Gamma-ray Bursts Produced by Mirror Stars

dc.creatorBlinnikov, S.
dc.date1999-02-21
dc.date.accessioned2026-07-07T02:30:33Z
dc.date.available2026-07-07T02:30:33Z
dc.descriptionI argue that cosmic Gamma-ray Bursts (GRB) may be produced by collapses or mergers of stars made of `mirror' matter. The mirror neutrinos (which are sterile for our matter) produced at these events can oscillate into ordinary neutrinos. The annihilations or decays of the latter create an electron-positron plasma and subsequent relativistic fireball with a very low baryon load needed for GRBs. The concept of mirror matter is able to explain several key problems of modern astrophysics: neutrino anomalies, the missing mass, MACHO microlensing events and GRBs. Thus this concept becomes very appealing and should be considered quite seriously and attentively.
dc.description7 pages, no figures.Presented at XXVII ITEP Winter School, Snegiri, Feb. 16 -- 24, 1999
dc.identifierhttps://arxiv.org/abs/astro-ph/9902305
dc.identifierhttp://arxiv.org/abs/astro-ph/9902305
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/13850
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.titleGamma-ray Bursts Produced by Mirror Stars
dc.typetext

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