# Constraining Type Ia Supernova Asymmetry with the Gamma-Ray Escape Timescale

## TL;DR

This study investigates how asymmetry in the distribution of radioactive nickel in Type Ia supernovae affects gamma-ray escape times, finding that asymmetry has a modest effect and both Chandrasekhar and sub-Chandrasekhar mass models are needed to explain observations.

## Contribution

It introduces a parameterized model of nickel asymmetry in SN Ia ejecta and constrains the asymmetry using gamma-ray escape times and observational data.

## Key findings

- Asymmetry has a modest effect on gamma-ray escape times.
- Single-mass models cannot explain the full diversity of observations.
- Both Chandrasekhar and sub-Chandrasekhar mass explosions are necessary.

## Abstract

We calculate the effects of an asymmetric $^{56}\mathrm{Ni}$ distribution in Type Ia supernova (SN Ia) ejecta on the gamma-ray escape timescale ($t_0$) that characterizes the late light curve ($>40$ days after peak) and find the effect is modest compared to other possible variations in ejecta structure. We parameterize asymmetry in the $^{56}\mathrm{Ni}$ distribution and calculate $t_0$ for a grid of SN ejecta models spanning a large volume of the asymmetry parameter space. The models have spherical density profiles while the $^{56}\mathrm{Ni}$ distribution in them has various levels of asymmetry. By placing constraints based on the observational measurement of $t_0$ and other general properties of SN Ia ejecta, we find the range of allowed asymmetry in the $^{56}\mathrm{Ni}$ distribution. Considering these constraints we find that some level of asymmetry in the distribution is not ruled out. However, models with a single ejecta mass and varying $^{56}\mathrm{Ni}$ distributions cannot explain the full range of observed $t_0$ values. This strengthens the claim that both Chandrasekhar mass and sub-Chandrasekhar mass explosions are required to explain the diversity of SN Ia observations.