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Lithium and Beryllium Isotopes with the PAMELA Experiment
Univ Siegen, Dept Phys, D-57068 Siegen, Germany..
Ioffe Phys Tech Inst, RU-194021 St Petersburg, Russia..
Univ Siegen, Dept Phys, D-57068 Siegen, Germany..
Ioffe Phys Tech Inst, RU-194021 St Petersburg, Russia..
Vise andre og tillknytning
2018 (engelsk)Inngår i: Astrophysical Journal, ISSN 0004-637X, E-ISSN 1538-4357, Vol. 862, nr 2, artikkel-id 141Artikkel i tidsskrift (Fagfellevurdert) Published
Abstract [en]

The cosmic ray (CR) lithium and beryllium (Li-6, Li-7, Be-7, Be-9, Be-10) isotopic composition has been measured with the satellite-borne experiment PAMELA, which was launched into low-Earth orbit on board the Resurs-DKJ satellite on 2006 June 15. The rare lithium and beryllium isotopes in CRs are believed to originate mainly from the interaction of high-energy carbon, nitrogen, and oxygen nuclei with the interstellar medium (ISM), but also on "tertiary" interactions in the ISM (i.e., produced by further fragmentation of secondary beryllium and boron). In this paper, the isotopic ratios Li-7/Li-6 and Be-7/(Be-9 + Be-10), measured between 150 and 1100 MeV n(-1) using two different detector systems from 2006 July to 2014 September, will be presented.

sted, utgiver, år, opplag, sider
Institute of Physics Publishing (IOPP), 2018. Vol. 862, nr 2, artikkel-id 141
Emneord [en]
astroparticle physics, cosmic rays
HSV kategori
Identifikatorer
URN: urn:nbn:se:kth:diva-233280DOI: 10.3847/1538-4357/aacf89ISI: 000440621800003Scopus ID: 2-s2.0-85051533703OAI: oai:DiVA.org:kth-233280DiVA, id: diva2:1240664
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QC 20180822

Tilgjengelig fra: 2018-08-22 Laget: 2018-08-22 Sist oppdatert: 2018-10-16bibliografisk kontrollert

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