A theoretical color-velocity correlation for supernovae associated with gamma-ray bursts
Sharon Rapoport, Stuart A. Sim, Keiichi Maeda, Masaomi Tanaka, Markus, Kromer, Brian P. Schmidt, Kenichi Nomoto

TL;DR
This paper presents multi-dimensional radiative transfer models of supernovae with bipolar outflows, predicting orientation-dependent spectral and light curve features, including a correlation between line velocity and color that aids in identifying jet-driven supernovae.
Contribution
It introduces the first multi-dimensional radiative transfer calculations for aspherical supernova models, revealing orientation-dependent observable features and a consistent line velocity-color correlation.
Findings
Spectral and light curve features vary systematically with observer orientation.
Early phase light curves are brighter and bluer near the polar axis.
A consistent correlation between line velocity and color is predicted.
Abstract
We carry out the first multi-dimensional radiative transfer calculations to simultaneously compute synthetic spectra and light curves for models of supernovae driven by fast bipolar outflows. These allow us to make self-consistent predictions for the orientation dependence of both colour evolution and spectral features. We compare models with different degrees of asphericity and metallicity and find significant observable consequences of both. In aspherical models, we find spectral and light curve features that vary systematically with observer orientation. In particular, we find that the early phase light curves are brighter and bluer when viewed close to the polar axis but that the peak flux is highest for equatorial (off-axis) inclinations. Spectral line features also depend systematically on observer orientation, including the velocity of the SiII 6355A line. Consequently, our…
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