Gamma-ray emission expected from Kepler's SNR

Abstract

Nonlinear kinetic theory of cosmic ray (CR) acceleration in supernova remnants (SNRs) is used to investigate the properties of Kepler's SNR and, in particular, to predict the gamma-ray spectrum expected from this SNR. Observations of the nonthermal radio and X-ray emission spectra as well as theoretical constraints for the total supernova (SN) explosion energy E_sn are used to constrain the astronomical and particle acceleration parameters of the system. Under the assumption that Kepler's SN is a type Ia SN we determine for any given explosion energy E_sn and source distance d the mass density of the ambient interstellar medium (ISM) from a fit to the observed SNR size and expansion speed. This makes it possible to make predictions for the expected gamma-ray flux. Exploring the expected distance range we find that for a typical explosion energy E_sn=10^51 erg the expected energy flux of TeV gamma-rays varies from 2x10^{-11} to 10^{-13} erg/(cm^2 s) when the distance changes from d=3.4 kpc to 7 kpc. In all cases the gamma-ray emission is dominated by π^0-decay gamma-rays due to nuclear CRs. Therefore Kepler's SNR represents a very promising target for instruments like H.E.S.S., CANGAROO and GLAST. A non-detection of gamma-rays would mean that the actual source distance is larger than 7 kpc.

6 pages, 4 figures. Accepted for publication in Astronomy and Astrophysics, minor typos corrected

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• Postshock turbulence and diffusive shock acceleration in young supernova remnants
• Cosmic Ray Acceleration by Supernova Shocks
• H.E.S.S. upper limits for Kepler's supernova remnant
• Radio Emission from Supernova Remnants: Implications for Post-Shock Magnetic Field Amplification and the Magnetic Fields of Galaxies
• Non-thermal emission from old supernova remnants
• Hadronic versus leptonic origin of gamma-ray emission from supernova remnants
• Inverse Compton gamma-ray models for remnants of Galactic type Ia supernovae?
• Evidence for gamma-ray emission from the remnant of Kepler's supernova based on deep H.E.S.S. observations
• CANGAROO-III Search for Gamma Rays from Kepler's Supernova Remnant