Discovery of Localized Regions of Excess 10-TeV Cosmic Rays

Research output: Contribution to journalArticleResearchpeer review

Authors

  • 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

External Research Organisations

  • U.S. Naval Research Laboratory (NRL)
  • Harvard University
  • University of California at Santa Cruz
  • University of Maryland
  • Max Planck Institute for Nuclear Physics
  • 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
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Details

Original languageEnglish
Article number221101
Number of pages5
JournalPhysical review letters
Volume101
Issue number22
Early online date24 Nov 2008
Publication statusPublished - 28 Nov 2008
Externally publishedYes

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 subject areas

Cite this

Discovery of Localized Regions of Excess 10-TeV Cosmic Rays. / Abdo, A. A.; Allen, B.; Aune, T. et al.
In: Physical review letters, Vol. 101, No. 22, 221101, 28.11.2008.

Research output: Contribution to journalArticleResearchpeer 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, vol. 101, no. 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), Article 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 ; Vol. 101, No. 22.
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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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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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