Информация о цитировании статьи получена из
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Статья опубликована в журнале из списка Web of Science и/или Scopus
Дата последнего поиска статьи во внешних источниках: 18 июля 2013 г.
Аннотация:The present status of extensive air shower (EAS) simulation procedures is
reviewed. The advantages of combining numerical and Monte Carlo methods
for the description of EAS development are discussed. Physics content of
cosmic ray interaction models is briefly described and their predictions are
compared to the first LHC data. Finally, some outstanding puzzles related
to cosmic ray composition at the “ankle” energies are analyzed.