Thermonuclear explosions of rapidly differentially rotating white dwarfs: Candidates for superluminous Type Ia supernovae?

@article{Fink2018ThermonuclearEO,
  title={Thermonuclear explosions of rapidly differentially rotating white dwarfs: Candidates for superluminous Type Ia supernovae?},
  author={Michael Fink and Markus Kromer and W Hillebrandt and Friedrich K. Roepke and R{\"u}ediger Pakmor and Ivo R. Seitenzahl and Stuart A. Sim},
  journal={Astronomy \& Astrophysics},
  year={2018}
}
The observed sub-class of “superluminous” Type Ia supernovae lacks a convincing theoretical explanation. If the emission of such objects were powered exclusively by radioactive decay of 56Ni formed in the explosion, a progenitor mass close to or even above the Chandrasekhar limit for a non-rotating white dwarf star would be required. Masses significantly exceeding this limit can be supported by differential rotation. We, therefore, explore explosions and predict observables for various… 

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