Ultra-High Energy Cosmic Rays and the GeV-TeV Diffuse Gamma-Ray Flux
arXiv:0704.2463 · doi:10.1103/PhysRevD.79.063005
Abstract
Ultra-high energy cosmic ray protons accelerated in astrophysical objects produce secondary electromagnetic cascades during propagation in the cosmic microwave and infrared backgrounds. We show that such cascades can contribute between ~1% and ~50% of the GeV-TeV diffuse photon flux measured by the EGRET experiment. The GLAST satellite should have a good chance to discover this flux.
4 pages, 5 figures
References in corpus (21)
- First Observation of the Greisen-Zatsepin-Kuzmin Suppression
- Observation of the suppression of the flux of cosmic rays above 4x10^19eV
- UV Luminosity Functions at z~4, 5, and 6 from the HUDF and other Deep HST ACS Fields: Evolution and Star Formation History
- A galaxy at a redshift z = 6.96
- The Starburst Contribution to the Extra-Galactic Gamma-Ray Background
- A dip in the UHECR spectrum and the transition from galactic to extragalactic cosmic rays
- Search for ultra-high energy photons using air showers
- The intergalactic propagation of ultra-high energy cosmic ray nuclei
- Predictions for the Cosmogenic Neutrino Flux in Light of New Data from the Pierre Auger Observatory
- Rapid Evolution in the Most Luminous Galaxies During the First 900 Million Years
- Statistics of Cosmological Black Hole Jet Sources: Blazar Predictions for GLAST
- Ultra-high energy cosmic rays, cascade gamma-rays, and high-energy neutrinos from gamma-ray bursts
- CRPropa: A Numerical Tool for the Propagation of UHE Cosmic Rays, Gamma-rays and Neutrinos
- The Signature of Large Scale Structures on the Very High Energy Gamma-Ray Sky
- Angular Signatures of Dark Matter in the Diffuse Gamma Ray Background
- TeV gamma-rays from photo-disintegration/de-excitation of cosmic-ray nuclei
- GZK Photons in the Minimal Ultra High Energy Cosmic Rays Model
- GZK Photons Above 10 EeV
- Non-Universal Spectra of Ultra-High Energy Cosmic Ray Primaries and Secondaries in a Structured Universe
- Gamma ray signatures of ultra high energy cosmic ray accelerators: electromagnetic cascade versus synchrotron radiation of secondary electrons
- Composition of UHECR and the Pierre Auger Observatory Spectrum
Cited by in corpus (36)
- The Spectrum of the Isotropic Diffuse Gamma-Ray Emission Derived From First-Year Fermi Large Area Telescope Data
- GZK Neutrinos after the Fermi-LAT Diffuse Photon Flux Measurement
- Dark Matter Searches with Astroparticle Data
- Angular, spectral, and time distributions of highest energy protons and associated secondary gamma-rays and neutrinos propagating through extragalactic magnetic and radiation fields
- The nature of the Diffuse Gamma-Ray Background
- Extragalactic propagation of ultrahigh energy cosmic-rays
- Anisotropies in the diffuse gamma-ray background measured by the Fermi LAT
- Components of the Extragalactic Gamma Ray Background
- Gamma-ray induced cascades and magnetic fields in intergalactic medium
- Circum-Galactic Gas and the Isotropic Gamma Ray Background
- Gamma-Ray and Neutrino Backgrounds as Probes of the High-Energy Universe: Hints of Cascades, General Constraints, and Implications for TeV Searches
- Diffuse gamma-ray emission from galactic pulsars
- Deciphering Contributions to the Extragalactic Gamma-Ray Background from 2 GeV to 2 TeV
- Characterization of Dark-Matter-induced anisotropies in the diffuse gamma-ray background
- The diffuse gamma-ray flux associated with sub-PeV/PeV neutrinos from starburst galaxies
- Cosmogenic gamma-rays and the composition of cosmic rays
- Constraints on the origin of ultra-high-energy cosmic rays from cosmogenic neutrinos and photons
- Identifying Dark Matter Annihilation Products In The Diffuse Gamma Ray Background
- Testing gamma-ray models of blazars in the extragalactic sky
- Anisotropies in the Diffuse Gamma-Ray Background from Dark Matter with Fermi LAT: a closer look
- Parameter constraints in a near-equipartition model with multi-frequency \emph{NuSTAR}, \emph{Swift} and \emph{Fermi-LAT} data from 3C 279
- Constraining the Emissivity of Ultrahigh Energy Cosmic Rays in the Distant Universe with the Diffuse Gamma-ray Emission
- Gamma-ray luminosity function of BL Lac objects and contribution to the extragalactic gamma-ray background
- The Spectral Shape and Photon Fraction as Signatures of the GZK-Cutoff
- Galactic-Centre Gamma Rays in CMSSM Dark Matter Scenarios
- The Effect of Blazar Spectral Breaks on the Blazar Contribution to the Extragalactic Gamma-ray Background
- Constraining Dark Matter Properties with Gamma-Rays from the Galactic Center with Fermi-LAT
- Characterising the signatures of star-forming galaxies in the extra-galactic -ray background
- Extragalactic Very-High-Energy gamma-ray background
- A self-consistent interpretation of the GeV-TeV emission from a distant blazar PKS 1424+240
- Constraints on dark matter and astrophysics from tomographic -ray cross-correlations
- Observable spectral and angular distributions of -rays from extragalactic ultrahigh energy cosmic ray accelerators: the case of extreme TeV blazars
- Ultra High Energy Cosmic Ray, Neutrino, and Photon Propagation and the Multi-Messenger Approach
- Conservative upper limits on WIMP annihilation cross section from Fermi-LAT -rays
- KiDS-Legacy: WIMP dark matter constraints from the cross-correlation of weak lensing and Fermi-LAT gamma rays
- Extragalactic Searches for Dark Matter Annihilation