Primordial antimatter in the contemporary universe

dc.creatorBambi, Cosimo
dc.date2007-07-05
dc.date2007-07-11
dc.date.accessioned2026-07-07T09:38:28Z
dc.date.available2026-07-07T09:38:28Z
dc.descriptionIn some baryogenesis scenarios, the universe acquires a non-vanishing average baryonic charge, but the baryon to photon ratio is not spatially constant and can be even negative in some space regions. This allows for existence of lumps of antimatter in our neighborhood and the possibility that very compact antimatter objects make a part of cosmological dark matter. Here I discuss the peculiar signatures which may be observed in a near future.
dc.description8 pages. Talk presented at "SciNeGHE07", 18 - 20 June 2007, Frascati, Rome, Italy
dc.identifierhttps://arxiv.org/abs/0707.0721
dc.identifierhttp://arxiv.org/abs/0707.0721
dc.identifierFrascati Phys. Ser. 45, 129 (2007)
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/160816
dc.subjectHigh Energy Physics - Phenomenology
dc.titlePrimordial antimatter in the contemporary universe
dc.typetext

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