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,… 展开作者
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, 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
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.
Deep Learning for Multi-Messenger Astrophysics: A Gateway for Discovery in the Big Data Era
NCSA, University of Illinois at Urbana-Champaign（伊利诺伊大学厄巴纳-香槟分校国家超级计算应用中心）；Department of Astronomy, University of Illinois at Urbana-Champaign（伊利诺伊大学厄巴纳-香槟分校天文学系）；California Institute of Technology（加州理工学院）；Las Cumbres Observatory（拉斯坎布雷斯天文台）；Caltech/IPAC-NExScI（加州理工学院/红外处理与分析中心-系外行星科学研究所）；Department of Physics and Astronomy, University of Delaware（特拉华大学物理与天文学系）；Data Science Institute, University of Delaware（特拉华大学数据科学研究所）；Center for Urban Science and Progress, New York University（纽约大学城市科学与进步中心）；The Oskar Klein Centre for Cosmoparticle Physics, Stockholm University（斯德哥尔摩大学奥斯卡·克莱因宇宙粒子物理中心）；The University of Chicago（芝加哥大学）；IBM Systems（IBM系统部）
Enabling real-time multi-messenger astrophysics discoveries with deep learning
University of Illinois at Urbana-Champaign（伊利诺伊大学厄巴纳-香槟分校）；California Institute of Technology（加州理工学院）；Tecnologico de Monterrey（蒙特雷理工学院）；Las Cumbres Observatory（拉斯坎布雷斯天文台）；University of Delaware（特拉华大学）；Stockholm University（斯德哥尔摩大学）；The University of Chicago（芝加哥大学）；IBM T.J. Watson Research Center（IBM托马斯·J·沃森研究中心）；Carnegie Institute for Science（卡内基科学研究所）；West Virginia University（西弗吉尼亚大学）
LUMOS : Linear programming Utility for Multi-messenger Optical Scheduling
Astrophysics Research Institute, Liverpool John Moores University（利物浦约翰摩尔斯大学天体物理研究所）；Department of Physics, Indian Institute of Technology Bombay（印度理工学院孟买分校物理系）；School of Physics and Astronomy, University of Minnesota（明尼苏达大学物理与天文学学院）；Astrophysics Science Division, NASA Goddard Space Flight Center（NASA戈达德太空飞行中心天体物理学科学部）；Joint Space-Science Institute, University of Maryland（马里兰大学联合空间科学研究所）
Observational strategies for ultrahigh-energy neutrinos: the importance of deep sensitivity for detection and astronomy
Sorbonne Université（索邦大学）；CNRS（法国国家科学研究中心）；Institut d’Astrophysique de Paris（巴黎天体物理研究所）；Vrije Universiteit Brussels（布鲁塞尔自由大学）；The Pennsylvania State University（宾夕法尼亚州立大学）；Universite Paris Diderot（巴黎第七大学）；Laboratoire de Physique Nucleaire et de Hautes Energies（核物理与高能物理实验室）；Center for Multimessenger Astrophysics（多信使天文学中心）；Institute for Gravitation and the Cosmos（引力与宇宙研究所）
A Multi-Messenger Search for Exotic Field Emission with a Global Magnetometer Network
University of California, Los Angeles（加州大学洛杉矶分校）；Bucknell University（巴克内尔大学）；Helmholtz Institute Mainz（美因茨亥姆霍兹研究所）；GSI Helmholtzzentrum für Schwerionenforschung GmbH（德国重离子研究中心有限公司）；Australian National University（澳大利亚国立大学）；University of California, Berkeley（加州大学伯克利分校）；Ben-Gurion University of the Negev（内盖夫本-古里安大学）；University of Belgrade（贝尔格莱德大学）；Peking University（北京大学）；The Australian National University（澳大利亚国立大学）；California State University -- East Bay（东湾州立大学）；IBS（韩国基础科学研究院）；KAIST（韩国科学技术院）；Messiah University（救主大学）；Friedrich Schiller University Jena（耶拿弗里德里希·席勒大学）；Jagiellonian University in Krakow（克拉科夫雅盖隆大学）；Oberlin College（欧柏林学院）；University of Minnesota（明尼苏达大学）；Hebrew University of Jerusalem（耶路撒冷希伯来大学）；Leibniz Institute of Photonic Technology（莱布尼茨光子技术研究所）；University of Fribourg（弗里堡大学）
An agentic framework for gravitational-wave counterpart association in the multi-messenger era
Department of Astronomy, School of Physics（天文学系，物理系）；Kavli Institute for Astronomy and Astrophysics（天体物理研究所）；Institute for Gravitational Wave Astronomy（引力波天文研究所）；School of Information Science and Technology（信息科学与技术学院）；National Astronomical Observatories（国家天文台）
