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Energy estimation of ultra-high energy cosmic ray hadrons by monte carlo simulations of extensive air showers

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dc.contributor.author Geranios, A en
dc.contributor.author Koutsokosta, D en
dc.contributor.author Mastichiadis, A en
dc.contributor.author Malandraki, O en
dc.contributor.author Rosaki-Mavrouli, H en
dc.contributor.author Maltezos, S en
dc.date.accessioned 2014-03-01T01:33:22Z
dc.date.available 2014-03-01T01:33:22Z
dc.date.issued 2010 en
dc.identifier.issn 0217-751X en
dc.identifier.uri https://dspace.lib.ntua.gr/xmlui/handle/123456789/20395
dc.subject Cosmic rays en
dc.subject Energy estimation en
dc.subject UHECR en
dc.subject.classification Physics, Nuclear en
dc.subject.classification Physics, Particles & Fields en
dc.title Energy estimation of ultra-high energy cosmic ray hadrons by monte carlo simulations of extensive air showers en
heal.type journalArticle en
heal.identifier.primary 10.1142/S0217751X10049372 en
heal.identifier.secondary http://dx.doi.org/10.1142/S0217751X10049372 en
heal.language English en
heal.publicationDate 2010 en
heal.abstract Ultra-High Energy Cosmic Rays (E < 5 ×1019 eV) are detected through Extensive Air Showers that are created when a primary cosmic ray particle interacts with the atmosphere of the Earth. The energy of the primary particle can be estimated experimentally based on simulations. In this paper we attempt to estimate the energy of UHECR hadrons (He, Li, C, Fe) by applying a Monte Carlo simulation code and we compare the results with the ones derived in our previous paper for proton initiated showers. The scenario of simulations is adapted to the P. Auger Observatory site. © 2010 World Scientific Publishing Company. en
heal.publisher WORLD SCIENTIFIC PUBL CO PTE LTD en
heal.journalName International Journal of Modern Physics A en
dc.identifier.doi 10.1142/S0217751X10049372 en
dc.identifier.isi ISI:000277688800011 en
dc.identifier.volume 25 en
dc.identifier.issue 12 en
dc.identifier.spage 2561 en
dc.identifier.epage 2571 en


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