GRB-SN Association within the Binary-Driven Hypernova Model
Aimuratov Y. Becerra L.M. Bianco C.L. Cherubini C. Della Valle M. Filippi S. Li L. Lin W. Moradi R. Rastegarnia F. Rueda J.A. Ruffini R. Sahakyan N. Wang Y. Zhang S.R.
December 2023Pleiades Publishing
Astronomy Reports
2023#67Issue Suppl 2S87 - S92 pp.
Abstract: Long gamma-ray bursts (GRBs), in a few seconds, release luminosities (in gamma-rays) comparable to the luminosity of all stars in the observable Universe, which makes them detectable to the dawn of galaxy and stellar formation. One of the most striking observational properties of some of these sources is that they are accompanied by a supernova (SN) of type Ic, traditionally called GRB-SN association or connection. The GRB-SN association, probably the most constraining property of GRB theoretical models, is the subject of this article.
gamma-ray bursts
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Fesenkov Astrophysical Institute, Observatory 23, Almaty, 050020, Kazakhstan
ICRANet, Piazza della Repubblica 10, Pescara, I-65122, Italy
Escuela de F´ısica, Universidad Industrial de Santander, A.A.678, Bucaramanga, 680002, Colombia
ICRA, Dipartamento di Fisica, Sapienza Università di Roma, Rome, I-00185, Italy
Universit´e de Nice Sophia-Antipolis, Grand Château Parc Valrose, CEDEX 2, Nice, France
INAF, Istituto di Astrofisica e Planetologia Spaziali, Rome, I-00133, Italy
ICRA, University Campus Bio-Medico of Rome, Rome, I-00128, Italy
Department of Science and Technology for Sustainable Development and One Health, Università Campus Bio-Medico di Roma, Rome, 21-I-00128, Italy
INAF, Osservatorio Astronomico di Capodimonte, Napoli, I-80131, Italy
Department of Engineering, Università Campus Bio-Medico di Roma, Rome, 21-I-00128, Italy
INAF, Osservatorio Astronomico d’Abruzzo, Teramo, I-64100, Italy
School of Mathematics and Physics, University of South China, Hengyang, 421001, China
Department of Physics, Faculty of Physics and Chemistry, Alzahra University, Tehran, Iran
ICRANet-Ferrara, Dip. di Fisica e Scienze della Terra, Università degli Studi di Ferrara, Ferrara, I-44122, Italy
Dipartamento di Fisica e Scienze della Terra, Università degli Studi di Ferrara, Ferrara, I-44122, Italy
INAF, Rome, I-00136, Italy
ICRANet-Armenia, Yerevan, 0019, Armenia
School of Astronomy and Space Science, University of Science and Technology of China, Hefei, 230026, China
CAS Key Laboratory for Research in Galaxies and Cosmology, Department of Astronomy, University of Science and Technology of China, Hefei, 230026, China
Fesenkov Astrophysical Institute
ICRANet
Escuela de F´ısica
ICRA
Universit´e de Nice Sophia-Antipolis
INAF
ICRA
Department of Science and Technology for Sustainable Development and One Health
INAF
Department of Engineering
INAF
School of Mathematics and Physics
Department of Physics
ICRANet-Ferrara
Dipartamento di Fisica e Scienze della Terra
INAF
ICRANet-Armenia
School of Astronomy and Space Science
CAS Key Laboratory for Research in Galaxies and Cosmology
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