Constraints on dark matter annihilation with electron spectrum from VERITAS

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Cosmic-ray electrons (and positrons) can be used to probe self-annihilation or decay of dark matter particles. We have used spectrum of high energy cosmic-ray electrons between 300 GeV and 5 TeV measured by Very Energetic Radiation Imaging Telescope Array System (VERITAS) to constrain dark matter annihilation cross-section in the solar neighbourhood. A diffusion-loss equation with a canonical model has been used as a spectrum model function by assuming a NFW profile for the Milky Way halo. We have considered cosmic-ray electrons as products of annihilation of heavy dark matter particles (GeV -TeV). During the propagation through interstellar medium, the cosmic-ray electrons lose their energy due to synchrotron radiation, inverse-Compton scattering and ionization processes.