Properties of Cosmic Lithium Isotopes Measured by the Alpha Magnetic Spectrometer

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dc.contributor.authorAguilar, M.
dc.contributor.authorAmbrosi, G.
dc.contributor.authorAnderson, H.
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dc.contributor.authorLuo, Xi
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dc.contributor.authorRossi, F.
dc.contributor.authorRozhkov, A.
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dc.contributor.authorSagdeev, R.
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dc.contributor.authorvon Dratzig, A. Schultz
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dc.contributor.authorSeo, E. S.
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dc.contributor.authorSong, J. W.
dc.contributor.authorSong, X. J.
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dc.contributor.authorTang, Z. C.
dc.contributor.authorTian, J.
dc.contributor.authorTian, Y.
dc.contributor.authorTing, Samuel C. C.
dc.contributor.authorTing, S. M.
dc.contributor.authorTomassetti, N.
dc.contributor.authorTorsti, J.
dc.contributor.authorTurk, B.
dc.contributor.authorUbaldi, A.
dc.contributor.authorUrban, T.
dc.contributor.authorUsoskin, I.
dc.contributor.authorVagelli, V.
dc.contributor.authorVainio, R.
dc.contributor.authorVaisanen, P.
dc.contributor.authorValencia-Otero, M.
dc.contributor.authorValente, E.
dc.contributor.authorValtonen, E.
dc.contributor.authorAcosta, M. Vazquez
dc.contributor.authorVecchi, M.
dc.contributor.authorVelasco, M.
dc.contributor.authorWang, C. X.
dc.contributor.authorWang, J. C.
dc.contributor.authorWang, L.
dc.contributor.authorWang, L. Q.
dc.contributor.authorWang, N. H.
dc.contributor.authorWang, Q. L.
dc.contributor.authorWang, S.
dc.contributor.authorWang, X.
dc.contributor.authorWang, Z. M.
dc.contributor.authorWei, J.
dc.contributor.authorWeng, Z. L.
dc.contributor.authorWu, H.
dc.contributor.authorWu, Y.
dc.contributor.authorWu, Z. B.
dc.contributor.authorXiao, J. N.
dc.contributor.authorXiong, R. Q.
dc.contributor.authorXiong, X. Z.
dc.contributor.authorXu, W.
dc.contributor.authorYan, Q.
dc.contributor.authorYang, H. T.
dc.contributor.authorYang, Y.
dc.contributor.authorYi, H.
dc.contributor.authorYou, Y. H.
dc.contributor.authorYu, Y. M.
dc.contributor.authorYu, Z. Q.
dc.contributor.authorZhang, C.
dc.contributor.authorZhang, F. Z.
dc.contributor.authorZhang, J.
dc.contributor.authorZhang, J. H.
dc.contributor.authorZhang, Z.
dc.contributor.authorZhao, P. W.
dc.contributor.authorZheng, C.
dc.contributor.authorZheng, Z. M.
dc.contributor.authorZhuang, H. L.
dc.contributor.authorZhukov, V.
dc.contributor.authorZichichi, A.
dc.contributor.authorZuberi, M.
dc.contributor.authorZuccon, P.
dc.contributor.authorAMS Collaboration
dc.contributor.organizationfi=avaruustutkimuslaboratorio|en=Space Research Laboratory|
dc.contributor.organizationfi=matemaattis-luonnontieteellinen tiedekunta|en=Faculty of Science|
dc.contributor.organization-code1.2.246.10.2458963.20.36798383026
dc.contributor.organization-code1.2.246.10.2458963.20.47833719389
dc.converis.publication-id499096602
dc.converis.urlhttps://research.utu.fi/converis/portal/Publication/499096602
dc.date.accessioned2025-08-28T00:47:14Z
dc.date.available2025-08-28T00:47:14Z
dc.description.abstractWe present the first measurement of cosmic-ray fluxes of Li-6 and Li-7 isotopes in the rigidity range from 1.9 to 25 GV. The measurements are based on 9.7 x 10(5) 6Li and 1.04 x 10(6) 7Li nuclei collected by the Alpha Magnetic Spectrometer on the International Space Station from May 2011 to October 2023. We observe that over the entire rigidity range the Li-6 and Li-7 fluxes exhibit nearly identical time variations and, above similar to 4 GV, the time variations of Li-6, Li-7, He, Be, B, C, N, and O fluxes are identical. Above similar to 7 GV, we find an identical rigidity dependence of the Li-6 and Li-7 fluxes. This shows that they are both produced by collisions of heavier cosmic-ray nuclei with the interstellar medium and, in particular, excludes the existence of a sizable primary component in the Li-7 flux.
dc.identifier.eissn1079-7114
dc.identifier.jour-issn0031-9007
dc.identifier.olddbid206412
dc.identifier.oldhandle10024/189439
dc.identifier.urihttps://www.utupub.fi/handle/11111/45837
dc.identifier.urlhttps://journals.aps.org/prl/abstract/10.1103/PhysRevLett.134.201001
dc.identifier.urnURN:NBN:fi-fe2025082791246
dc.language.isoen
dc.okm.affiliatedauthorVainio, Rami
dc.okm.affiliatedauthorValtonen, Eino
dc.okm.discipline115 Astronomy and space scienceen_GB
dc.okm.discipline115 Avaruustieteet ja tähtitiedefi_FI
dc.okm.internationalcopublicationinternational co-publication
dc.okm.internationalityInternational publication
dc.okm.typeA1 ScientificArticle
dc.publisherAMER PHYSICAL SOC
dc.publisher.countryUnited Statesen_GB
dc.publisher.countryYhdysvallat (USA)fi_FI
dc.publisher.country-codeUS
dc.publisher.placeCOLLEGE PK
dc.relation.articlenumber201001
dc.relation.doi10.1103/PhysRevLett.134.201001
dc.relation.ispartofjournalPhysical Review Letters
dc.relation.issue20
dc.relation.volume134
dc.source.identifierhttps://www.utupub.fi/handle/10024/189439
dc.titleProperties of Cosmic Lithium Isotopes Measured by the Alpha Magnetic Spectrometer
dc.year.issued2025

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