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arXiv · 1411.5126

Superluminous Supernovae Powered by Magnetars: Late-time Light Curves and Hard Emission Leakage

S. Q. Wang·L. J. Wang·Z. G. Dai·X. F. Wu
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Abstract

Recently, researches performed by two groups have revealed that the magnetar spin-down energy injection model with full energy trapping can explain the early-time light curves of SN 2010gx, SN 2013dg, LSQ12dlf, SSS120810 and CSS121015, but fails to fit the late-time light curves of these Superluminous Supernovae (SLSNe). These results imply that the original magnetar-powered model is challenged in explaining these SLSNe. Our paper aims to simultaneously explain both the early- and late-time data/upper limits by considering the leakage of hard emissions. We incorporate quantitatively the leakage effect into the original magnetar-powered model and derive a new semi-analytical equation. Comparing the light curves reproduced by our revised magnetar-powered model to the observed data and/or upper limits of these five SLSNe, we found that the late-time light curves reproduced by our semi-analytical equation are in good agreement with the late-time observed data and/or upper limits of SN 2010gx, CSS121015, SN 2013dg and LSQ12dlf and the late-time excess of SSS120810, indicating that the magnetar-powered model might be responsible for these SLSNe and that the gamma ray and X-ray leakage are unavoidable when the hard photons were down-Comptonized to softer photons. To determine the details of the leakage effect and unveil the nature of SLSNe, more high quality bolometric light curves and spectra of SLSNe are required.

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S. Q. Wang, L. J. Wang, Z. G. Dai, X. F. Wu. 2014-11-19. Superluminous Supernovae Powered by Magnetars: Late-time Light Curves and Hard Emission Leakage. https://doi.org/10.1088/0004-637x%2F799%2F1%2F107

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