THESEUS: A key space mission concept for Multi-Messenger Astrophysics

被引：63

作者：

Stratta, G. ^{[1
,2
]}

Ciolfi, R. ^{[3
,4
]}

Amati, L. ^{[2
]}

Bozzo, E. ^{[5
]}

Ghirlanda, G. ^{[6
]}

Maiorano, E. ^{[2
]}

Nicastro, L. ^{[2
]}

Rossi, A. ^{[2
]}

Vinciguerra, S. ^{[7
,8
]}

Frontera, F. ^{[2
,9
]}

Gotz, D. ^{[10
]}

Guidorzi, C. ^{[9
]}

O'Brien, P. ^{[11
]}

Osborne, J. P. ^{[11
]}

Tanvir, N. ^{[12
,13
]}

Branchesi, M. ^{[14
,15
]}

Brocato, E. ^{[26
]}

Dainotti, M. G. ^{[2
,16
,52
]}

De Pasquale, M. ^{[17
]}

Grado, A. ^{[18
]}

Greiner, J. ^{[19
]}

Longo, F. ^{[20
,21
]}

Maio, U. ^{[22
,23
]}

Mereghetti, D. ^{[24
]}

Mignani, R. ^{[24
,25
]}

Piranomonte, S. ^{[26
]}

Rezzolla, L. ^{[27
,28
]}

Salvaterra, R. ^{[24
]}

Starling, R. ^{[11
]}

Willingale, R. ^{[11
]}

Boer, M. ^{[29
]}

Bulgarelli, A. ^{[2
]}

Caruana, J. ^{[30
,31
]}

Colafrancesco, S. ^{[32
]}

Colpi, M. ^{[33
,34
]}

Covino, S. ^{[6
]}

D'Avanzo, P. ^{[6
]}

D'Elia, V ^{[26
,35
]}

Drago, A. ^{[9
]}

Fuschino, F. ^{[2
]}

Gendre, B. ^{[36
,37
,38
]}

Hudec, R. ^{[39
,40
]}

Jonker, P. ^{[41
,42
]}

Labanti, C. ^{[2
]}

Malesani, D. ^{[43
]}

Mundell, C. G. ^{[44
]}

Palazzi, E. ^{[2
]}

Patricelli, B. ^{[45
]}

Razzano, M. ^{[45
]}

Campana, R. ^{[2
]}

机构：

[1] Univ Urbino, Dipartimento Sci Pure & Applicate, Via S Chiara 27, I-61029 Urbino, Italy

[2] INAF OAS Bologna, Via P Gobetti 9313, Bologna, Italy

[3] Osserv Astron Padova, INAF, Vicolo Osservatorio 5, I-35122 Padua, Italy

[4] Ist Nazl Fis Nucl, TIFPA, Via Sommarive 14, I-38123 Trento, Italy

[5] Univ Geneva, Dept Astron, Ch Ecogia 16, CH-1290 Versoix, Switzerland

[6] INAF Osservatorio Astron Brera, Via E Bianchi 46, I-23807 Merate, LC, Italy

[7] Univ Birmingham, Inst Gravitat Wave Astron, Birmingham B15 2TT, W Midlands, England

[8] Univ Birmingham, Sch Phys & Astron, Birmingham B15 2TT, W Midlands, England

[9] Univ Ferrara, Dept Phys & Earth Sci, Via Saragat 1, I-44122 Ferrara, Italy

[10] Univ Paris Saclay, CEA, IRFU, Dept Astrophys, F-91191 Gif Sur Yvette, France

[11] Univ Leicester, Dept Phys & Astron, Leicester LE1 7RH, Leics, England

[12] Univ Leicester, Dept Phys & Astron, Univ Rd, Leicester LE1 7RH, Leics, England

[13] Univ Leicester, Leicester Inst Space & Earth Observat, Univ Rd, Leicester LE1 7RH, Leics, England

[14] Ist Nazl Fis Nucl, Sez Firenze, Via G Sansone 1, I-50019 Sesto Fiorentino, Italy

[15] GSSI, Viale Francesco Crispi 7, I-67100 Laquila, Italy

[16] Stanford Univ, Dept Phys & Astron, Via Pueblo Mall 382, Stanford, CA 94305 USA

[17] Istanbul Univ, Dept Astron & Space Sci, TR-34119 Istanbul, Turkey

[18] INAF Capodimonte Astron Observ Naples, Via Moiariello 16, I-80131 Naples, Italy

[19] Max Planck Inst Astrophys, Karl Schwarzschild Str 1, D-85741 Garching, Germany

[20] Univ Trieste, Dept Phys, Via Valerio 2, Trieste, Italy

[21] INFN Trieste, Via Valerio 2, Trieste, Italy

[22] Leibniz Inst Astrophys, Sternwarte 16, D-14482 Potsdam, Germany

[23] INAF Osservatorio Astron Trieste, Via G Tiepolo 11, I-34131 Trieste, Italy

[24] INAF Ist Astrofis Spaziale & Fis Cosm Milano, Via E Bassini 15, I-20133 Milan, Italy

