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dc.contributor.author
Supanitsky, Alberto Daniel
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Medina Tanco, G.
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Guzman, A.
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Adams, J. H.
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Ahmad, S.
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Albert, J. N.
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Allard, D.
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Anchordoqui, L.
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Andreev, V.
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Anzalone, A.
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Arai, Y.
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Asano, K.
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Ave Pernas, M.
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Baragatti, P.
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Barrillon, P.
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Batsch, T.
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Bayer, J.
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Bechini, R.
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Belenguer, T.
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Bellotti, R.
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Belov, K.
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Berlind, A. A.
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Bertaina, M.
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Biermann, P. L.
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Biktemerova, S.
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Blaksley, C.
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Blanc, N.
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Blecki, J.
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Blin-Bondil, S.
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Blumer, J.
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The JEM-EUSO Collaboration
dc.date.available
2017-06-16T17:44:09Z
dc.date.issued
2015-11
dc.identifier.citation
Supanitsky, Alberto Daniel; Medina Tanco, G.; Guzman, A.; Adams, J. H.; Ahmad, S.; et al.; Ultra high energy photons and neutrinos with JEM-EUSO; Springer; Experimental Astronomy; 40; 1; 11-2015; 215-233
dc.identifier.issn
0922-6435
dc.identifier.uri
http://hdl.handle.net/11336/18310
dc.description.abstract
Ultra high energy photons and neutrinos are carriers of very importantastrophysical information. They may be produced at the sites of cosmic ray acceleration or during the propagation of the cosmic rays in the intergalactic medium. In contrast to charged cosmic rays, photon and neutrino arrival directions point to the production site because they are not deflected by the magnetic fields of the Galaxy or the intergalactic medium. In this work we study the characteristics of the longitudinal development of showers initiated by photons and neutrinos at the highestenergies. These studies are relevant for development of techniques for neutrino and photon identification by the JEM-EUSO telescope. In particular, we study the possibility of observing the multi-peak structure of very deep horizontal neutrino showers with JEM-EUSO. We also discuss the possibility to determine the flavor content of the incident neutrino flux by taking advantage of the different characteristics of thelongitudinal profiles generated by different type of neutrinos. This is of grate importance for the study of the fundamental properties of neutrinos at the highest energies. Regarding photons, we discuss the detectability of the cosmogenic component by JEM-EUSO and also estimate the expected upper limits on the photon fraction which can be obtained from the future JEM-EUSO data for the case in which there are no photons in the samples.
dc.format
application/pdf
dc.language.iso
eng
dc.publisher
Springer
dc.rights
info:eu-repo/semantics/openAccess
dc.rights.uri
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.subject
Neutrinos
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Photons
dc.subject
Space Observation
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Astronomía
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Ciencias Físicas
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CIENCIAS NATURALES Y EXACTAS
dc.title
Ultra high energy photons and neutrinos with JEM-EUSO
dc.type
info:eu-repo/semantics/article
dc.type
info:ar-repo/semantics/artículo
dc.type
info:eu-repo/semantics/publishedVersion
dc.date.updated
2017-06-13T14:13:39Z
dc.journal.volume
40
dc.journal.number
1
dc.journal.pagination
215-233
dc.journal.pais
Alemania
dc.journal.ciudad
Berlin
dc.description.fil
Fil: Supanitsky, Alberto Daniel. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
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Fil: Medina Tanco, G.. Universidad Nacional Autónoma de México; México
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Fil: Guzman, A.. University of Tubingen; Alemania
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Fil: Adams, J. H.. University of Alabama in Huntsville; Estados Unidos
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Fil: Ahmad, S.. Ecole Polytechnique; Francia
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Fil: Albert, J. N.. Univ Paris-Sud; Francia
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Fil: Allard, D.. Univ Paris Diderot; Francia
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Fil: Anchordoqui, L.. University of Wisconsin-Milwaukee; Estados Unidos
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Fil: Andreev, V.. University of California; Estados Unidos
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Fil: Anzalone, A.. Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo; Italia
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Fil: Arai, Y.. High Energy Accelerator Research Organization (KEK); Japón
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Fil: Asano, K.. Tokyo Institute of Technology; Japón
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Fil: Ave Pernas, M.. Universidad de Alcalá; España
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Fil: Baragatti, P.. UTIU, Dipartimento di Ingegneria; Italia
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Fil: Barrillon, P.. Univ Paris-Sud; Francia
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Fil: Batsch, T.. National Centre for Nuclear Research; Polonia
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Fil: Bayer, J.. University of Tubingen; Alemania
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Fil: Bechini, R.. Istituto Nazionale di Fisica Nucleare; Italia
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Fil: Belenguer, T.. Instituto Nacional de Tecnica Aeroespacial (INTA); España
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Fil: Bellotti, R.. Istituto Nazionale di Fisica Nucleare; Italia
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Fil: Belov, K.. University of California; Estados Unidos
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Fil: Berlind, A. A.. Vanderbilt University; Estados Unidos
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Fil: Bertaina, M.. Istituto Nazionale di Fisica Nucleare; Italia
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Fil: Biermann, P. L.. Karlsruhe Institute of Technology (KIT); Alemania
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Fil: Biktemerova, S.. Joint Institute for Nuclear Research; Rusia
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Fil: Blaksley, C.. Univ Paris Diderot; Francia
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Fil: Blanc, N.. Swiss Center for Electronics and Microtechnology (CSEM); Suiza
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Fil: Blecki, J.. Space Research Centre of the Polish Academy of Sciences (CBK); Polonia
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Fil: Blin-Bondil, S.. Ecole Polytechnique; Francia
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Fil: Blumer, J.. Karlsruhe Institute of Technology (KIT); Alemania
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Fil: The JEM-EUSO Collaboration.
dc.journal.title
Experimental Astronomy
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1007/s10686-013-9353-2
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/ark/https://link.springer.com/article/10.1007/s10686-013-9353-2
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