Mohamad-Ziad Charif - Antares
Mohamad-Ziad Charif - Antares Mohamad-Ziad Charif - Antares
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- Page 112 and 113: Figure 6.1: . True Position of the
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- Page 156 and 157: Bibliography[1] Volders, L. M. J. S
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[74] C. Hettlage, K. Mannheim, and J. G. Learned, “The Sun as a high-energyneutrino source,” Astropart.Phys., vol. 13, pp. 45–50, 2000.[75] G. Wikstrom and J. Edsjo, “Limits on the WIMP-nucleon scattering crosssectionfrom neutrino telescopes,” JCAP, vol. 0904, p. 009, 2009.[76] J. Edsjo, “Wimpsim web tool,” http: // www. physto. se/ ~edsjo/wimpsim/ scripts. html .[77] T. Sjostrand, S. Mrenna, and P. Z. Skands, “PYTHIA 6.4 Physics and Manual,”JHEP, vol. 0605, p. 026, 2006.[78] S. Fukuda et al., “Determination of solar neutrino oscillation parametersusing 1496 days of Super-Kamiokande I data,” Phys.Lett., vol. B539,pp. 179–187, 2002.[79] Y. Ashie et al., “Evidence for an oscillatory signature in atmospheric neutrinooscillation,” Phys.Rev.Lett., vol. 93, p. 101801, 2004.[80] Q. Ahmad et al., “Direct evidence for neutrino flavor transformationfrom neutral current interactions in the Sudbury Neutrino Observatory,”Phys.Rev.Lett., vol. 89, p. 011301, 2002.[81] E. Aliu et al., “Evidence for muon neutrino oscillation in an acceleratorbasedexperiment,” Phys.Rev.Lett., vol. 94, p. 081802, 2005.[82] Yao, W.-M. et al., “Review of Particle Physics,” Journal of Physics G,vol. 33, pp. 1+, 2006.[83] L. Wolfenstein, “Neutrino oscillations in matter,” Physical Review D 17,2369 (1978).[84] A. Y. S. S. P. Mikheyev, “Resonance amplification of oscillations in matterand spectroscopy of solar neutrinos,” Soviet Journal of Nuclear Physics42,913 (1985).[85] M. Maltoni, T. Schwetz, M. Tortola, and J. Valle, “Status of global fits toneutrino oscillations,” New J.Phys., vol. 6, p. 122, 2004.[86] M. Blennow, J. Edsjo, and T. Ohlsson, “Neutrinos from WIMP annihilationsusing a full three-flavor Monte Carlo,” JCAP, vol. 0801, p. 021, 2008.[87] D. J. Griffiths, “Introduction to Electrodynamics,” PHI learning.160
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