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Abstract:

Using data collected at the Pierre Auger Observatory during the past 3.7 years, we demonstrated a correlation between the arrival directions of cosmic rays with energy above 6 × 10 19 electron volts and the positions of active galactic nuclei (AGN) lying within ∼75 megaparsecs. We rejected the hypothesis of an isotropic distribution of these cosmic rays with at least a 99% confidence level from a prescribed a priori test. The correlation we observed is compatible with the hypothesis that the highest-energy particles originate from nearby extragalactic sources whose flux has not been substantially reduced by interaction with the cosmic background radiation. AGN or objects having a similar spatial distribution are possible sources.

Registro:

Documento: Artículo
Título:Correlation of the highest-energy cosmic rays with nearby extragalactic objects
Autor:Abraham, J. et al.
Este artículo contiene 444 autores, consultelos en el artículo en formato pdf.
Filiación: Este artículo contiene 444 autores con sus filiaciones, consultelas en el artículo en formato pdf.
Palabras clave:correlation; cosmic ray; electromagnetic radiation; electron; hypothesis testing; spatial distribution; article; correlation analysis; cosmic radiation; energy yield; magnetic field; priority journal
Año:2007
Volumen:318
Número:5852
Página de inicio:938
Página de fin:943
DOI: http://dx.doi.org/10.1126/science.1151124
Título revista:Science
Título revista abreviado:Science
ISSN:00368075
CODEN:SCIEA
Registro:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00368075_v318_n5852_p938_Abraham

Referencias:

  • Linsley, J., (1963) Phys. Rev. Lett, 10, p. 146
  • Abraham, J., (Pierre Auger Collaboration) (2004) Nucl. Instrum. Methods A, 523, p. 50
  • Greisen, K., (1966) Phys. Rev. Lett, 16, p. 748
  • Zatsepin, G.T., Kuzmin, V.A., (1966) Sov. Phys. JETP Lett, 4, p. 78
  • Berezinsky, V.S., Grigorieva, S.I., (1988) Astron. Astrophys, 199, p. 1
  • Hayashida, N., (1996) Phys. Rev. Lett, 77, p. 1000
  • Abbasi, R.U., The HiRes collaboration (2004) Astrophys. J, 610, pp. L73
  • Stanev, T., Biermann, P.L., Lloyd-Evans, J., Rachen, J.P., Watson, A.A., (1995) Phys. Rev. Lett, 75, p. 3056
  • Uchihori, Y., Nagano, M., Takeda, M., Teshima, M., Lloyd-Evans, J., Watson, A.A., (2000) Astropart. Phys, 13, p. 151
  • Ginzburg, V.L., Syrovatskii, S.I., (1964) The Origin of Cosmic Rays, , Pergamon, Oxford
  • Hillas, A.M., (1984) Annu. Rev. Astron. Astrophys, 22, p. 425
  • Véron-Cetty, M.-P., Véron, P., (2006) Astron. Astrophys, 455, p. 773
  • D. Allard et al. (Pierre Auger Collaboration), Astrophysics, available at http://arxiv.org/abs/astro-ph/0511104; Bonifazi, C., Letessier-Selvon, A., Santos, E.M., Astrophysics, , http://arxiv.org/abs/0705.1856, available at
  • Bonifazi, C., Pierre Auger Collaboration (2005) Proceedings of the 29th International Cosmic Ray Conference, 17, pp. 17-20. , Pune, India Tata Institute of Fundamental Research, India
  • M. Ave (Auger Collaboration), Astrophysics, available at http://arxiv.org/abs/0709.2125; M. Roth (Pierre Auger Collaboration), Astrophysics, available at http://arxiv.org/abs/0706.2096; B. R. Dawson (Pierre Auger Collaboration), Astrophysics, available at http://arxiv.org/abs/0706.1105; A redshift z corresponds to a distance 42 Mpc x (z/0.01) for a Hubble constant H 0 = 71 km s -1 Mpc -1 ; R. W. Clay (Pierre Auger Collaboration), in Proceedings of the 28th International Cosmic Ray Conference, Tsukuba, Japan (Universal Academic Press, Tokyo, Japan, 2003), 1, pp. 421-424; Revenu, B., Pierre Auger Collaboration (2005) Proceedings of the 29th International Cosmic Ray Conference, , Pune, India, 75
  • Han, J.L., Manchester, R.N., Lyne, A.G., Qiao, G.J., van Straten, W., (2006) Astrophys. J, 642, p. 868
  • S. Mollerach (Pierre Auger Collaboration), Astrophysics, available at http://arxiv.org/abs/0706.1749; We are grateful to the following agencies and organizations for financial support: Gobierno De La Provincia de Mendoza, Comisión Nacional de Energía Atómica, Municipalidad de Malargüe, Fundación Antorchas, Argentina; the Australian Research Council; Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq, Financiadora de Estudos e Projetos do Ministerio da Ciencia e Tecnologia (FINEP/MCT, Fundação de Amparo à Pesquisa do Estado de Rio de Janeiro (FAPERJ, Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP, Brazil; Ministry of Education, Youth and Sports of the Czech Republic; Centre National de la Recherche Scientifique (CNRS, Conseil Régional Ile-de-France, Département Physique Nucléaire et Corpusculaire (PNC-IN2P3/CNRS, Département Sciences de l'Univers (SDU-INSU/CNRS, France; Bundesministerium für Bildung und Forschung BMBF, Deut

Citas:

---------- APA ----------
(2007) . Correlation of the highest-energy cosmic rays with nearby extragalactic objects. Science, 318(5852), 938-943.
http://dx.doi.org/10.1126/science.1151124
---------- CHICAGO ----------
Abraham, J. "Correlation of the highest-energy cosmic rays with nearby extragalactic objects" . Science 318, no. 5852 (2007) : 938-943.
http://dx.doi.org/10.1126/science.1151124
---------- MLA ----------
Abraham, J. "Correlation of the highest-energy cosmic rays with nearby extragalactic objects" . Science, vol. 318, no. 5852, 2007, pp. 938-943.
http://dx.doi.org/10.1126/science.1151124
---------- VANCOUVER ----------
Abraham, J. Correlation of the highest-energy cosmic rays with nearby extragalactic objects. Science. 2007;318(5852):938-943.
http://dx.doi.org/10.1126/science.1151124