The light curve in supernova modeled by a continuous radioactive decay of ⁵⁶Ni
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🌌 astro-ph.SR
keywords
radioactivecontinuousdecaylightmodeledorderabsoluteapparent
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The UVOIR bolometric light curves are usually modeled by the radioactive decay. In order to model more precisely the absolute/apparent magnitude versus time relationship the continuous production of radioactive isotopes is introduced. A differential equation of the first order with separable variables is solved.
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