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We simulate the first minutes of the evolution of a binary-driven hypernova (BdHN) event, with a special focus on the associated accretion processes of supernova (SN) ejecta onto the newborn neutron star ($\nu$NS) and the NS companion.
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C. Breu and L. Rezzolla, MNRAS 459
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B. Zhang, The Physics of Gamma-Ray Bursts (2018)
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L. Becerra, M. M. Guzzo, F. Rossi-Torres, J. A. Rueda, R. Ruffini, and J. D. Uribe, ApJ 852
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L. Becerra, C. L. Ellinger, C. L. Fryer, J. A. Rueda, and R. Ruffini, ApJ 871
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Y. Wang, J. A. Rueda, R. Ruffini, L. Becerra, C. Bianco, L. Becerra, L. Li, and M. Karlica, ApJ 874
2019
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2019
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2019
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2021
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J. A. Rueda, R. Ruffini, R. Moradi, and Y. Wang, International Journal of Modern Physics D 30
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J. A. Rueda, Astronomy Reports 65
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2022
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2022
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2022
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