About: Anisotropy and chemical composition of ultra-high energy cosmic rays using arrival directions measured by the Pierre Auger Observatory     Goto   Sponge   NotDistinct   Permalink

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  • The Pierre Auger Collaboration has reported evidence for anisotropy in the distribution of arrival directions of the cosmic rays with energies E > Eth = 5.51019 eV. These show a correlation with the distribution of nearby extragalactic objects, including an apparent excess around the direction of Centaurus A. If the particles responsible for these excesses at E > Eth are heavy nuclei with charge Z, the proton component of the sources should lead to excesses in the same regions at energies E/Z. We here report the lack of anisotropies in these directions at energies above Eth/Z (for illustrative values of Z = 6, 13, 26). If the anisotropies above Eth are due to nuclei with charge Z, and under reasonable assumptions about the acceleration process, these observations imply stringent constraints on the allowed proton fraction at the lower energies.
  • The Pierre Auger Collaboration has reported evidence for anisotropy in the distribution of arrival directions of the cosmic rays with energies E > Eth = 5.51019 eV. These show a correlation with the distribution of nearby extragalactic objects, including an apparent excess around the direction of Centaurus A. If the particles responsible for these excesses at E > Eth are heavy nuclei with charge Z, the proton component of the sources should lead to excesses in the same regions at energies E/Z. We here report the lack of anisotropies in these directions at energies above Eth/Z (for illustrative values of Z = 6, 13, 26). If the anisotropies above Eth are due to nuclei with charge Z, and under reasonable assumptions about the acceleration process, these observations imply stringent constraints on the allowed proton fraction at the lower energies. (en)
Title
  • Anisotropy and chemical composition of ultra-high energy cosmic rays using arrival directions measured by the Pierre Auger Observatory
  • Anisotropy and chemical composition of ultra-high energy cosmic rays using arrival directions measured by the Pierre Auger Observatory (en)
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  • Anisotropy and chemical composition of ultra-high energy cosmic rays using arrival directions measured by the Pierre Auger Observatory
  • Anisotropy and chemical composition of ultra-high energy cosmic rays using arrival directions measured by the Pierre Auger Observatory (en)
skos:notation
  • RIV/68378271:_____/11:00371933!RIV13-AV0-68378271
http://linked.open...avai/predkladatel
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  • P(1M06002), P(KJB100100904), P(KJB300100801), P(LA08016), P(LC527), P(LG11044), P(MEB111003), Z(AV0Z10100502), Z(AV0Z10100522), Z(MSM0021620859)
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  • 6
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  • 186303
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  • RIV/68378271:_____/11:00371933
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  • ultra high energy cosmic rays; cosmic ray experiments (en)
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  • GB - Spojené království Velké Británie a Severního Irska
http://linked.open...ontrolniKodProRIV
  • [7314B3AA3C8C]
http://linked.open...i/riv/nazevZdroje
  • Journal of Cosmology and Astroparticle Physics
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  • 11
http://linked.open...iv/tvurceVysledku
  • Abreu, P.
  • Aglietta, M.
  • Ahn, E. J.
  • Boháčová, Martina
  • Chudoba, Jiří
  • Ebr, Jan
  • Mandát, Dušan
  • Nožka, Libor
  • Nečesal, Petr
  • Nyklíček, Michal
  • Palatka, Miroslav
  • Pech, Miroslav
  • Prouza, Michael
  • Schovancová, Jaroslava
  • Schovánek, Petr
  • Trávníček, Petr
  • Vícha, Jakub
  • Řídký, Jan
  • Šmída, Radomír
http://linked.open...ain/vavai/riv/wos
  • 000292332400022
http://linked.open...n/vavai/riv/zamer
issn
  • 1475-7516
number of pages
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  • 10.1088/1475-7516/2011/06/022
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