Multi-messenger astrophysics with THESEUS in the 2030s

Experimental Astronomy - Tập 52 - Trang 245-275 - 2021
Riccardo Ciolfi1,2, Giulia Stratta3,4, Marica Branchesi5,6, Bruce Gendre7, Stefan Grimm5,8, Jan Harms5,6, Gavin Paul Lamb9, Antonio Martin-Carrillo10, Ayden McCann7, Gor Oganesyan5,6, Eliana Palazzi11, Samuele Ronchini5,6, Andrea Rossi11, Om Sharan Salafia12,13, Lana Salmon10, Stefano Ascenzi14,15, Antonio Capone16,17, Silvia Celli16,17, Simone Dall’Osso5, Irene Di Palma16,17, Michela Fasano16,17, Paolo Fermani16,17, Dafne Guetta18, Lorraine Hanlon10, Eric Howell7, Stephane Paltani19, Luciano Rezzolla20,21,22, Serena Vinciguerra23, Angela Zegarelli16,17, Lorenzo Amati11, Andrew Blain9, Enrico Bozzo19, Sylvain Chaty24,25, Paolo D’Avanzo12,13, fnmMassimiliano De Pasquale26, Hüsne Dereli-Bégué27,28, Giancarlo Ghirlanda12,13, Andreja Gomboc29, Diego Götz30, Istvan Horvath31, Rene Hudec32,33,34, Luca Izzo35, Emeric Le Floch36, Liang Li37, Francesco Longo38,39,40, S. Komossa41, Albert K. H. Kong42, Sandro Mereghetti43, Roberto Mignani43,44, Antonios Nathanail45, Paul T. O’Brien9, Julian P. Osborne9, Asaf Pe’er28, Silvia Piranomonte46, Piero Rosati47, Sandra Savaglio48, Fabian Schüssler49, Olga Sergijenko50,51, Lijing Shao52,53, Nial Tanvir9, Sara Turriziani54, Yuji Urata55, Maurice van Putten56,7, Susanna Vergani57, Silvia Zane58, Bing Zhang59
1INAF, Osservatorio Astronomico di Padova, Padova, Italy
2INFN Sezione di Padova, Padova, Italy
3INAF, Osservatorio di Astrofisica e Scienza dello Spazio, Bologna, Italy
4INFN Sezione di Firenze, Firenze, Italy
5Gran Sasso Science Institute, L’Aquila (AQ), Italy
6INFN Laboratori Nazionali del Gran Sasso, Assergi, Italy
7OzGrav-UWA, University of Western Australia, Crawley, Australia
8INFN - Laboratori Nazionali del Gran Sasso, Assergi, Italy
9School of Physics and Astronomy, University of Leicester, Leicester, UK
10School of Physics and Centre for Space Research, University College Dublin, Dublin 4, Ireland
11INAF-Osservatorio di Astrofisica e Scienza dello Spazio, Bologna, Italy
12INAF-Osservatorio Astronomico di Brera, Merate, Italy
13INFN Sezione di Milano-Bicocca, Milano, Italy
14Institute of Space Sciences (ICE, CSIC) Campus UAB, Barcelona, Spain
15Institut d’Estudis Espacials de Catalunya (IEEC), Barcelona, Spain
16Dipartimento di Fisica dell’Università “La Sapienza”, Rome, Italy
17INFN Sezione di Roma, Rome, Italy
18ORT-Braude College, Carmiel, Israel
19Department of Astronomy, University of Geneva, Versoix, Switzerland
20Institut für Theoretische Physik, Frankfurt, Germany
21Frankfurt Institute for Advanced Studies, Frankfurt, Germany
22School of Mathematics, Trinity College, Dublin 2, Ireland
23Anton Pannekoek Institute for Astronomy, University of Amsterdam, Amsterdam, Netherlands
24CEA, CNRS, AIM, Université de Paris and Université Paris Saclay, Gif-sur-Yvette, France
25CNRS, AstroParticule et Cosmologie, Université de Paris, Paris, France
26Department of Astronomy and Space Sciences, Istanbul University, Istanbul, Turkey
27Max Planck Institute for Extraterrestrial Physics, Garching, Germany
28Department of Physics, Bar-Ilan University, 52900, Israel
29Center for Astrophysics and Cosmology, University of Nova Gorica, Nova Gorica, Slovenia
30AIM-CEA/DRF/Irfu/Département d’Astrophysique, CNRS, Université Paris-Saclay, Université de Paris, Gif-sur-Yvette, France
31University of Public Service, Budapest, Hungary
32Faculty of Electrical Engineering, Czech Technical University in Prague, Prague, Czech Republic
33Astronomical Institute, Czech Academy of Sciences, Ondrejov, Czech Republic
34Kazan Federal University, Kazan, Russian Federation
35DARK, Niels Bohr Institute, University of Copenhagen, Copenhagen, Denmark
36Laboratoire AIM, CEA/DSM/IRFU, CNRS, Université Paris-Diderot, Gif-sur-Yvette, France
37ICRANet, Pescara, Italy
38Università degli studi di Trieste, Trieste, Italy
39INFN Sezione di Trieste, Trieste, Italy
40Institute for Fundamental Physics of the Universe (IFPU), Trieste, Italy
41Max-Planck Institut für Radioastronomie, Bonn, Germany
42Institute of Astronomy, National Tsing Hua University, 30013, Taiwan
43INAF-Istituto di Astrofisica Spaziale e Fisica cosmica, Milano, Italy
44Janusz Gil Institute of Astronomy, University of Zielona Góra, Zielona Góra, Poland
45Department of Physics, National and Kapodistrian University of Athens, Zografos, Greece
46INAF, Osservatorio Astronomico di Roma, Monte Porzio Catone (RM), Italy
47Department of Physics and Earth Sciences, University of Ferrara, Ferrara, Italy
48Physics Department, University of Calabria, Rende, Italy
49IRFU, CEA, Université Paris-Saclay, Gif-sur-Yvette, France
50Astronomical Observatory of Taras Shevchenko, National University of Kyiv, Kyiv, Ukraine
51Main Astronomical Observatory of the National Academy of Sciences of Ukraine, Kyiv, Ukraine
52Kavli Institute for Astronomy and Astrophysics, Peking University, Beijing, China
53National Astronomical Observatories, Chinese Academy of Sciences, Beijing, China
54Physics Department, Gubkin Russian State University, Moscow, Russian Federation
55Institute of Astronomy, National Central University, Chung-Li, Taiwan
56Physics and Astronomy, Sejong University, Seoul, Korea
57CNRS, GEPI, Observatoire de Paris, PSL University, Meudon, France
58Mullards Space Science Laboratory, University College London, Surrey, UK
59Department of Physics and Astronomy, University of Nevada Las Vegas, Las Vegas, USA

Tóm tắt

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.

Tài liệu tham khảo

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