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dc.date.accessioned 2019-08-22T15:00:50Z
dc.date.available 2019-08-22T15:00:50Z
dc.date.issued 2005-03-16
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/79549
dc.description.abstract The shadowing of high-energy cosmic rays by the Moon has been observed with a significance of 9.4 standard deviations with the L3 + C muon spectrometer at CERN. A significant effect of the Earth magnetic field is observed. Since no event deficit on the east side of the Moon has been observed, an upper limit at 90% confidence level on the antiproton to proton ratio of 0.11 is obtained for primary energies around 1 TeV. en
dc.format.extent 411-434 es
dc.language en es
dc.subject Radiación cósmica es
dc.subject Luna es
dc.subject Protones es
dc.title Measurement of the shadowing of high-energy cosmic rays by the Moon: a search for TeV-energy antiprotons en
dc.type Articulo es
sedici.identifier.other https://doi.org/10.1016/j.astropartphys.2005.02.002
sedici.identifier.issn 0927-6505 es
sedici.creator.person Dova, María Teresa es
sedici.creator.person L3 Collaboration es
sedici.subject.materias Ciencias Exactas es
sedici.subject.materias Física es
sedici.description.fulltext true es
mods.originInfo.place Facultad de Ciencias Exactas es
sedici.subtype Articulo es
sedici.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/
sedici.description.peerReview peer-review es
sedici.relation.journalTitle Astroparticle Physics es
sedici.relation.journalVolumeAndIssue vol. 23, no. 4 es


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Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Except where otherwise noted, this item's license is described as Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)