WebSep 28, 2024 · Binary-driven hypernova (BdHN) models long gamma-ray burst (GRB) as occurring in the binary systems involving a carbon–oxygen core (CO [Formula: see text]) and a companion neutron star (NS)... WebJul 9, 2015 · The induced gravitational collapse (IGC) paradigm addresses energetic (1052-1054 erg), long gamma-ray bursts (GRBs) associated to supernovae (SNe) and proposes as their progenitors tight binary systems composed of an evolved FeCO core and a companion neutron star (NS).
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WebDec 4, 2015 · Binary-driven hypernovae (BdHNe) within the induced gravitational collapse paradigm have been introduced to explain energetic (E iso ≳ 10 52 erg), long gamma-ray bursts (GRBs) associated with type Ic supernovae (SNe).The progenitor is a tight binary composed of a carbon-oxygen (CO) core and a neutron-star (NS) companion, a subclass … WebOct 1, 2024 · 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. theory of the solution of inventive problems
[2208.02725] GRB 171205A: Hypernova and Newborn …
WebINIS Repository Search provides online access to one of the world's largest collections on the peaceful uses of nuclear science and technology. The International Nuclear Information System is operated by the IAEA in collaboration with over 150 members. Web(Dated: March 28, 2024) We estimate the neutrino emission from the decay chain of the ˇ-meson and -lepton, produced by proton-proton inelastic scattering in energetic (E iso & 1052 erg) long gamma-ray bursts (GRBs), within the type I binary-driven hypernova (BdHN) model. The BdHN I progenitor is a binary system composed of a carbon-oxygen star (CO WebJul 9, 2015 · The induced gravitational collapse (IGC) paradigm addresses energetic (10 52-10 54 erg), long gamma-ray bursts (GRBs) associated to supernovae (SNe) and … shs102.ersp.biz/scripts/index.cfm