Deuteron and antideuteron production simulation in cosmic-ray interactions

Diego-Mauricio Gomez-Coral, Arturo Menchaca Rocha, Varlen Grabski, Amaresh Datta, Philip von Doetinchem, and Anirvan Shukla
Phys. Rev. D 98, 023012 – Published 12 July 2018

Abstract

The study of the cosmic-ray deuteron and antideuteron flux is receiving increasing attention in current astrophysics investigations. For both cases, an important contribution is expected from the nuclear interactions of primary cosmic rays with intergalactic matter. In this work, deuteron and antideuteron production from 20 to 2.6×107GeV beam energy in p+p and p+A collisions were simulated using EPOS-LHC and Geant4’s FTFP-BERT Monte Carlo models by adding an event-by-event coalescence model afterburner. These estimates depend on a single parameter (p0) obtained from a fit to the data. The p0 for deuterons in this wide energy range was evaluated for the first time. It was found that p0 for antideuterons is not a constant at all energies as previous works suggested and, as a consequence, the antideuteron production cross section can be at least 20 times smaller in the low-collision-energy region than earlier estimations.

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  • Received 10 February 2018

DOI:https://doi.org/10.1103/PhysRevD.98.023012

© 2018 American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & Astrophysics

Authors & Affiliations

Diego-Mauricio Gomez-Coral*, Arturo Menchaca Rocha, and Varlen Grabski

  • Instituto de Física, Universidad Nacional Autónoma de México, Circuito de la Investigación Científica, Ciudad de México 04510, México

Amaresh Datta, Philip von Doetinchem, and Anirvan Shukla

  • Department of Physics and Astronomy, University of Hawaii at Manoa, 2505 Correa Rd, Honolulu, Hawaii 96822, USA

  • *diegomez@estudiantes.fisica.unam.mx

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Issue

Vol. 98, Iss. 2 — 15 July 2018

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