http://www.scopus.com/inward/record.url?scp=85117111956&partnerID=8YFLogxK

U2 - 10.1007/s10686-021-09795-9

DO - 10.1007/s10686-021-09795-9

M3 - Article

AN - SCOPUS:85117111956

SN - 0922-6435

VL - 52

SP - 245

EP - 275

JO - Experimental Astronomy

JF - Experimental Astronomy

IS - 3

ER -

Multi-messenger astrophysics with THESEUS in the 2030s

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Probing cosmic transients through gravitational wave observations

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Multi-messenger astrophysics with THESEUS in the 2030s

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