Ultra high energy photons and neutrinos with JEM-EUSO
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 dir...
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Springer Netherlands
2015
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Acceso en línea: | Registro en Scopus DOI Handle Registro en la Biblioteca Digital |
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001 | PAPER-24622 | ||
003 | AR-BaUEN | ||
005 | 20240318172625.0 | ||
008 | 190411s2015 xx ||||fo|||| 00| 0 eng|d | ||
024 | 7 | |2 scopus |a 2-s2.0-84961746401 | |
040 | |a Scopus |b spa |c AR-BaUEN |d AR-BaUEN | ||
110 | 2 | |a JEM-EUSO Collaboration |4 aut |e autor | |
245 | 1 | 0 | |a Ultra high energy photons and neutrinos with JEM-EUSO |
260 | |b Springer Netherlands |c 2015 | ||
270 | 1 | 0 | |m Supanitsky, D.; Instituto de Astronomía y Física del Espacio (IAFE), CONICET-UBA, Buenos Aires, Germany; email: dalesupa@gmail.com |
506 | |2 openaire |e Política editorial | ||
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504 | |a Whitehorn, N., Results from IceCube (2013) IceCube Particle Astrophysics Symposium (IPA 2013), May 13–15. Madison, , http://wipac.wisc.edu/meetings/home/IPA2013 | ||
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504 | |a Blennow, M., Meloni, D., (2009) Phys. Rev., D80, p. 065009 | ||
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504 | |a Block, M., Ha, P., McKay, D., Ultrahigh energy neutrino scattering: an update (2010) Phys. Rev. D, 82, p. 077302 | ||
504 | |a Sjöstrand, T., Mrenna, S., Skands, P., PYTHIA 6.4 physics and manual (2006) JHEP, 605, p. 026 | ||
504 | |a Whalley, M., http://hepforge.cedar.ac.uk/lhapdf/; Nadolsky, P., Implications of CTEQ global analysis for collider observables (2008) Phys. Rev. D, 78, p. 013004 | ||
504 | |a Supanitsky, A.D., Medina-Tanco, G., Neutrino initiated cascades at mid and high altitudes in the atmosphere (2011) Astropart. Phys., 34, pp. 8-16 | ||
504 | |a Bergmann, T., One-dimensional hybrid approach to extensive air shower simulation (2007) Astropart. Phys., 26, pp. 420-432 | ||
504 | |a Ostapchenko, S., QGSJET-II: towards reliable description of very high energy hadronic interactions (2006) Nucl. Phys. Proc. Suppl. B, 151, pp. 143-146 | ||
504 | |a Landau, L., Pomeranchuk, I., Limits of applicability of the theory of bremsstrahlung electrons and pair production at high-energies (1953) Dokl. Akad. Nauk SSSR, 92, pp. 535-536 | ||
504 | |a Landau, L., Pomeranchuk, I., Electron cascade process at very high-energies (1953) Dokl. Akad. Nauk SSSR, 92, pp. 735-738 | ||
504 | |a Migdal, A., Bremsstrahlung and pair production in condensed media at high-energies (1956) Phys. Rev., 103, pp. 1811-1820 | ||
504 | |a Supanitsky, A.D., Medina-Tanco, G., On the possibility of neutrino flavor identification at the highest energies (2012) Phys. Rev. D, 86, p. 093020 | ||
504 | |a Davidson, N., Nanava, G., Przedziński, T., Richter-Was, E., Was, Z., Universal interface of TAUOLA: technical and physics documentation (2012) Comput. Phys. Commun, 183, pp. 821-843 | ||
504 | |a Berat, C., Full simulation of space-based extensive air showers detectors with ESAF (2010) Astropart. Phys., 33, pp. 221-247 | ||
504 | |a Guzman, A., A study on JEM-EUSOs trigger probability for neutrino-initiated EAS (2013) Proceedings of the 33rd ICRC, p. 533. Brazil | ||
504 | |a Risse, M., Homola, P., Search for ultra-high energy photons using air showers (2007) Mod. Phys. Lett., A22, pp. 749-766 | ||
504 | |a Adams, J.H., Jr., (JEM-EUSO Collaboration), An evaluation of the exposure in nadir observation of the JEM-EUSO mission (2013) Astropart. Phys., 44, pp. 76-90 | ||
504 | |a Supanitsky, A.D., Medina-Tanco, G., Etchegoyen, A., New numerical technique to determine primary cosmic ray composition in the ankle region (2009) A. Astropart. Phys., 31, pp. 75-85 | ||
504 | |a Supanitsky, A.D., Medina-Tanco, G., The potential of the JEM-EUSO telescope for the astrophysics of extreme energy photons (2011) Proceedings of the 32nd ICRC, vol. 2, pp. 153–156. Beijing, 2, pp. 153-156 | ||
