New calculation of radioactive secondaries in cosmic rays

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dc.creatorMoskalenko, I. V.
dc.creatorMashnik, S. G.
dc.creatorStrong, A. W.
dc.date2001-06-27
dc.date2001-08-17
dc.date.accessioned2026-07-07T01:59:06Z
dc.date.available2026-07-07T01:59:06Z
dc.descriptionWe use a new version of our numerical model for particle propagation in the Galaxy to study radioactive secondaries. For evaluation of the production cross sections we use the Los Alamos compilation of all available experimental cross sections together with calculations using the improved Cascade-Exciton Model code CEM2k. Using the radioactive secondary ratios 26Al/27Al, 36Cl/Cl, 54Mn/Mn, we show how the improved cross-section calculations together with the new propagation code allow us to better constrain the size of the CR halo.
dc.descriptionerror in units (GeV->MeV) in Fig.1 is corrected; 4 pages, 8 ps-figures, to appear in the Proc. of 27th Int. Cosmic Ray Conf. (Hamburg, 2001), OG 1.3. More details can be found at http://www.gamma.mpe-garching.mpg.de/~aws/aws.html
dc.identifierhttps://arxiv.org/abs/astro-ph/0106502
dc.identifierhttp://arxiv.org/abs/astro-ph/0106502
dc.identifierProc. 27th ICRC (Hamburg), 2001, pp.1836-1839
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2973
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectNuclear Experiment
dc.subjectNuclear Theory
dc.titleNew calculation of radioactive secondaries in cosmic rays
dc.typetext

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