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Ultra high energy photons and neutrinos with JEM-EUSO

Title
Ultra high energy photons and neutrinos with JEM-EUSO
Authors
The JEM-EUSO CollaborationAdams J.H.Jr.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.Błȩcki J.Blin-Bondil S.Blümer J.Bobik P.Bogomilov M.Bonamente M.Briggs M.S.Briz S.Bruno A.Cafagna F.Campana D.Capdevielle J.-N.Caruso R.Casolino M.Cassardo C.Castellinic G.Catalano C.Catalano G.Cellino A.Chikawa M.Christl M.J.Cline D.Connaughton V.Conti L.Cordero G.Crawford H.J.Cremonini R.Csorna S.Dagoret-Campagne S.de Castro A.J.De Donato C.de la Taille C.De Santis C.del Peral L.Dell’Oro A.De Simone N.Di Martino M.Distratis G.Dulucq F.Dupieux M.Ebersoldt A.Ebisuzaki T.Engel R.Falk S.Fang K.Fenu F.Fernández-Gómez I.Ferrarese S.Finco D.Flamini M.Fornaro C.Franceschi A.Fujimoto J.Fukushima M.Galeotti P.Garipov G.Geary J.Gelmini G.Giraudo G.Gonchar M.González Alvarado C.Gorodetzky P.Guarino F.Guzmán A.Hachisu Y.Harlov B.Haungs A.Hernández Carretero J.Higashide K.Ikeda D.Ikeda H.Inoue N.Inoue S.Insolia A.Isgrò F.Itow Y.Joven E.Judd E.G.Jung A.Kajino F.Kajino T.Kaneko I.Karadzhov Y.Karczmarczyk J.Karus M.Katahira K.Kawai K.Kawasaki Y.Keilhauer B.Khrenov B.A.Kim J.-S.Kim S.-W.Kleifges M.Klimov P.A.Kolev D.Kreykenbohm I.Kudela K.Kurihara Y.Kusenko A.Kuznetsov E.Lacombe M.Lachaud C.Lee J.Licandro J.Lim H.López F.Maccarone M.C.Mannheim K.Maravilla D.Marcelli L.Marini A.Martinez O.Masciantonio G.Mase K.Matev R.Medina-Tanco G.Mernik T.Miyamoto H.Miyazaki Y.Mizumoto Y.Modestino G.Monaco A.Monnier-Ragaigne D.Morales de los Ríos J.A.Moretto C.Morozenko V.S.Mot B.Murakami T.Murakami M.N.Nagata M.Nagataki S.Nakamura T.Napolitano T.Naumov D.Nava R.Neronov A.Nomoto K.Nonaka T.Ogawa T.Ogio S.Ohmori H.Olinto A.V.Orleański P.Osteria G.Panasyuk M.I.Parizot E.Park I.H.Park H.W.Pastircak B.Patzak T.Paul T.Pennypacker C.Perez Cano S.Peter T.Picozza P.Pierog T.Piotrowski L.W.Piraino S.Plebaniak Z.Pollini A.Prat P.Prévôt G.Prieto H.Putis M.Reardon P.Reyes M.Ricci M.Rodríguez I.Rodríguez Frías M.D.Ronga F.Roth M.Rothkaehl H.Roudil G.Rusinov I.Rybczyński M.Sabau M.D.Sáez-Cano G.Sagawa H.Saito A.Sakaki N.Sakata M.Salazar H.Sánchez S.Santangelo A.Santiago Crúz L.Sanz Palomino M.Saprykin O.Sarazin F.Sato H.Sato M.Schanz T.Schieler H.Scotti V.Segreto A.Selmane S.Semikoz D.Serra M.Sharakin S.Shibata T.Shimizu H.M.Shinozaki K.Shirahama T.Siemieniec-Oziȩbło G.Silva López H.H.Sledd J.Słomińska K.Sobey A.Sugiyama T.Supanitsky D.Suzuki M.Szabelska B.Szabelski J.Tajima F.Tajima N.Tajima T.Takahashi Y.Takami H.Takeda M.Takizawa Y.Tenzer C.Tibolla O.Tkachev L.Tokuno H.Tomida T.Tone N.Toscano S.Trillaud F.Tsenov R.Tsunesada Y.Tsuno K.Tymieniecka T.Uchihori Y.Unger M.Vaduvescu O.Valdés-Galicia J.F.Vallania P.Valore L.Vankova G.Vigorito C.Villaseñor L.von Ballmoos P.Wada S.Watanabe J.Watanabe S.Watts J.Weber M.Weiler T.J.Wibig T.Wiencke L.Wille M.Wilms J.Włodarczyk Z.Yamamoto T.Yamamoto Y.Yang J.Yano H.Yashin I.V.Yonetoku D.Yoshida K.Yoshida S.Young R.Zotov M.Y.Zuccaro Marchi A.
Ewha Authors
양종만
SCOPUS Author ID
양종만scopus
Issue Date
2015
Journal Title
Experimental Astronomy
ISSN
0922-6435JCR Link
Citation
vol. 40, no. 1, pp. 215 - 233
Keywords
NeutrinosPhotonsSpace observation
Publisher
Springer Netherlands
Indexed
SCIE; SCOPUS scopus
Abstract
Ultra high energy photons and neutrinos are carriers of very important astrophysical 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 highest energies. 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 the longitudinal 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. © 2013, Springer Science+Business Media Dordrecht.
DOI
10.1007/s10686-013-9353-2
Appears in Collections:
자연과학대학 > 물리학전공 > Journal papers
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