Ultra high energy photons and neutrinos with JEM-EUSO

Autores
Supanitsky, Alberto Daniel; Medina Tanco, G.; Guzman, A.; Adams, J. H.; Ahmad, S.; Albert, J. N.; Allard, D.; Anchordoqui, L.; Andreev, V.; Anzalone, A.; Arai, Y.; Asano, K.; Ave Pernas, M.; Baragatti, P.; Barrillon, P.; Batsch, T.; Bayer, J.; Bechini, R.; Belenguer, T.; Bellotti, R.; Belov, K.; Berlind, A. A.; Bertaina, M.; Biermann, P. L.; Biktemerova, S.; Blaksley, C.; Blanc, N.; Blecki, J.; Blin-Bondil, S.; Blumer, J.; The JEM-EUSO Collaboration
Año de publicación
2015
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
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.
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
Fil: Medina Tanco, G.. Universidad Nacional Autónoma de México; México
Fil: Guzman, A.. University of Tubingen; Alemania
Fil: Adams, J. H.. University of Alabama in Huntsville; Estados Unidos
Fil: Ahmad, S.. Ecole Polytechnique; Francia
Fil: Albert, J. N.. Univ Paris-Sud; Francia
Fil: Allard, D.. Univ Paris Diderot; Francia
Fil: Anchordoqui, L.. University of Wisconsin-Milwaukee; Estados Unidos
Fil: Andreev, V.. University of California; Estados Unidos
Fil: Anzalone, A.. Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo; Italia
Fil: Arai, Y.. High Energy Accelerator Research Organization (KEK); Japón
Fil: Asano, K.. Tokyo Institute of Technology; Japón
Fil: Ave Pernas, M.. Universidad de Alcalá; España
Fil: Baragatti, P.. UTIU, Dipartimento di Ingegneria; Italia
Fil: Barrillon, P.. Univ Paris-Sud; Francia
Fil: Batsch, T.. National Centre for Nuclear Research; Polonia
Fil: Bayer, J.. University of Tubingen; Alemania
Fil: Bechini, R.. Istituto Nazionale di Fisica Nucleare; Italia
Fil: Belenguer, T.. Instituto Nacional de Tecnica Aeroespacial (INTA); España
Fil: Bellotti, R.. Istituto Nazionale di Fisica Nucleare; Italia
Fil: Belov, K.. University of California; Estados Unidos
Fil: Berlind, A. A.. Vanderbilt University; Estados Unidos
Fil: Bertaina, M.. Istituto Nazionale di Fisica Nucleare; Italia
Fil: Biermann, P. L.. Karlsruhe Institute of Technology (KIT); Alemania
Fil: Biktemerova, S.. Joint Institute for Nuclear Research; Rusia
Fil: Blaksley, C.. Univ Paris Diderot; Francia
Fil: Blanc, N.. Swiss Center for Electronics and Microtechnology (CSEM); Suiza
Fil: Blecki, J.. Space Research Centre of the Polish Academy of Sciences (CBK); Polonia
Fil: Blin-Bondil, S.. Ecole Polytechnique; Francia
Fil: Blumer, J.. Karlsruhe Institute of Technology (KIT); Alemania
Fil: The JEM-EUSO Collaboration.
