<script type="text/javascript">
<!--
document.write('<div id="oa_widget"></div>');
document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=undefined&type=result"></script>');
-->
</script>

COPY SCRIPT

For further information contact us at helpdesk@openaire.eu

Constraints of hadronic interaction models from the cosmic muon observations

descriptionPublicationkeyboard_double_arrow_right Article , Preprint 01 Jan 2015Embargo end date: 01 Jan 2015Publisher:EDP SciencesJournal:EPJ Web of Conferences, volume 99, page 10,003 (eissn: 2100-014X,

Authors: T. M. Roganova; L. G. Dedenko; A.V. Lukyashin; G. F. Fedorova;

doi: 10.1051/epjconf/20159910003 , 10.48550/arxiv.1504.05853

arXiv: http://arxiv.org/abs/1504.05853

Constraints of hadronic interaction models from the cosmic muon observations

- Summary
- Subjects
- Related research
  (1)
- Metrics

Abstract

A simple method of the vertical muon energy spectrum simulations have been suggested. These calculations have been carried out in terms of various models of hadronic interactions. The most energetic $ ��^\pm $-mesons and K$^\pm $-mesons produced in hadron interactions contribute mainly in to this energy spectrum of muons due to the very steep energy spectrum of the primary particles. So, some constraints on the hadronic interaction models may be set from a comparison of calculated results with the cosmic data on the vertical muon energy spectrum. This comparison showed that the most energetic secondary particles production is too high in case of the QGSJET II-04 model and rather low in case of the QGSJET II-03 model. These conclusion have been supported by the LHC data.

5 pages with 9 figures. (LaTeX template webofc.cls). This article is a contribution to proceedings of the conference International Symposium on Very High Energy Cosmic Ray Interactions 2014

Related Organizations

Lomonosov Moscow State University
Russian Federation
Moscow State University of Fine Chemical Technologies
Russian Federation

Keywords

High Energy Astrophysical Phenomena (astro-ph.HE), Physics, QC1-999, FOS: Physical sciences, Astrophysics - High Energy Astrophysical Phenomena

1 Research products, page of 1

Impact byBIP!

	citations This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).	11
	popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.	Average
	influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).	Average
	impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.	Top 10%