Publication Date:
2016-06-11
Description:
The interpretation of the experimental data in superhigh energy cosmic rays requires the calculations using various models of elementary hadron interaction. One should prefer the models justified by accelerator data and giving definite predictions for superhigh energies. The model of quark-gluon pomeron strings (the QGPS models) satisfies this requirement.
Keywords:
SPACE RADIATION
Type:
19th Intern. Cosmic Ray Conf - Vol. 7; p 44-47; NASA-CP-2376-VOL-7
Format:
application/pdf