504 | |a Silvermann, B., (1986) Density Estimation for Statistics and Data Analysis, , Chapman and Hall, London | ||
504 | |a Ave, M., New constraints from haverah park data on the photon and iron fluxes of ultrahigh-energy cosmic rays (2000) Phys. Rev. Lett., 85, pp. 2244-2247 | ||
504 | |a Ave, M., Constraints on the ultrahigh-energy photon flux using inclined showers from the Haverah Park array (2002) Phys. Rev. D, 65, p. 063007 | ||
504 | |a Risse, M., Upper limit on the photon fraction in highest-energy cosmic rays from AGASA data (2005) Phys. Rev. Lett., 95, p. 171102 | ||
504 | |a Shinozaki, K., Upper limit on gamma-ray flux above 1019 eV estimated by the Akeno giant air shower array (2002) Astrophys. J., 571, p. L117—L120 | ||
504 | |a Abraham, J., (Pierre Auger Collaboration), An upper limit to the photon fraction in cosmic rays above {ARS}10 | ||
504 | |a Settimo, M., An update on a search for ultra-high energy photons using the Pierre Auger observatory (2011) Proceedings of the 32nd ICRC, vol. 2, pp. 55–58. Beijing, 2, pp. 55-58 | ||
504 | |a Abraham, J., (Pierre Auger Collaboration), Upper limit on the cosmic-ray photon flux above {ARS}1019 eV using the surface detector of the Pierre Auger observatory (2008) Astropart. Phys., 29, pp. 243-256 | ||
504 | |a Rubtsov, G., Upper limit on the ultrahigh-energy photon flux from AGASA and Yakutsk data (2006) Phys. Rev. D, 73, p. 063009 | ||
504 | |a Glushkov, A., Constraints on the fraction of primary gamma rays at ultra-high energies from the muon data of the Yakutsk EAS array (2007) JETP Lett., 85, pp. 131-135 | ||
504 | |a Salamida, F., Update on the measurement of the CR energy spectrum above 1018 eV made using the Pierre Auger observatory (2011) Proceedings of the 32nd ICRC, 2, pp. 145-148 | ||
520 | 3 | |a 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. |l eng | |
593 | |a St. Kliment Ohridski University of Sofia, Sofia, Bulgaria | ||
593 | |a LAL, Univ Paris-Sud, CNRS/IN2P3, Orsay, France | ||
593 | |a Omega, Ecole Polytechnique, CNRS/IN2P3, Palaiseau, France | ||
593 | |a APC, Univ Paris Diderot, CNRS/IN2P3, CEA/Irfu, Obs. de Paris, Sorbonne Paris Cité, Paris, France | ||
593 | |a IRAP, Université de Toulouse, CNRS, Toulouse, France | ||
593 | |a ECAP, University of Erlangen-Nuremberg, Erlangen, Germany | ||
593 | |a Karlsruhe Institute of Technology (KIT), Karlsruhe, Germany | ||
593 | |a Ludwig Maximilian University, Munich, Germany | ||
593 | |a Institute for Astronomy and Astrophysics, Kepler Center, University of Tübingen, Tübingen, Germany | ||
593 | |a Institut für Theoretische Physik und Astrophysik, University of Würzburg, Würzburg, Germany | ||
593 | |a Istituto Nazionale di Fisica Nucleare, Sezione di Bari, Bari, Italy | ||
593 | |a Universita’ degli Studi di Bari Aldo Moro and INFN, Sezione di Bari, Bari, Italy | ||
593 | |a Dipartimento di Fisica e Astronomia, Universita’ di Catania, Catania, Italy | ||
593 | |a Consiglio Nazionale delle Ricerche (CNR), Ist. di Fisica Applicata Nello Carrara, Firenze, Italy | ||
593 | |a Istituto Nazionale di Fisica Nucleare - Laboratori Nazionali di Frascati, Frascati, Italy | ||
593 | |a Istituto Nazionale di Fisica Nucleare - Sezione di Napoli, Naples, Italy | ||
593 | |a Dipartimento di Scienze Fisiche, Universita’ di Napoli Federico II, Naples, Italy | ||
593 | |a INAF - Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo, Palermo, Italy | ||
593 | |a Istituto Nazionale di Fisica Nucleare - Sezione di Roma Tor Vergata, Roma, Italy | ||
593 | |a Dipartimento di Fisica, Universita’ di Roma Tor Vergata, Roma, Italy | ||
593 | |a Istituto Nazionale di Fisica Nucleare - Sezione di Torino, Torino, Italy | ||
593 | |a Dipartimento di Fisica, Università di Torino, INFN Torino, Torino, Italy | ||
593 | |a Istituto Nazionale di Astrofisica, Osservatorio Astrofisico di Torino, Torino, Italy | ||
593 | |a Istituto Nazionale di Fisica Nucleare - Sezione di Catania, Catania, Italy | ||
593 | |a Dipartimento di Ingegneria, UTIU, Rome, Italy | ||
593 | |a DIETI, Universita’ degli Studi di Napoli Federico II, Napoli, Italy | ||
593 | |a Chiba University, Chiba, Japan | ||
