Ultrahigh energy cosmic rays as a Grand Unification signal

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dc.creatorFodor, Z.
dc.creatorKatz, S. D.
dc.date2001-05-31
dc.date.accessioned2026-07-07T03:44:40Z
dc.date.available2026-07-07T03:44:40Z
dc.descriptionWe analyze the spectrum of the ultrahigh energy (above \approx 10^{9} GeV) cosmic rays. With a maximum likelihood analysis we show that the observed spectrum is consistent with the decay of extragalactic GUT scale particles. The predicted mass for these superheavy particles is m_X=10^b GeV, where b=14.6_{-1.7}^{+1.6}.
dc.description4 pages, 3 figures, talk to be presented at the 27th International Cosmic Ray Conference, Hamburg, Germany, August 7-15, 2001
dc.identifierhttps://arxiv.org/abs/hep-ph/0105348
dc.identifierhttp://arxiv.org/abs/hep-ph/0105348
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/40657
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.titleUltrahigh energy cosmic rays as a Grand Unification signal
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