Ultra high energy cosmic rays: clustering, GUT scale and neutrino masses
by
Zoltan Fodor (Eotvos University, Budapest)
→
Europe/Zurich
TH Auditorium (CERN)
TH Auditorium
CERN
Description
Using the clustering properties of ultrahigh energy cosmic rays we determine the density of compact sources. We analyze the spectrum of the ultrahigh energy cosmic rays. With a maximum likelihood analysis we show that the observed spectrum is consistent with the decay of extragalactic GUT scale particles (predicted mass $m_X=10^b$ GeV, where $b=14.6_-1.7^+1.6$) or with a Z-burst scenario (neutrino mass $2.34^+1.29_-0.84$ eV or $0.26^+0.20_-0.14$ eV, assuming Galactic halo or extragalactic origin for the power part of the spectrum, respectively).