Materia
Neutrinos
Photons
Space Observation
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/18310

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network_name_str CONICET Digital (CONICET)
spelling Ultra high energy photons and neutrinos with JEM-EUSOSupanitsky, Alberto DanielMedina Tanco, G.Guzman, A.Adams, J. H.Ahmad, S.Albert, J. N.Allard, D.Anchordoqui, L.Andreev, V.Anzalone, A.Arai, Y.Asano, K.Ave Pernas, M.Baragatti, P.Barrillon, P.Batsch, T.Bayer, J.Bechini, R.Belenguer, T.Bellotti, R.Belov, K.Berlind, A. A.Bertaina, M.Biermann, P. L.Biktemerova, S.Blaksley, C.Blanc, N.Blecki, J.Blin-Bondil, S.Blumer, J.The JEM-EUSO CollaborationNeutrinosPhotonsSpace Observationhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Ultra 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.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; ArgentinaFil: Medina Tanco, G.. Universidad Nacional Autónoma de México; MéxicoFil: Guzman, A.. University of Tubingen; AlemaniaFil: Adams, J. H.. University of Alabama in Huntsville; Estados UnidosFil: Ahmad, S.. Ecole Polytechnique; FranciaFil: Albert, J. N.. Univ Paris-Sud; FranciaFil: Allard, D.. Univ Paris Diderot; FranciaFil: Anchordoqui, L.. University of Wisconsin-Milwaukee; Estados UnidosFil: Andreev, V.. University of California; Estados UnidosFil: Anzalone, A.. Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo; ItaliaFil: Arai, Y.. High Energy Accelerator Research Organization (KEK); JapónFil: Asano, K.. Tokyo Institute of Technology; JapónFil: Ave Pernas, M.. Universidad de Alcalá; EspañaFil: Baragatti, P.. UTIU, Dipartimento di Ingegneria; ItaliaFil: Barrillon, P.. Univ Paris-Sud; FranciaFil: Batsch, T.. National Centre for Nuclear Research; PoloniaFil: Bayer, J.. University of Tubingen; AlemaniaFil: Bechini, R.. Istituto Nazionale di Fisica Nucleare; ItaliaFil: Belenguer, T.. Instituto Nacional de Tecnica Aeroespacial (INTA); EspañaFil: Bellotti, R.. Istituto Nazionale di Fisica Nucleare; ItaliaFil: Belov, K.. University of California; Estados UnidosFil: Berlind, A. A.. Vanderbilt University; Estados UnidosFil: Bertaina, M.. Istituto Nazionale di Fisica Nucleare; ItaliaFil: Biermann, P. L.. Karlsruhe Institute of Technology (KIT); AlemaniaFil: Biktemerova, S.. Joint Institute for Nuclear Research; RusiaFil: Blaksley, C.. Univ Paris Diderot; FranciaFil: Blanc, N.. Swiss Center for Electronics and Microtechnology (CSEM); SuizaFil: Blecki, J.. Space Research Centre of the Polish Academy of Sciences (CBK); PoloniaFil: Blin-Bondil, S.. Ecole Polytechnique; FranciaFil: Blumer, J.. Karlsruhe Institute of Technology (KIT); AlemaniaFil: The JEM-EUSO Collaboration.Springer2015-11info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/18310Supanitsky, 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; 215-2330922-6435CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1007/s10686-013-9353-2info:eu-repo/semantics/altIdentifier/ark/https://link.springer.com/article/10.1007/s10686-013-9353-2info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T11:23:20Zoai:ri.conicet.gov.ar:11336/18310instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-10-22 11:23:21.081CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Ultra high energy photons and neutrinos with JEM-EUSO
title Ultra high energy photons and neutrinos with JEM-EUSO
spellingShingle Ultra high energy photons and neutrinos with JEM-EUSO
Supanitsky, Alberto Daniel
Neutrinos
Photons
Space Observation
title_short Ultra high energy photons and neutrinos with JEM-EUSO
title_full Ultra high energy photons and neutrinos with JEM-EUSO
title_fullStr Ultra high energy photons and neutrinos with JEM-EUSO
title_full_unstemmed Ultra high energy photons and neutrinos with JEM-EUSO
title_sort Ultra high energy photons and neutrinos with JEM-EUSO
dc.creator.none.fl_str_mv Supanitsky, Alberto Daniel
Medina Tanco, G.
Guzman, A.
Adams, J. H.
Ahmad, S.
Albert, J. N.
Allard, D.
Anchordoqui, L.
Andreev, V.
Anzalone, A.
Arai, Y.
Asano, K.
Ave Pernas, M.
Baragatti, P.
Barrillon, P.
Batsch, T.
Bayer, J.
Bechini, R.
Belenguer, T.
Bellotti, R.
Belov, K.
Berlind, A. A.
Bertaina, M.
Biermann, P. L.
Biktemerova, S.
Blaksley, C.
Blanc, N.
Blecki, J.
Blin-Bondil, S.
Blumer, J.
The JEM-EUSO Collaboration
author Supanitsky, Alberto Daniel
author_facet Supanitsky, Alberto Daniel
Medina Tanco, G.
Guzman, A.
Adams, J. H.
Ahmad, S.
Albert, J. N.
Allard, D.
Anchordoqui, L.