593 | |a National Institute of Radiological Sciences, Chiba, Japan | ||
593 | |a Fukui University of Technology, Fukui, Japan | ||
593 | |a Kinki University, Higashi-Osaka, Japan | ||
593 | |a Hiroshima University, Hiroshima, Japan | ||
593 | |a Kanazawa University, Kanazawa, Japan | ||
593 | |a Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Japan | ||
593 | |a Kobe University, Kobe, Japan | ||
593 | |a Konan University, Kobe, Japan | ||
593 | |a Kyoto University, Kyoto, Japan | ||
593 | |a Yukawa Institute, Kyoto University, Kyoto, Japan | ||
593 | |a National Astronomical Observatory, Mitaka, Japan | ||
593 | |a Nagoya University, Nagoya, Japan | ||
593 | |a Solar-Terrestrial Environment Laboratory, Nagoya University, Nagoya, Japan | ||
593 | |a Graduate School of Science, Osaka City University, Osaka, Japan | ||
593 | |a Institute of Space and Astronautical Science/JAXA, Sagamihara, Japan | ||
593 | |a Aoyama Gakuin University, Sagamihara, Japan | ||
593 | |a Saitama University, Saitama, Japan | ||
593 | |a Hokkaido University, Sapporo, Japan | ||
593 | |a Interactive Research Center of Science, Tokyo Institute of Technology, Tokyo, Japan | ||
593 | |a University of Tokyo, Tokyo, Japan | ||
593 | |a High Energy Accelerator Research Organization (KEK), Tsukuba, Japan | ||
593 | |a RIKEN, Wako, Japan | ||
593 | |a Korea Astronomy and Space Science Institute (KASI), Daejeon, South Korea | ||
593 | |a Ewha Womans University, Seoul, South Korea | ||
593 | |a Sungkyunkwan University, Seoul, South Korea | ||
593 | |a Center for Galaxy Evolution Research, Yonsei University, Seoul, South Korea | ||
593 | |a Universidad Nacional Autónoma de México (UNAM), Mexico City, Mexico | ||
593 | |a Universidad Michoacana de San Nicolas de Hidalgo (UMSNH), Morelia, Mexico | ||
593 | |a Benemérita Universidad Autónoma de Puebla (BUAP), Puebla, Mexico | ||
593 | |a Institute of Physics, Jan Kochanowski University, Kielce, Poland | ||
593 | |a Astronomical Observatory, Jagiellonian University, Krakow, Poland | ||
593 | |a National Centre for Nuclear Research, Lodz, Poland | ||
593 | |a Space Research Centre of the Polish Academy of Sciences (CBK), Warsaw, Poland | ||
593 | |a Joint Institute for Nuclear Research, Dubna, Russian Federation | ||
593 | |a Central Research Institute of Machine Building, TsNIIMash, Korolev, Russian Federation | ||
593 | |a Skobeltsyn Institute of Nuclear Physics, Lomonosov Moscow State University, Moscow, Russian Federation | ||
593 | |a Department of Space Physics, Institute of Experimental Physics, Kosice, Slovakia | ||
593 | |a Consejo Superior de Investigaciones Científicas (CSIC), Madrid, Spain | ||
593 | |a Instituto Nacional de Técnica Aeroespacial (INTA), Madrid, Spain | ||
593 | |a Universidad de Alcalá (UAH), Madrid, Spain | ||
593 | |a Universidad Carlos III de Madrid, Madrid, Spain | ||
593 | |a Instituto de Astrofísica de Canarias (IAC), Tenerife, Spain | ||
593 | |a Swiss Center for Electronics and Microtechnology (CSEM), Neuchâtel, Switzerland | ||
593 | |a ISDC Data Centre for Astrophysics, Versoix, Switzerland | ||
593 | |a Institute for Atmospheric and Climate Science, ETH Zürich, Zürich, Switzerland | ||
593 | |a Space Science Laboratory, University of California, Berkeley, United States | ||
593 | |a University of Chicago, Chicago, United States | ||
593 | |a Colorado School of Mines, Golden, United States | ||
593 | |a University of Alabama in Huntsville, Huntsville, United States | ||
593 | |a University of California (UCLA), Los Angeles, United States | ||
593 | |a University of Wisconsin-Milwaukee, Milwaukee, United States | ||
593 | |a NASA - Marshall Space Flight Center, Madison County, United States | ||
593 | |a Vanderbilt University, Nashville, United States | ||
593 | |a Instituto de Astronomía y Física del Espacio (IAFE), CONICET-UBA, Buenos Aires, Argentina, Germany | ||
593 | |a Instituto de Ciencias Nucleares, UNAM, A. P. 70-543, México, D. F. 04510, Mexico | ||
690 | 1 | 0 | |a NEUTRINOS |
690 | 1 | 0 | |a PHOTONS |
690 | 1 | 0 | |a SPACE OBSERVATION |
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