Registration of Particles Delayed by 400 1000 Microsec after EAS

Details Registration of Particles Delayed by 400 1000 Microsec after EAS Registration of Particles Delayed by 400 1000 Microsec after EAS

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....1...45g&link_type=abstract

Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I

Physics

1

Scientific paper

Particles are detected up to 2 milliseconds after the EAS front. These are likely to be neutrons. The scenario that these neutrons originate due to EAS hadron interactions is discussed. Neutrons evaporated from excited target nuclei diffuse and get thermalized and then diffuse and can be detected. The relation between number of detected neutrons and EAS hadron content is being investigated. We found that the time distribution of registered neutrons does not match distribution predicted by simulations using MCNP code.

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