Sensitivity of cosmic-ray experiments to ultra-high-energy photons: reconstruction of the spectrum and limits on the superheavy dark matter
arXiv:0812.1020 · doi:10.1103/PhysRevD.80.103006
Abstract
We estimate the sensitivity of various experiments detecting ultra-high-energy cosmic rays to primary photons with energies above 10^19 eV. We demonstrate that the energy of a primary photon may be significantly (up to a factor of ~ 10) under- or overestimated for particular primary energies and arrival directions. We consider distortion of the reconstructed cosmic-ray spectrum for the photonic component. As an example, we use these results to constrain the parameter space of models of superheavy dark matter by means of both the observed spectra and available limits on the photon content. We find that a significant contribution of ultra-high-energy particles (photons and protons) from decays of superheavy dark matter is allowed by all these constraints.
18 pages, 7 figures
References in corpus (10)
- Observation of the suppression of the flux of cosmic rays above 4x10^19eV
- Upper limit on the cosmic-ray photon flux above 10^19 eV using the surface detector of the Pierre Auger Observatory
- Search for ultra-high energy photons using air showers
- Upper limit on the ultra-high-energy photon flux from AGASA and Yakutsk data
- Upper limit on the photon fraction in highest-energy cosmic rays from AGASA data
- Constraining the fraction of primary gamma rays at ultra-high energies from the muon data of the Yakutsk extensive-air-shower array
- GZK Photons in the Minimal Ultra High Energy Cosmic Rays Model
- GZK Photons Above 10 EeV
- Global anisotropy of arrival directions of ultra-high-energy cosmic rays: capabilities of space-based detectors
- Spectral energy distributions and high-energy emission of BL Lac type objects
Cited by in corpus (19)
- Dark Matter Spectra from the Electroweak to the Planck Scale
- Regular black hole remnants and graviatoms with de Sitter interior as heavy dark matter candidates probing inhomogeneity of early universe
- Photon-axion mixing and ultra-high-energy cosmic rays from BL Lac type objects -- Shining light through the Universe
- Heavy decaying dark matter and IceCube high energy neutrinos
- Constraining heavy decaying dark matter with the high energy gamma-ray limits
- Upper limit on the flux of photons with energies above 10^19 eV using the Telescope Array surface detector
- Constraints on the flux of primary cosmic-ray photons at energies E > 10^18 eV from Yakutsk muon data
- Hunting for super-heavy dark matter with the highest-energy cosmic rays
- Constraints on the flux of eV cosmic photons from the EAS-MSU muon data
- Hadronically decaying heavy dark matter and high-energy neutrino limits
- Constraints on the proton fraction of cosmic rays at the highest energies and the consequences for cosmogenic neutrinos and photons
- Estimate of the fraction of primary photons in the cosmic-ray flux at energies ~10^17 eV from the EAS-MSU experiment data
- Particle Production in f(R) Gravity during Structure Formation
- Review of the Multimessenger Working Group at UHECR-2012
- Full Monte-Carlo description of the Moscow State University Extensive Air Shower experiment
- The local-filament pattern in the anomalous transparency of the Universe for energetic gamma rays
- Bounds from multi-messenger astronomy on the Super Heavy Dark Matter
- Report from the Multi-Messenger Working Group at UHECR-2014 Conference
- Some Observable Effects of Modified Gravity in Cosmology and Astrophysics