Navegar

Colección

Datos Estadísticas

Artículo

Estamos trabajando para incorporar este artículo al repositorio
Consulte el artículo en la página del editor
Consulte la política de Acceso Abierto del editor

Abstract:

The origin of ultrahigh energy cosmic rays (UHECR) is still unknown. However, great progress has been achieved in past years due to the good quality and large statistics in experimental data collected by the current observatories. The data of the Pierre Auger Observatory show that the composition of UHECRs becomes progressively lighter starting from 1017 eV up to ∼1018.3 eV and then, beyond that energy, it becomes increasingly heavier. These analyses are subject to important systematic uncertainties due to the use of hadronic interaction models that extrapolate lower energy accelerator data to the highest energies. Although proton models of UHECRs are disfavored by these results, they cannot be completely ruled out. It is well known that the energy spectra of gamma rays and neutrinos, produced during propagation of these very energetic particles through the intergalactic medium, are a useful tool to constrain the spectrum models. In particular, it has recently been shown that the neutrino upper limits obtained by IceCube challenge the proton models at 95% C.L. In this work we study the constraints imposed by the extragalactic gamma-ray background, measured by Fermi-LAT, on proton models of UHECRs. In particular, we make use of the extragalactic gamma-ray background flux, integrated from 50 GeV to 2 TeV, that originates in point sources, which has recently been obtained by the Fermi-LAT Collaboration, in combination with the neutrino upper limits, to constrain the emission of UHECRs at high redshifts (z>1), in the context of the proton models. © 2016 American Physical Society.

Registro:

Documento: Artículo
Título:Implications of gamma-ray observations on proton models of ultrahigh energy cosmic rays
Autor:Supanitsky, A.D.
Filiación:Instituto de Astronomía y Física Del Espacio (IAFE CONICET-UBA), CC 67, Sucursal 28, Buenos Aires, C1428ZAA, Argentina
Año:2016
Volumen:94
Número:6
DOI: http://dx.doi.org/10.1103/PhysRevD.94.063002
Título revista:Physical Review D
Título revista abreviado:Phy. Rev. D
ISSN:24700010
Registro:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_24700010_v94_n6_p_Supanitsky

Referencias:

