Probing the cosmic ray mass composition in the knee region through TeV secondary particle fluxes from solar surroundings

Prabir Banik, Biplab Bijay, Samir K. Sarkar, and Arunava Bhadra
Phys. Rev. D 95, 063014 – Published 22 March 2017

Abstract

The possibility of estimating the mass composition of primary cosmic rays above the knee of their energy spectrum through the study of high-energy gamma rays, muons, and neutrinos produced in the interactions of cosmic rays with solar ambient matter and radiation is explored. It is found that the theoretical fluxes of TeV gamma rays, muons, and neutrinos from a region around 15° of the Sun are sensitive to a mass composition of cosmic rays in the PeV energy range. The experimental prospects for the detection of such TeV gamma rays/neutrinos by future experiments are discussed.

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  • Received 27 June 2016

DOI:https://doi.org/10.1103/PhysRevD.95.063014

© 2017 American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & Astrophysics

Authors & Affiliations

Prabir Banik*, Biplab Bijay, Samir K. Sarkar, and Arunava Bhadra

  • High Energy & Cosmic Ray Research Centre, University of North Bengal, Siliguri, West Bengal 734013, India

  • *pbanik74@yahoo.com
  • Corresponding Author. aru_bhadra@yahoo.com

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Issue

Vol. 95, Iss. 6 — 15 March 2017

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