Antihelium flux signature for antimatter globular cluster in our Galaxy

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dc.creatorBelotsky, K. M.
dc.creatorGolubkov, Yu. A.
dc.creatorKhlopov, M. Yu.
dc.creatorKonoplich, R. V.
dc.creatorSakharov, A. S.
dc.date1998-07-02
dc.date.accessioned2026-07-07T02:27:19Z
dc.date.available2026-07-07T02:27:19Z
dc.descriptionThe AMS experiment is shown to be sensitive to test the hypothesis on the existence of antimatter globular cluster in our Galaxy. The hypothesis follows from the analysis of possible tests for the mechanisms of baryosynthesis and uses antimatter domains in the matter dominated Universe as the probe for the physics underlying the origin of the matter. The interval of masses for the antimatter in our Galaxy is fixed from below by the condition of antimatter domain survival in the matter dominated Universe and from above by the observed gamma ray flux. For this interval the expected fluxes of antihelium-3 and antihelium-4 are calculated with the account for their interaction with the matter in the Galaxy.
dc.description20 pages, 3 Postscript figures, Latex2e
dc.identifierhttps://arxiv.org/abs/astro-ph/9807027
dc.identifierhttp://arxiv.org/abs/astro-ph/9807027
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/12642
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.titleAntihelium flux signature for antimatter globular cluster in our Galaxy
dc.typetext

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