Secondary neutrino and gamma-ray fluxes from SimProp and CRPropa

Abstract

The interactions of ultra-high-energy cosmic rays (UHECRs) in extragalactic space with photons of the cosmic microwave background (CMB) and extragalactic background light (EBL) can generate high-energy neutrinos and photons. Simulations of UHECR propagation require knowledge about physical quantities such as the spectrum of the EBL and photodisintegration cross sections. These assumptions, as well as the approximations used in the codes, may influence the computed UHECR spectrum and composition, and the associated cosmogenic neutrino and photon fluxes. Following up on our previous work where we studied the effects of these uncertainties on the UHECR spectrum and composition, here we quantify those on neutrino fluxes and production rates of photons, electrons, and positrons, using the Monte Carlo codes CRPropa and SimProp, in various astrophysical scenarios. We show that cosmogenic neutrinos are more sensitive to the choice of EBL model than UHECRs, whereas the overall cosmogenic gamma-ray production rates are relatively independent of propagation details. We also find significant differences between neutrino fluxes predicted by the latest released versions of CRPropa and SimProp, and discuss their causes and possible improvements in future versions of the codes.

1+26 pages, 12 figures, 1 table; typo fixes and other minor changes

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Cited by in corpus (10)

• CRPropa 3.2 -- an advanced framework for high-energy particle propagation in extragalactic and galactic spaces
• Ultra-High-Energy Cosmic Rays: The Intersection of the Cosmic and Energy Frontiers
• The Gamma-Ray Window to Intergalactic Magnetism
• Constraining the sources of ultra-high-energy cosmic rays across and above the ankle with the spectrum and composition data measured at the Pierre Auger Observatory
• White Paper and Roadmap for Quantum Gravity Phenomenology in the Multi-Messenger Era
• Probing Cosmic-Ray Accelerated Light Dark Matter with IceCube
• UHECR mass composition at highest energies from anisotropy of their arrival directions
• Probing UHECR production in Centaurus A using secondary neutrinos and gamma-rays
• Evaluations of uncertainties in simulations of propagation of ultrahigh-energy cosmic-ray nuclei derived from microscopic nuclear models
• Cosmogenic neutrinos as probes of new physics