Supernovae (SNe) are an extremely energetic phenomena. The recent discovery of new classes of SNe including Super-Luminous SNe (SLSNe) and double-humped SNe (DHSNe) have pushed the limits of current theory. Here we show some of our fits to SN light curves using the Quark Nova model.
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"Quark Nova Signatures in Super-luminous Supernovae", Kostka et al. Revista Mexicana de Astronomía y Astrofísica Vol. 50, pp. 167-180 (2014)
"Quark Nova Signatures in Super-luminous Supernovae", Kostka et al. Revista Mexicana de Astronomía y Astrofísica Vol. 50, pp. 167-180 (2014)
"Quark Nova Signatures in Super-luminous Supernovae", Kostka et al. Revista Mexicana de Astronomía y Astrofísica Vol. 50, pp. 167-180 (2014)
"Quark Nova Signatures in Super-luminous Supernovae", Kostka et al. Revista Mexicana de Astronomía y Astrofísica Vol. 50, pp. 167-180 (2014)
"Quark Nova Signatures in Super-luminous Supernovae", Kostka et al. Revista Mexicana de Astronomía y Astrofísica Vol. 50, pp. 167-180 (2014)
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