Discovery of Localized Regions of Excess 10-TeV Cosmic Rays

Publikation: Beitrag in FachzeitschriftArtikelForschungPeer-Review

Autorschaft

  • A. A. Abdo
  • B. Allen
  • T. Aune
  • D. Berley
  • E. Blaufuss
  • S. Casanova
  • C. Chen
  • B. L. Dingus
  • R. W. Ellsworth
  • L. Fleysher
  • R. Fleysher
  • M. M. Gonzalez
  • J. A. Goodman
  • C. M. Hoffman
  • P. H. Hüntemeyer
  • B. E. Kolterman
  • C. P. Lansdell
  • J. T. Linnemann
  • J. E. McEnery
  • A. I. Mincer
  • P. Nemethy
  • D. Noyes
  • J. Pretz
  • J. M. Ryan
  • P. M.Saz Parkinson
  • A. Shoup
  • G. Sinnis
  • A. J. Smith
  • G. W. Sullivan
  • V. Vasileiou
  • G. P. Walker
  • D. A. Williams
  • G. B. Yodh

Externe Organisationen

  • U.S. Naval Research Laboratory (NRL)
  • Harvard University
  • University of California at Santa Cruz
  • University of Maryland
  • Max-Planck-Institut für Kernphysik
  • University of California at Irvine
  • Los Alamos National Laboratory
  • George Mason University
  • New York University (NYU)
  • Universidad Nacional Autónoma de México (UNAM)
  • Institute for Defense Analysis (IDA)
  • Michigan State University (MSU)
  • NASA Goddard Space Flight Center (NASA-GSFC)
  • University of New Hampshire
  • The Ohio State University
  • National Security Technologies
Forschungs-netzwerk anzeigen

Details

OriginalspracheEnglisch
Aufsatznummer221101
Seitenumfang5
FachzeitschriftPhysical review letters
Jahrgang101
Ausgabenummer22
Frühes Online-Datum24 Nov. 2008
PublikationsstatusVeröffentlicht - 28 Nov. 2008
Extern publiziertJa

Abstract

The 7 year data set of the Milagro TeV observatory contains 2.2×1011 events of which most are due to hadronic cosmic rays. These data are searched for evidence of intermediate scale structure. Excess emission on angular scales of ∼10° has been found in two localized regions of unknown origin with greater than 12σ significance. Both regions are inconsistent with pure gamma-ray emission with high confidence. One of the regions has a different energy spectrum than the isotropic cosmic-ray flux at a level of 4.6σ, and it is consistent with hard spectrum protons with an exponential cutoff, with the most significant excess at ∼10TeV. Potential causes of these excesses are explored, but no compelling explanations are found.

ASJC Scopus Sachgebiete

Zitieren

Discovery of Localized Regions of Excess 10-TeV Cosmic Rays. / Abdo, A. A.; Allen, B.; Aune, T. et al.
in: Physical review letters, Jahrgang 101, Nr. 22, 221101, 28.11.2008.

Publikation: Beitrag in FachzeitschriftArtikelForschungPeer-Review

Abdo, AA, Allen, B, Aune, T, Berley, D, Blaufuss, E, Casanova, S, Chen, C, Dingus, BL, Ellsworth, RW, Fleysher, L, Fleysher, R, Gonzalez, MM, Goodman, JA, Hoffman, CM, Hüntemeyer, PH, Kolterman, BE, Lansdell, CP, Linnemann, JT, McEnery, JE, Mincer, AI, Nemethy, P, Noyes, D, Pretz, J, Ryan, JM, Parkinson, PMS, Shoup, A, Sinnis, G, Smith, AJ, Sullivan, GW, Vasileiou, V, Walker, GP, Williams, DA & Yodh, GB 2008, 'Discovery of Localized Regions of Excess 10-TeV Cosmic Rays', Physical review letters, Jg. 101, Nr. 22, 221101. https://doi.org/10.48550/arXiv.0801.3827, https://doi.org/10.1103/PhysRevLett.101.221101
Abdo, A. A., Allen, B., Aune, T., Berley, D., Blaufuss, E., Casanova, S., Chen, C., Dingus, B. L., Ellsworth, R. W., Fleysher, L., Fleysher, R., Gonzalez, M. M., Goodman, J. A., Hoffman, C. M., Hüntemeyer, P. H., Kolterman, B. E., Lansdell, C. P., Linnemann, J. T., McEnery, J. E., ... Yodh, G. B. (2008). Discovery of Localized Regions of Excess 10-TeV Cosmic Rays. Physical review letters, 101(22), Artikel 221101. https://doi.org/10.48550/arXiv.0801.3827, https://doi.org/10.1103/PhysRevLett.101.221101
Abdo AA, Allen B, Aune T, Berley D, Blaufuss E, Casanova S et al. Discovery of Localized Regions of Excess 10-TeV Cosmic Rays. Physical review letters. 2008 Nov 28;101(22):221101. Epub 2008 Nov 24. doi: 10.48550/arXiv.0801.3827, 10.1103/PhysRevLett.101.221101
Abdo, A. A. ; Allen, B. ; Aune, T. et al. / Discovery of Localized Regions of Excess 10-TeV Cosmic Rays. in: Physical review letters. 2008 ; Jahrgang 101, Nr. 22.
Download
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abstract = "The 7 year data set of the Milagro TeV observatory contains 2.2×1011 events of which most are due to hadronic cosmic rays. These data are searched for evidence of intermediate scale structure. Excess emission on angular scales of ∼10° has been found in two localized regions of unknown origin with greater than 12σ significance. Both regions are inconsistent with pure gamma-ray emission with high confidence. One of the regions has a different energy spectrum than the isotropic cosmic-ray flux at a level of 4.6σ, and it is consistent with hard spectrum protons with an exponential cutoff, with the most significant excess at ∼10TeV. Potential causes of these excesses are explored, but no compelling explanations are found.",
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T1 - Discovery of Localized Regions of Excess 10-TeV Cosmic Rays

AU - Abdo, A. A.

AU - Allen, B.

AU - Aune, T.

AU - Berley, D.

AU - Blaufuss, E.

AU - Casanova, S.

AU - Chen, C.

AU - Dingus, B. L.

AU - Ellsworth, R. W.

AU - Fleysher, L.

AU - Fleysher, R.

AU - Gonzalez, M. M.

AU - Goodman, J. A.

AU - Hoffman, C. M.

AU - Hüntemeyer, P. H.

AU - Kolterman, B. E.

AU - Lansdell, C. P.

AU - Linnemann, J. T.

AU - McEnery, J. E.

AU - Mincer, A. I.

AU - Nemethy, P.

AU - Noyes, D.

AU - Pretz, J.

AU - Ryan, J. M.

AU - Parkinson, P. M.Saz

AU - Shoup, A.

AU - Sinnis, G.

AU - Smith, A. J.

AU - Sullivan, G. W.

AU - Vasileiou, V.

AU - Walker, G. P.

AU - Williams, D. A.

AU - Yodh, G. B.

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AB - The 7 year data set of the Milagro TeV observatory contains 2.2×1011 events of which most are due to hadronic cosmic rays. These data are searched for evidence of intermediate scale structure. Excess emission on angular scales of ∼10° has been found in two localized regions of unknown origin with greater than 12σ significance. Both regions are inconsistent with pure gamma-ray emission with high confidence. One of the regions has a different energy spectrum than the isotropic cosmic-ray flux at a level of 4.6σ, and it is consistent with hard spectrum protons with an exponential cutoff, with the most significant excess at ∼10TeV. Potential causes of these excesses are explored, but no compelling explanations are found.

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