Energy dependent neutrino flavor ratios from cosmic accelerators on the Hillas plot

Astroparticle Physics

Volumn 34, Issue 4, 2010, Pages 205-224

  Hummer S ^a   Maltoni, M ^b   Winter, W ^a   Yaguna, C ^b  

^a UNIVERSITY OF WÜRZBURG   (Germany)

^b UNIVERSIDAD AUTÓNOMA DE MADRID   (Spain)

Author keywords

Astrophysical neutrinos; Cosmic rays

Indexed keywords

ACCELERATED ELECTRONS; ASTROPHYSICAL NEUTRINOS; CHARGED PIONS; DAMPED BEAM; DIRECT PRODUCTION; ENERGY DEPENDENT; ENERGY REGIONS; FLAVOR RATIOS; HELICITIES; HIGH ENERGY; HIGH ENERGY PROCESS; INTERACTION MODEL; MIXING PARAMETERS; MUON BEAM; MUON DECAYS; NEUTRINO FLUXES; NEUTRON DECAYS; NEUTRON INTERACTIONS; NEW SOURCES; ORDERS OF MAGNITUDE; PILE-UPS; THIN SOURCE;

ASTROPHYSICS; COSMIC RAYS; HADRONS; HIGH ENERGY PHYSICS; MAGNETIC FIELDS; NEUTRONS; RESONANCE; SYNCHROTRONS;

COSMOLOGY;

EID: 77956613161     PISSN: 09276505     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.astropartphys.2010.07.003     Document Type: Article

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