Evolution of Hard X-ray Radiation from Clusters of Galaxies

@inproceedings{Takizawa2001EvolutionOH,
  title={Evolution of Hard X-ray Radiation from Clusters of Galaxies},
  author={Motokazu Takizawa},
  year={2001}
}
We have calculated the evolution of a non-thermal electron population from super-thermal (but weakly relativistic) to highly relativistic energy range in clusters of galaxies. We investigate the evolution of hard X-ray radiation due to both bremsstrahlung and inverse Compton scattering of the cosmic microwave background photons. The bremsstrahlung component is more significant than that of inverse Compton scattering when the momentum spectra of the electron sources are steeper than ∼ P −3.0 e… Expand

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