[25] Univ Zielona Gora, Janusz Gil Inst Astron, Lubuska 2, PL-65265 Zielona Gora, Poland

[26] INAF Osservatorio Astron Roma, Via Frascati 33, I-00040 Monte Porzio Catone, Italy

[27] Goethe Univ Frankfurt, Inst Theoret Phys, Max von Laue Str 1, D-60438 Frankfurt, Germany

[28] Frankfurt Inst Adv Studies, Ruth Moufang Str 1, D-60438 Frankfurt, Germany

[29] Univ Cote dAzur, CNRS UMR 5270, ARTEMIS, Observ Cote dAzur, Blvd Observ,CS 34229, F-06304 Nice 04, France

[30] Univ Malta, Dept Phys, Msida Msd 2080, Malta

[31] Univ Malta, Inst Space Sci & Astron, Msida Msd 2080, Malta

[32] Univ Witwatersrand, Sch Phys, Private Bag 3, ZA-2050 Johannesburg, South Africa

[33] Univ Milano Bicocca, Dipartimento Fis G Occhialini, Piazza Sci 3, I-20126 Milan, Italy

[34] Ist Nazl Fis Nucl, Sez Milano Bicocca, Piazza Sci 3, I-20126 Milan, Italy

[35] Agenzia Spaziale Italiana, SSDC, Via Politecn, I-100133 Rome, Italy

[36] Univ Western Australia, Sch Phys, M013, Crawley, WA 6009, Australia

[37] Univ Virgin Isl, 2 John Brewers Bay, St Thomas, VI 00802 USA

[38] Etelman Observ, Bonne Resolut, St Thomas, VI USA

[39] Czech Tech Univ, Fac Elect Engn, Prague 16627, Czech Republic

[40] Kazan Fed Univ, Kazan 420008, Russia

[41] SRON Netherlands Inst Space Res, SRON, Sorbonnelaan 2, NL-3584 CA Utrecht, Netherlands

[42] Radboud Univ Nijmegen, Dept Astrophys, IMAPP, POB 9010, NL-6500 GL Nijmegen, Netherlands

[43] Univ Copenhagen, Dark Cosmol Ctr, Niels Bohr Inst, Juliane Maries Vej 30, DK-2100 Copenhagen, Denmark

[44] Univ Bath, Dept Phys, Bath BA2 7AY, Avon, England

[45] Scuola Normale Super Pisa, Piazza Cavalieri 7, I-56126 Pisa, Italy

[46] Slovenian Ctr Excellence Space Sci & Technol, SPACE SI, Ljubljana, Slovenia

[47] Czech Acad Sci, Astron Inst, Fricova 298, Ondrejov 25165, Czech Republic

[48] Sejong Univ, 98 Gunja Dong, Seoul 143747, South Korea

[49] CNRS, Observ Paris, PSL Res Univ, GEPI, Pl Jules Janssen, F-92190 Meudon, France

[50] Univ Nevada, Dept Phys & Astron, Las Vegas, NV 89154 USA

来源：

ADVANCES IN SPACE RESEARCH | 2018年 / 62卷 / 03期

基金：

新加坡国家研究基金会;

关键词：

X-ray sources; X-ray bursts; Gamma-ray sources; Gamma-ray bursts; Astronomical and space-research instrumentation; GAMMA-RAY BURSTS; NEUTRON-STAR; ELECTROMAGNETIC COUNTERPART; GRAVITATIONAL-WAVES; EMISSION; SUPERNOVA; KILONOVA; MERGER; POPULATION; AFTERGLOW;

D O I：

10.1016/j.asr.2018.04.013

中图分类号：

V [航空、航天];

学科分类号：

08 ; 0825 ;

摘要：

The recent discovery of the electromagnetic counterpart of the gravitational wave source GW170817, has demonstrated the huge informative power of multi-messenger observations. During the next decade the nascent field of multi-messenger astronomy will mature significantly. Around 2030 and beyond, third generation ground-based gravitational wave detectors will be roughly ten times more sensitive than the current ones. At the same time, neutrino detectors currently upgrading to multi km(3) telescopes, will include a 10 km(3) facility in the Southern hemisphere. In this review, we describe the most promising sources of high frequency gravitational waves and neutrinos that will be detected in the next two decades. In this context, we show the important role of the Transient High Energy Sky and Early Universe Surveyor (THESEUS), a mission concept accepted by ESA for phase A study and proposed by a large international collaboration in response to the call for the Cosmic Vision Programme M5 missions. THESEUS aims at providing a substantial advancement in early Universe science as well as in multi-messenger and time-domain astrophysics, operating in strong synergy with future gravitational wave and neutrino detectors as well as major ground- and space-based telescopes. This review is an extension of the THESEUS white paper (Amati et al., 2017), also in light of the discovery of GW170817/GRB170817A that was announced on October 16th, 2017. (C) 2018 COSPAR. Published by Elsevier Ltd. All rights reserved.

引用

页码：662 / 682

页数：21

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