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What can we Learn from the Rising Light Curves of Radioactively Powered Supernovae?

  • Authors: Anthony L. Piro and Ehud Nakar

Piro & Nakar 2013 The Astrophysical Journal 769 67.

  • Provider: AAS Journals

Caption: Figure 8.

Comparisons on the light curves (shown in each top panel) for different distributions of 56Ni (shown in the bottom panels), when the full integrals are used for both the direct and diffusive tail heating according to Equation (B6). In the middle panels, we plot the ratio of the local heating rate L 56, which is usually what we wish to infer from the observations, to the total luminosity L.

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