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Energy dependence of σp-air up to 20 TeV
Authors:TK Gaisser  GB Yodh
Institution:Bartol Research Foundation of The Franklin Institute, Swarthmore, Pennsylvania 19081, USA;Physics Department, University of Maryland, College Park, Maryland 20742, USA
Abstract:The observed neutral to charge ratio in unaccompanied atmospheric hadron fluxes is used to improve the cosmic ray lower bound on the p-air inelastic cross section between 0.5 and 20 TeV. The conclusion drawn about the magnitude of continued increase of σpp between 2 and 20 TeV depends on the model relation between σpp and σp-air.
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