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An Update of the Binary-Driven Hypernovae Scenario of Long Gamma-Ray Bursts

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Abstract

I discuss some most recent theoretical and observational results on the inner engine of the high-energy (GeV) emission of long gamma-ray bursts (GRBs), within the context of the binary-driven hypernova (BdHN) model.

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Authors and Affiliations

  1. ICRANet, I-65122, Pescara, Italy

    J. A. Rueda

  2. ICRA, Dipartimento di Fisica, Sapienza Università di Roma, I-00185, Rome, Italy

    J. A. Rueda

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

    J. A. Rueda

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

    J. A. Rueda

  5. INAF, Istituto di Astrofisica e Planetologia Spaziali, 00133, Rome, Italy

    J. A. Rueda

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  1. J. A. Rueda
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Correspondence to J. A. Rueda.

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Paper presented at the Fourth Zeldovich meeting, an international conference in honor of Ya.B. Zeldovich held in Minsk, Belarus, on September 7–11, 2020. Published by the recommendation of the special editors: S.Ya. Kilin, R. Ruffini, and G.V. Vereshchagin.

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Rueda, J.A. An Update of the Binary-Driven Hypernovae Scenario of Long Gamma-Ray Bursts. Astron. Rep. 65, 1026–1029 (2021). https://doi.org/10.1134/S1063772921100309

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  • DOI: https://doi.org/10.1134/S1063772921100309

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