4.2 Article

Search for signatures of magnetically-induced alignment in the arrival directions measured by the Pierre Auger Observatory

Journal

ASTROPARTICLE PHYSICS
Volume 35, Issue 6, Pages 354-361

Publisher

ELSEVIER
DOI: 10.1016/j.astropartphys.2011.10.004

Keywords

Ultra-high energy cosmic rays; Pierre auger observatory; Arrival directions

Funding

  1. Comision Nacional de Energia Atomica
  2. Fundacion Antorchas
  3. Gobierno De La Provincia de Mendoza
  4. Municipalidad de Malargue
  5. NDM Holdings and Valle Las Lenas, Argentina
  6. Australian Research Council
  7. Conselho Nacional de Desenvolvimento Cientifico e Tecnologico (CNPq)
  8. Financiadora de Estudos e Projetos (FINEP)
  9. Fundacao de Amparo a Pesquisa do Estado de Rio de Janeiro (FAPERJ)
  10. Fundacao de Amparo A Pesquisa do Estado de Sao Paulo (FAPESP)
  11. Ministerio de Ciencia e Tecnologia (MCT), Brazil
  12. AVCR [AV0Z10100502, AV0Z10100522]
  13. GAAV [KJB100100904]
  14. MSMT-CR, Czech Republic [LA08016, LC527, 1M06002, MSM0021620859]
  15. Centre de Calcul IN2P3/CNRS
  16. Centre National de la Recherche Scientifique (CNRS)
  17. Conseil Regional Ile-de-France
  18. Departement Physique Nucleaire et Corpusculaire (PNC-IN2P3/CNRS)
  19. Departement Sciences de l'Univers (SDU-INSU/CNRS), France
  20. Bundesministerium fur Bildung und Forschung (BMBF)
  21. Deutsche Forschungsgemeinschaft (DFG)
  22. Finanzministerium Baden-Wurttemberg
  23. Helmholtz-Gemeinschaft Deutscher Forschungszentren (HGF)
  24. Ministerium fur Wissenschaft und Forschung
  25. Nordrhein-Westfalen
  26. Ministerium fur Wissenschaft, Forschung und Kunst, Baden-Wurttemberg, Germany
  27. Istituto Nazionale di Fisica Nucleare (INFN)
  28. Ministero dell'Istruzione, dell'Universita e della Ricerca (MIUR), Italy
  29. Consejo Nacional de Ciencia y Tecnologia (CONACYT), Mexico
  30. Ministerie van Onderwijs
  31. Cultuur en Wetenschap
  32. Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO)
  33. Stichting voor Fundamenteel Onderzoek der Materie (FOM), Netherlands
  34. Ministry of Science and Higher Education, Poland [1 P03 D 014 30, N202 090 31/0623, PAP/218/2006]
  35. Fundacao para a Ciencia e a Tecnologia, Portugal
  36. Ministry for Higher Education, Science, and Technology
  37. Slovenian Research Agency, Slovenia
  38. Comunidad de Madrid
  39. Consejeria de Educacion de la Comunidad de Castilla La Mancha
  40. FEDER
  41. Ministerio de Ciencia e Innovacion
  42. Consolider-Ingenio
  43. Xunta de Galicia, Spain
  44. Science and Technology Facilities Council, United Kingdom
  45. Department of Energy [DE-AC02-07CH11359, DE-FR02-04ER41300]
  46. National Science Foundation [0450696]
  47. Grainger Foundation USA
  48. ALFA-EC/HELEN
  49. European Union [MEIF-CF-2005-025057, PIEF-GA-2008-220240]
  50. UNESCO
  51. STFC [ST/J000507/1] Funding Source: UKRI
  52. Science and Technology Facilities Council [ST/J000507/1] Funding Source: researchfish
  53. Direct For Mathematical & Physical Scien
  54. Division Of Physics [1068210] Funding Source: National Science Foundation
  55. Division Of Physics
  56. Direct For Mathematical & Physical Scien [1068696, 0855623] Funding Source: National Science Foundation

Ask authors/readers for more resources

We present the results of an analysis of data recorded at the Pierre Auger Observatory in which we search for groups of directionally-aligned events (or 'multiplets') which exhibit a correlation between arrival direction and the inverse of the energy. These signatures are expected from sets of events coming from the same source after having been deflected by intervening coherent magnetic fields. The observation of several events from the same source would open the possibility to accurately reconstruct the position of the source and also measure the integral of the component of the magnetic field orthogonal to the trajectory of the cosmic rays. We describe the largest multiplets found and compute the probability that they appeared by chance from an isotropic distribution. We find no statistically significant evidence for the presence of multiplets arising from magnetic deflections in the present data. (C) 2011 Elsevier B.V. All rights reserved.

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