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2013

An exact integral relation between the Ni56 mass and the bolometric light curve of a type Ia supernova

Katz, Boaz, Kushnir, Doron, Dong, Subo

Understand

An exact relation between the Ni56 mass and the bolometric light curve of a type Ia supernova can be derived as follows, using the following excellent approximations: 1.

  • the emission is powered solely by Ni56-> Co56 ->Fe56; 2.
  • each mass element propagates at a non-relativistic velocity which is constant in time (free coasting); and 3.
  • the internal energy is dominated by radiation.

Built on

  • Colgate, S. A., & McKee, C. 1969, ApJ, 157, 623

    1969

    Earlier work this paper cites.

  • Arnett, W. D. 1979, ApJ, 230, L37

    1979

    Earlier work this paper cites.

Similar

  • Colgate, S. A., Petschek, A. G., & Kriese, J. T. 1980, ApJ, 237, L81

    1980

    Cited alongside, same era.

  • Arnett, W. D. 1982, ApJ, 253, 785

    1982

    Cited alongside, same era.

Then

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