[Les rayons cosmiques, de la cheville à la coupure]
Les récentes avancées des mesures et de l'interprétation des rayons cosmiques, depuis la caractéristique spectrale appelé « cheville » jusqu'aux plus hautes énergies, sont brièvement revues. Aux plus hautes énergie, la question principale concerne l'origine de la suppression du flux observée au dessus de
Recent advances in measuring and interpreting cosmic rays from the spectral ankle to the highest energies are briefly reviewed. The prime question at the highest energies is about the origin of the flux suppression observed at
Mots-clés : Rayons cosmiques, Composition masse, Anisotropie
Karl-Heinz Kampert 1 ; Peter Tinyakov 2
@article{CRPHYS_2014__15_4_318_0, author = {Karl-Heinz Kampert and Peter Tinyakov}, title = {Cosmic rays from the ankle to the cutoff}, journal = {Comptes Rendus. Physique}, pages = {318--328}, publisher = {Elsevier}, volume = {15}, number = {4}, year = {2014}, doi = {10.1016/j.crhy.2014.04.006}, language = {en}, }
Karl-Heinz Kampert; Peter Tinyakov. Cosmic rays from the ankle to the cutoff. Comptes Rendus. Physique, Ultra-high-energy cosmic rays: From the ankle to the tip of the spectrum, Volume 15 (2014) no. 4, pp. 318-328. doi : 10.1016/j.crhy.2014.04.006. https://comptes-rendus.academie-sciences.fr/physique/articles/10.1016/j.crhy.2014.04.006/
[1] et al. Nucl. Instrum. Methods A, 523 (2004), p. 50
[2] et al. Nucl. Instrum. Methods A, 620 (2010), p. 227 | arXiv
[3] et al. Nucl. Instrum. Methods A, 689 (2012), p. 87 | arXiv
[4] et al. Nucl. Instrum. Methods A, 676 (2012), p. 54 | arXiv
[5] et al. Phys. Rev. Lett., 107 (2011) (171104) | arXiv
[6] et al. Phys. Rev. D, 87 (2013) (081101) | arXiv
[7] Astropart. Phys., 39–40 (2012), p. 129 | arXiv
[8] et al. Astron. Astrophys., 268 (1993), p. 726
[9] Phys. Rev. Lett., 16 (1966), p. 748
[10] Pis'ma Zh. Eksp. Teor. Fiz., 4 (1966), p. 114
[11] et al. Phys. Rev. Lett., 100 (2008) (101101) | arXiv
[12] et al. Phys. Rev. Lett., 101 (2008) (061101) | arXiv
[13] et al. EPJ Web Conf., 53 (2013) (01005) | arXiv
[14] arXiv
, 2013 |[15] et al., 2013 | arXiv
[16] arXiv
, 2013 |[17] et al. Astropart. Phys., 42 (2013), p. 90 | arXiv
[18] et al., 2013 | arXiv
[19] Astropart. Phys., 34 (2011), p. 620 | arXiv
[20] Astropart. Phys., 39–40 (2012), p. 33 | arXiv
[21] Astrophys. J., 746 (2012), p. 72 | arXiv
[22] Astropart. Phys., 54 (2014), p. 48 | arXiv
[23] et al. Astropart. Phys., 42 (2013), p. 41 | arXiv
[24] Front. Phys. China, 8 (2013), p. 748 | arXiv
[25] J. Cosmol. Astropart. Phys., 1310 (2013) (013) | arXiv
[26] Astropart. Phys., 35 (2012), p. 660 | arXiv
[27] Annu. Rev. Nucl. Part. Sci., 61 (2011), p. 467
[28] Astropart. Phys., 35 (2011), p. 98 | arXiv
[29] et al. Phys. Rev. Lett., 109 (2012) (062002) | arXiv
[30] TA Collaboration, H. Sagawa, et al. Highlight talk given at the 33rd Int. Cosmic Ray Conf., Rio de Janeiro, Brazil, 2013.
[31] et al. EPJ Web Conf., 53 (2013), p. 01006 | arXiv
[32] et al. Phys. Rev. Lett., 104 (2010) (091101) | arXiv
[33] et al. Rio de Janeiro, Brazil (2013) (#0964)
[34] et al. J. Cosmol. Astropart. Phys., 1302 (2013), p. 026 | arXiv
[35] Astropart. Phys., 33 (2010), p. 151 | arXiv
[36] et al. Beijing, China (2011), p. 149 | arXiv
[37] et al. Beijing, China (2011), p. 331
[38] et al. Nucl. Phys. Proc. Suppl., 190 (2009), p. 20 | arXiv
[39] et al. Astrophys. J., 768 (2013), p. L1 | arXiv
[40] et al. Nucl. Instrum. Methods A, 613 (2010), p. 29
[41] et al. Astrophys. J., 757 (2012), p. 26 | arXiv
[42] Rep. Prog. Phys., 57 (1994), p. 325
[43] J. Cosmol. Astropart. Phys., 0501 (2005) (009) | arXiv
[44] Phys. Rev. D, 70 (2004) (043007) | arXiv
[45] Science, 320 (2008), p. 909 | arXiv
[46] Astrophys. J., 682 (2008), p. 29 | arXiv
[47] Astrophys. J., 710 (2010), p. 1422
[48] Astropart. Phys., 35 (2011), p. 135
[49] Phys. Rev. D, 87 (2013) (063002)
[50] arXiv
, 1999 |[51] Astrophys. J., 674 (2008), p. 258
[52] Astrophys. J., 738 (2011), p. 192 | arXiv
[53] Astrophys. J., 761 (2012), p. L11 | arXiv
[54] Astropart. Phys., 24 (2005), p. 32 | arXiv
[55] arXiv
, 2013 |[56] JETP Lett., 74 (2001), p. 1 | arXiv
[57] et al. J. Cosmol. Astropart. Phys., 1204 (2012) (040)
[58] et al. Rio de Janeiro, Brazil (2013) (#0311)
[59] et al. Rio de Janeiro, Brazil (2013) (#0310)
[60] et al. J. Cosmol. Astropart. Phys., 1106 (2011) (022) | arXiv
[61] et al. Rio de Janeiro, Brazil (2013) (#1033)
[62] arXiv
, 2012 |[63] Astron. Astrophys., 455 (2006), p. 773
[64] et al. Science, 318 (2007), p. 938 | arXiv
[65] et al. Astropart. Phys., 34 (2010), p. 314 | arXiv
[66] et al. Astropart. Phys., 30 (2008), p. 175 | arXiv
[67] et al. Astropart. Phys., 34 (2011), p. 627 | arXiv
[68] et al. Astrophys. J., 762 (2013), p. L13 | arXiv
[69] et al. Searches for Large Scale Anisotropy in the Arrival Directions of Cosmic Rays Detected above
[70] et al., 2013 | arXiv
[71] J. Cosmol. Astropart. Phys., 0904 (2009) (003) | arXiv
[72] et al. J. Cosmol. Astropart. Phys., 1305 (2013) (015) | arXiv
[73] et al. Astrophys. J., 760 (2012), p. 148 | arXiv
[74] et al. Rio de Janeiro, Brazil (2013) | arXiv
[75] Annu. Rev. Astron. Astrophys., 47 (2009), p. 523
Cité par Sources :
Commentaires - Politique