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GRB-SN Association within the Binary-Driven Hypernova Model

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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.

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Funding

This work was supported by ongoing institutional funding. No additional grants to carry out or direct this particular research were obtained.

Author information

Authors and Affiliations

  1. Fesenkov Astrophysical Institute, Observatory 23, 050020, Almaty, Kazakhstan

    Y. Aimuratov

  2. ICRANet, Piazza della Repubblica 10, I-65122, Pescara, Italy

    Y. Aimuratov, L. M. Becerra, C. L. Bianco, C. Cherubini, M. Della Valle, S. Filippi, Liang Li, R. Moradi, F. Rastegarnia, J. A. Rueda, R. Ruffini, N. Sahakyan, Y. Wang & S. R. Zhang

  3. Escuela de F´ısica, Universidad Industrial de Santander, A.A.678, 680002, Bucaramanga, Colombia

    L. M. Becerra

  4. ICRA, Dipartamento di Fisica, Sapienza Università di Roma, I-00185, Rome, Italy

    C. L. Bianco, Liang Li, R. Moradi, J. A. Rueda, R. Ruffini & Y. Wang

  5. Universit´e de Nice Sophia-Antipolis, Grand Château Parc Valrose, Nice, CEDEX 2, France

    C. L. Bianco & R. Ruffini

  6. INAF, Istituto di Astrofisica e Planetologia Spaziali, I-00133, Rome, Italy

    C. L. Bianco & J. A. Rueda

  7. ICRA, University Campus Bio-Medico of Rome, I-00128, Rome, Italy

    C. Cherubini & S. Filippi

  8. Department of Science and Technology for Sustainable Development and One Health, Università Campus Bio-Medico di Roma, 21-I-00128, Rome, Italy

    C. Cherubini

  9. INAF, Osservatorio Astronomico di Capodimonte, I-80131, Napoli, Italy

    M. Della Valle

  10. Department of Engineering, Università Campus Bio-Medico di Roma, 21-I-00128, Rome, Italy

    S. Filippi

  11. INAF, Osservatorio Astronomico d’Abruzzo, I-64100, Teramo, Italy

    Liang Li, R. Moradi & Y. Wang

  12. School of Mathematics and Physics, University of South China, 421001, Hengyang, China

    Wenbin Lin

  13. Department of Physics, Faculty of Physics and Chemistry, Alzahra University, Tehran, Iran

    F. Rastegarnia

  14. ICRANet-Ferrara, Dip. di Fisica e Scienze della Terra, Università degli Studi di Ferrara, I-44122, Ferrara, Italy

    J. A. Rueda & S. R. Zhang

  15. Dipartamento di Fisica e Scienze della Terra, Università degli Studi di Ferrara, I-44122, Ferrara, Italy

    J. A. Rueda

  16. INAF, I-00136, Rome, Italy

    R. Ruffini

  17. ICRANet-Armenia, 0019, Yerevan, Armenia

    N. Sahakyan

  18. School of Astronomy and Space Science, University of Science and Technology of China, 230026, Hefei, China

    S. R. Zhang

  19. CAS Key Laboratory for Research in Galaxies and Cosmology, Department of Astronomy, University of Science and Technology of China, 230026, Hefei, China

    S. R. Zhang

Authors
  1. Y. Aimuratov
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  2. L. M. Becerra
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  3. C. L. Bianco
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  4. C. Cherubini
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  5. M. Della Valle
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  6. S. Filippi
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  7. Liang Li
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  8. Wenbin Lin
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  9. R. Moradi
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  10. F. Rastegarnia
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  11. J. A. Rueda
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  12. R. Ruffini
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  13. N. Sahakyan
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  14. Y. Wang
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  15. S. R. Zhang
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Corresponding authors

Correspondence to R. Moradi, J. A. Rueda or R. Ruffini.

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Paper presented at the Fifth Zeldovich meeting, an international conference in honor of Ya.B. Zeldovich held in Yerevan, Armenia on June 12–16, 2023. Published by the recommendation of the special editors: R. Ruffini, N. Sahakyan and G.V. Vereshchagin.

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Aimuratov, Y., Becerra, L.M., Bianco, C.L. et al. GRB-SN Association within the Binary-Driven Hypernova Model. Astron. Rep. 67 (Suppl 2), S87–S92 (2023). https://doi.org/10.1134/S1063772923140020

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