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"Discrepant hardenings" in cosmic ray spectra: a first estimate of the effects on secondary antiproton and diffuse gamma-ray yields
Discrepant hardenings cosmic ray spectra the effects on secondary antiproton
2011/1/11
Recent data from CREAM seem to confirm early suggestions that primary cosmic ray spectra at few TeV/nucleon are harder than in the 10-100 GeV range. Also, helium and heavier nuclei spectra appear syst...
Nonequilibrium ionization models for analysis of x-ray spectra of supernova remnants
x-ray spectra Nonequilibrium ionization models supernova remnants
2009/6/5
Nonequilibrium ionization models for analysis of x-ray spectra of supernova remnants。