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

Department of Physics - at Bar-Ilan University

Research output: Contribution to journal › Article › peer-review

18 Scopus citations

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
State	Published - Dec 2021

Bibliographical note

Publisher Copyright:
© 2021, The Author(s).

Funding

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. Open access funding provided by Istituto Nazionale di Astrofisica within the CRUI-CARE Agreement.

Funders	Funder number
EU AHEAD2020
Horizon 2020 Framework Programme	CE170100004, 871158
Australian Research Council	DE170100891
Science Foundation Ireland	19/FFP/6777
Irish Research Council	GOIPG/2017/1525
Agenzia Spaziale Italiana	I/004/11/4, 20179ZF5KS
Türkiye Bilimsel ve Teknolojik Araştirma Kurumu	MFAG-119F073
Istituto Nazionale di Astrofisica

Keywords

Compact binary merger
Gamma-ray burst
Kilonova
Multi-messenger astrophysics
Neutrino sources
X-ray sources

Access to Document

10.1007/s10686-021-09795-9

Cite this

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

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

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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

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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

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

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SN - 0922-6435

VL - 52

SP - 245

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Multi-messenger astrophysics with THESEUS in the 2030s

Abstract

Bibliographical note

Funding

Keywords

Access to Document

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