Future Perspectives for Gamma-ray Burst Detection from Space

作     者：Bozzo, Enrico Amati, Lorenzo Baumgartner, Wayne Chang, Tzu-Ching Cordier, Bertrand De Angelis, Nicolas Doi, Akihiro Feroci, Marco Froning, Cynthia Gaskin, Jessica Goldstein, Adam Götz, Diego Grove, Jon E. Guiriec, Sylvain Hernanz, Margarita Michelle Hui, C. Jenke, Peter Kocevski, Daniel Kole, Merlin Kouveliotou, Chryssa Maccarone, Thomas McConnell, Mark L. Matsuhara, Hideo O’Brien, Paul Produit, Nicolas Ray, Paul S. Roming, Peter Santangelo, Andrea Seiffert, Michael Sun, Hui van der Horst, Alexander Veres, Peter Wei, Jianyan White, Nicholas Wilson-Hodge, Colleen Yonetoku, Daisuke Yuan, Weimin Zhang, Shuang-Nan 

作者机构：INAF-OAS Bologna via P. Gobetti 93/3 Bologna40129 Italy NASA Marshall Space Flight Center HuntsvilleAL35812 United States Jet Propulsion Lab 4800 Oak Grove Dr PasadenaCA91109 United States INAF-IAPS Roma via del Fosso del Cavaliere 100 RomaI-00133 Italy DPNC University of Geneva quai Ernest-Ansermet 24 Geneva1205 Switzerland Space Science Division U.S. Naval Research Laboratory WashingtonDC20375 United States Department of Astronomy University of Geneva Chemin d’Ecogia 16 Versoix1290 Switzerland IRFU Département d’Astrophysique CEA Université Paris-Saclay Gif-sur-YvetteF-91191 France Science and Technology Institute Universities Space Research Association HuntsvilleAL35805 United States  3-1-1 Yoshinodai Chuo-ku Sagamihara Kanagawa229-8510 Japan Southwest Research Institute Space Science and Engineering Division 6220 Culebra Road San AntonioTX78238 United States Department of Physics George Washington University Corcoran Hall 725 21st Street NW WashingtonDC20052 United States  Campus UAB Carrer de can Magrans s/n Bellaterra Barcelona08193 Spain  Barcelona Spain University of Alabama in Huntsville HuntsvilleAL35805 United States Department of Physics & Astronomy Texas Tech University Box 41051 LubbockTX79409-1051 United States Space Science Center University of New Hampshire DurhamNH03824 United States Department of Earth Oceans and Space Southwest Research Institute DurhamNH03824 United States School of Physics and Astronomy University of Leicester LeicesterLE1 7RH United Kingdom Institut für Astronomie und Astrophysik Kepler Center for Astro and Particle Physics Eberhard Karls Universität Sand 1 TübingenD-72076 Germany National Astronomical Observatories Chinese Academy of Sciences Beijing100101 China College of Science and Engineering School of Mathematics and Physics Kanazawa University Kakuma Ishikawa Kanazawa920-1192 Japan University of Chinese Academy of Sciences Chinese Academy of Sciences Beijing100049 China Key Laboratory of Particle Astrophysics Institute of High Energy Physics Chinese Academy of Sciences Beijing100049 China University of Chinese Academy of Sciences Chinese Academy of Sciences Beijing100049 China 

出 版 物：《arXiv》 (arXiv)

年 卷 期：2024年

核心收录：

主　　题：Gamma rays 

摘      要：Since their first discovery in the late 1960s, Gamma-ray bursts have attracted an exponentially growing interest from the international community due to their central role in the most highly debated open questions of the modern research of astronomy, astrophysics, cosmology, and fundamental physics. These range from the intimate nuclear composition of high density material within the core of ultra-dense neuron stars, to stellar evolution via the collapse of massive stars, the production and propagation of gravitational waves, as well as the exploration of the early Universe by unveiling first stars and galaxies (assessing also their evolution and cosmic re-ionization). GRBs have stimulated in the past ∼50 years the development of cutting-edge technological instruments for observations of high energy celestial sources from space, leading to the launch and successful operations of many different scientific missions (several of them still in data taking mode nowadays). In this review, we provide a brief description of the GRB-dedicated missions from space being designed and developed for the future. The list of these projects, not meant to be exhaustive, shall serve as a reference to interested readers to understand what is likely to come next to lead the further development of GRB research and associated phenomenology. © 2024, CC BY.