Accession Number : ADA521427


Title :   Nonthermal Particles and Radiation Produced by Cluster Merger Shocks


Descriptive Note : Journal article


Corporate Author : NAVAL RESEARCH LAB WASHINGTON DC


Personal Author(s) : Berrington, Robert C ; Dermer, Charles D


Full Text : https://apps.dtic.mil/dtic/tr/fulltext/u2/a521427.pdf


Report Date : 10 Sep 2003


Pagination or Media Count : 24


Abstract : We have developed a numerical model for the temporal evolution of particle and photon spectra resulting from nonthermal processes at the shock fronts formed in merging clusters of galaxies. Fermi acceleration is approximated by injecting power-law distributions of particles during a merger event, subject to constraints on maximum particle energies. We consider synchrotron, bremsstrahlung, Compton, and Coulomb processes for the electrons, nuclear, photomeson, and Coulomb processes for the protons, and knock-on electron production during the merging process. The broadband radio through gamma-ray emission radiated by nonthermal protons and primary and secondary electrons is calculated both during and after the merger event. Using ROSAT observations to establish typical parameters for the matter density profile of clusters of galaxies, we find that typical merger shocks are weak and accelerate particles with relatively soft spectra. We consider the prospects for detecting nonthermal radio and gamma-ray emission from clusters of galaxies and implications for the origin of ultra-high-energy cosmic rays and the diffuse gamma-ray background. Our results suggest that only a few of the isotropically distributed unidentified EGRET sources are due to shocks formed in cluster mergers and that only a minor contribution to the diffuse extragalactic gamma-ray background can originate from cluster merger shocks. Cluster merger shocks can accelerate protons to 10(19) eV for the standard parameters considered here. We predict that GLAST will detect several cluster mergers, and depending on the mean magnetic fields in the intracluster medium, the Low Frequency Array could detect anywhere from several to several hundred.


Descriptors :   *SHOCK WAVES , *GALAXIES , *CLUSTERING , DENSITY , MAGNETIC FIELDS , ENERGY , FERMI SURFACES , PROTONS , ELECTRONS , SPECTRA , PARTICLES , GAMMA RAYS , PHOTONS , SECONDARY EMISSION , DIFFUSION , SYNCHROTRONS , BREMSSTRAHLUNG , REPRINTS , EXTRATERRESTRIAL RADIO WAVES , MATHEMATICAL MODELS , EMISSION


Subject Categories : Astrophysics


Distribution Statement : APPROVED FOR PUBLIC RELEASE