Institution(s): 1. Gauhati University
The gamma ray emission from Dark Matter annihilation in the dwarf spheroidal galaxy Draco has been studied. Dwarf Spheroidal (dSph) galaxies are through to be the repository of dark matter due to their high mass to light ratio. Draco is believed to emit energy due to certain dark matter candidates. One of the most motivated dark matter appears to be the neutralino as predicted in the Minimal Supersymmetric Standard model(MSSM). The mass of the neutralino is constrained to be in the range 6GeV to 100TeV by the CMB measurements and accelerator searches. Gamma Ray Spectra and fluxes have been calculated for neutral no annihilation over a mass range (10-100) GeV. The gamma ray flux from the annihilation of 100GeVneutralino in the dSph galaxy Draco is found to be ~1.6x10^(-10) cm^(-2)s^(-1)GeV^(-1) . This is found to be agreeable with the observed flux as measured from a NFW density profile for dark matter distribution in Draco. The gamma ray distribution for neutral no annihilation shows a maximum value near the centre and found to falls off as radially.