Strangelet propagation and cosmic ray flux

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dc.creatorMadsen, Jes
dc.date2004-11-18
dc.date2005-02-03
dc.date.accessioned2026-07-07T02:15:56Z
dc.date.available2026-07-07T02:15:56Z
dc.descriptionThe galactic propagation of cosmic ray strangelets is described and the resulting flux is calculated for a wide range of parameters as a prerequisite for strangelet searches in lunar soil and with an Earth orbiting magnetic spectrometer, AMS-02. While the inherent uncertainties are large, flux predictions at a measurable level are obtained for reasonable choices of parameters if strange quark matter is absolutely stable. This allows a direct test of the strange matter hypothesis.
dc.descriptionPublished version
dc.identifierhttps://arxiv.org/abs/astro-ph/0411538
dc.identifierhttp://arxiv.org/abs/astro-ph/0411538
dc.identifierPhys.Rev. D71 (2005) 014026
dc.identifierdoi:10.1103/PhysRevD.71.014026
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/8599
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectNuclear Theory
dc.titleStrangelet propagation and cosmic ray flux
dc.typetext

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