  • Aab, A., (2015) Nucl. Instrum. Methods Phys. Res., Sect. A, 798, p. 172
  • Abu-Zayyad, T., (2012) Nucl. Instrum. Methods Phys. Res., Sect. A, 689, p. 87
  • Valiño, I., Proc. Sci., 2015 (ICRC2015), p. 271. , (Pierre Auger Collaboration)
  • Jui, C., Proc. Sci., 2015 (ICRC2015), p. 035. , (Telescope Array Collaboration)
  • Porcelli, A., Proc. Sci., 2015 (ICRC2015), p. 420. , (Pierre Auger Collaboration)
  • Aab, A., (2014) Phys. Rev. D, 90, p. 122005
  • Abbasi, R., (2015) Astropart. Phys., 64, p. 49
  • Fujii, T., Proc. Sci., 2015 (ICRC2015), p. 320. , (Telescope Array Collaboration)
  • Abbasi, R., (2016) JPS Conf. Proc., 9, p. 010016. , (Pierre Auger and Telescope Array Collaborations)
  • Hill, C., Schramm, D., (1985) Phys. Rev. D, 31, p. 564
  • De Marco, D., Blasi, P., Olinto, A., (2003) Astropart. Phys., 20, p. 53
  • Berezinsky, V., Grigorieva, S., Hnatyk, B., (2004) Astropart. Phys., 21, p. 617
  • Berezinsky, V., Gazizov, A., Grigorieva, S., (2005) Phys. Lett. B, 612, p. 147
  • Berezinsky, V., Gazizov, A., Grigorieva, S., (2006) Phys. Rev. D, 74, p. 043005
  • Aloisio, R., Berezinsky, V., Blasi, P., Gazizov, A., Grigorieva, S.I., Hnatyk, B., (2007) Astropart. Phys., 27, p. 76
  • Aloisio, R., Berezinsky, V.S., Blasi, P., Ostapchenko, S., (2008) Phys. Rev. D, 77, p. 025007
  • Aloisio, R., Berezinsky, V., Gazizov, A., (2012) Astropart. Phys., 39-40, p. 129
  • Abreu, P., (2013) Astrophys. J. Lett., 762, p. L13
  • Aloisio, R., Berezinsky, V., Blasi, P., J. Cosmol. Astropart. Phys., 2014 (10), p. 020
  • Unger, M., Farrar, G., Anchordoqui, L., (2015) Phys. Rev. D, 92, p. 123001
  • Globus, N., Allard, D., Parizot, E., (2015) Phys. Rev. D, 92, p. 021302
  • Heinze, J., Boncioli, D., Bustamante, M., Winter, W., (2016) Astrophys. J., 825, p. 122
  • Ishihara, A., https://www.icrr.u-tokyo.ac.jp/indico/getFile.py/access?contribId=0&sessionId=2&resld=0&materialId=slides&confId=23, (IceCube Collaboration); Berezinsky, V., Smirnov, A., (1975) Astrophys. Space Sci., 32, p. 461
  • Fodor, Z., Katz, S., Ringwald, A., Tu, H., J. Cosmol. Astropart. Phys., 2003 (11), p. 015
  • Semikoz, D., Sigl, G., J. Cosmol. Astropart. Phys., 2004 (4), p. 003
  • Ahlers, M., Anchordoqui, L., Gonzalez-Garcia, M., Halzen, F., Sarkar, S., (2010) Astropart. Phys., 34, p. 106
  • Decerprit, G., Allard, D., (2011) Astron. Astrophys., 535, p. A66
  • Berezinsky, V., Gazizov, A., Kachelrieß, M., Ostapchenko, S., (2011) Phys. Lett. B, 695, p. 13
  • Hooper, D., Taylor, A., Sarkar, S., (2011) Astropart. Phys., 34, p. 340
  • Gelmini, G., Kalashev, O., Semikoz, D., Dmitri, V., J. Cosmol. Astropart. Phys., 2012 (1), p. 044
  • Ackermann, M., (2015) Astrophys. J., 799, p. 86
  • Ackermann, M., (2016) Astrophys. J. Suppl. Ser., 222, p. 5
  • Ackermann, M., (2016) Phys. Rev. Lett., 116, p. 151105
  • Liu, R., Taylor, A.M., Wang, X., Aharonian, F.A., Phys. Rev. D, , arXiv:1603.03223 [(to be published)]
  • Berezinsky, V., Kalashev, O., (2016) Phys. Rev. D, 94, p. 023007
  • Kido, E., Kalashev, O., Proc. Sci., 2015 (ICRC2015), p. 258. , (Telescope Array Collaboration)
  • Kalashev, O., Kusenko, A., Essey, W., (2013) Phys. Rev. Lett., 111, p. 041103
  • Kalashev, O., Kido, E., (2015) J. Exp. Theor. Phys., 120, p. 790
  • Mücke, A., Engel, R., Rachen, J., Protheroe, R., Stanev, T., (2000) Comput. Phys. Commun., 124, p. 290
  • Olive, K., (2014) Chin. Phys. C, 38, p. 090001. , (Particle Data Group Collaboration)
  • Cooray, A., (2016) R. Soc. Open Sci., 3, p. 150555
  • Stanev, T., De Marco, D., Malkan, M., Stecker, F., (2006) Phys. Rev. D, 73, p. 043003
  • Kneiske, T.M., Bretz, T., Mannheim, K., Hartmann, D.H., (2004) Astron. Astrophys., 413, p. 807
  • Inoue, Y., Inoue, S., Kobayashi, M.A.R., Makiya, R., Niino, Y., Totani, T., (2013) Astrophys. J., 768, p. 197
  • Berezinsky, V., Gazizov, A., (2007) Astrophys. J., 669, p. 684
  • Berezinsky, V., Gazizov, A., Kalashev, O., arXiv:1606.09293; Feldman, G., Cousins, R., (1998) Phys. Rev. D, 57, p. 3873
  • Bechtol, K., arXiv:1511.00688; Barlow, R., arXiv:physics/0406120

Citas:

---------- APA ----------
(2016) . Implications of gamma-ray observations on proton models of ultrahigh energy cosmic rays. Physical Review D, 94(6).
http://dx.doi.org/10.1103/PhysRevD.94.063002
---------- CHICAGO ----------
Supanitsky, A.D. "Implications of gamma-ray observations on proton models of ultrahigh energy cosmic rays" . Physical Review D 94, no. 6 (2016).
http://dx.doi.org/10.1103/PhysRevD.94.063002
---------- MLA ----------
Supanitsky, A.D. "Implications of gamma-ray observations on proton models of ultrahigh energy cosmic rays" . Physical Review D, vol. 94, no. 6, 2016.
http://dx.doi.org/10.1103/PhysRevD.94.063002
---------- VANCOUVER ----------
Supanitsky, A.D. Implications of gamma-ray observations on proton models of ultrahigh energy cosmic rays. Phy. Rev. D. 2016;94(6).
http://dx.doi.org/10.1103/PhysRevD.94.063002