Andreev, V.
Anzalone, A.
Arai, Y.
Asano, K.
Ave Pernas, M.
Baragatti, P.
Barrillon, P.
Batsch, T.
Bayer, J.
Bechini, R.
Belenguer, T.
Bellotti, R.
Belov, K.
Berlind, A. A.
Bertaina, M.
Biermann, P. L.
Biktemerova, S.
Blaksley, C.
Blanc, N.
Blecki, J.
Blin-Bondil, S.
Blumer, J.
The JEM-EUSO Collaboration
author_role author
author2 Medina Tanco, G.
Guzman, A.
Adams, J. H.
Ahmad, S.
Albert, J. N.
Allard, D.
Anchordoqui, L.
Andreev, V.
Anzalone, A.
Arai, Y.
Asano, K.
Ave Pernas, M.
Baragatti, P.
Barrillon, P.
Batsch, T.
Bayer, J.
Bechini, R.
Belenguer, T.
Bellotti, R.
Belov, K.
Berlind, A. A.
Bertaina, M.
Biermann, P. L.
Biktemerova, S.
Blaksley, C.
Blanc, N.
Blecki, J.
Blin-Bondil, S.
Blumer, J.
The JEM-EUSO Collaboration
author2_role author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv Neutrinos
Photons
Space Observation
topic Neutrinos
Photons
Space Observation
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv 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.
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
Fil: Medina Tanco, G.. Universidad Nacional Autónoma de México; México
Fil: Guzman, A.. University of Tubingen; Alemania
Fil: Adams, J. H.. University of Alabama in Huntsville; Estados Unidos
Fil: Ahmad, S.. Ecole Polytechnique; Francia
Fil: Albert, J. N.. Univ Paris-Sud; Francia
Fil: Allard, D.. Univ Paris Diderot; Francia
Fil: Anchordoqui, L.. University of Wisconsin-Milwaukee; Estados Unidos
Fil: Andreev, V.. University of California; Estados Unidos
Fil: Anzalone, A.. Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo; Italia
Fil: Arai, Y.. High Energy Accelerator Research Organization (KEK); Japón
Fil: Asano, K.. Tokyo Institute of Technology; Japón
Fil: Ave Pernas, M.. Universidad de Alcalá; España
Fil: Baragatti, P.. UTIU, Dipartimento di Ingegneria; Italia
Fil: Barrillon, P.. Univ Paris-Sud; Francia
Fil: Batsch, T.. National Centre for Nuclear Research; Polonia
Fil: Bayer, J.. University of Tubingen; Alemania
Fil: Bechini, R.. Istituto Nazionale di Fisica Nucleare; Italia
Fil: Belenguer, T.. Instituto Nacional de Tecnica Aeroespacial (INTA); España
Fil: Bellotti, R.. Istituto Nazionale di Fisica Nucleare; Italia
Fil: Belov, K.. University of California; Estados Unidos
Fil: Berlind, A. A.. Vanderbilt University; Estados Unidos
Fil: Bertaina, M.. Istituto Nazionale di Fisica Nucleare; Italia
Fil: Biermann, P. L.. Karlsruhe Institute of Technology (KIT); Alemania
Fil: Biktemerova, S.. Joint Institute for Nuclear Research; Rusia
Fil: Blaksley, C.. Univ Paris Diderot; Francia
Fil: Blanc, N.. Swiss Center for Electronics and Microtechnology (CSEM); Suiza
Fil: Blecki, J.. Space Research Centre of the Polish Academy of Sciences (CBK); Polonia
Fil: Blin-Bondil, S.. Ecole Polytechnique; Francia
Fil: Blumer, J.. Karlsruhe Institute of Technology (KIT); Alemania
Fil: The JEM-EUSO Collaboration.
description 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.
publishDate 2015
dc.date.none.fl_str_mv 2015-11
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/18310
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
0922-6435
CONICET Digital
CONICET
url http://hdl.handle.net/11336/18310
identifier_str_mv 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
0922-6435
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1007/s10686-013-9353-2
info:eu-repo/semantics/altIdentifier/ark/https://link.springer.com/article/10.1007/s10686-013-9353-2
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
dc.publisher.none.fl_str_mv Springer
publisher.none.fl_str_mv Springer
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
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instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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