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Estimation of 56Ni Needed in the Explosion Process of the Super Luminous Supernova ASASSN-15lh
Authors:Feng Dan-dan  Liu Men-quan  Luo Xia  Luo Zhi-quan  Feng Zhong-wen  Tang De-lin
Institution:1. Department of Astronomy, China West Normal University, Nanchong 637002;2. Department of Astronomy, Beijing Normal University, Beijing 100875
Abstract:ASASSN-15lh is a super luminous supernova, whose light curve is similar to that of the type Ia supernova (SN Ia). Since the luminosity of SN Ia is directly related to the decay of 56Ni, in this paper, we consider the de-excitation energy of the new nuclei, and calculate the energy generated by the decay of 56Ni in the explosive environment of ASASSN-15lh. The calculated mass of 56Ni needed by the ASASSN-15lh explosion is 31.32 M. This result agrees with the estimation of the mass of 56Ni ≥ 30 M derived from the observed light curve of ASASSN-15lh. No agreement has reached for the explosion mechanism of supernova ASASSN-15lh so far. The calculation in this paper provides a reference for the further study on the progenitor and explosion mechanism of the supernova ASASSN-15lh.
Keywords:supernovae: general—supernovae: individual: ASASSN-15lh— nuclear reactions—stars: evolution
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