TARDIS gamma \(\gamma\)

This code module simulates the propagation of \(\gamma\)-ray photons through the ejecta and can be used to study high energy phenomenon within the ejecta as well as the energy deposition of \(\gamma\)-rays and positrons.

Type Ia supernovae produce a large amount of energy from \(\gamma\)-rays produced from the radioactive decay of ⁵⁶ Ni and ⁵⁶ Co. These photons often are not able to escape the ejecta until later times in the supernova when the density decreases. Once the \(\gamma\)-rays are able to escape they can provide information about the mass and distribution of radioactive isotopes created in the supernova.

• Packet Initialization