A one-zone radioactive heating model with macroscopic nickel-oxygen mixing reproduces the [O III] luminosity of SN 2018ibb and yields a scaling relation for line strength among PISNe.
The power deposited in the oxy gen matter by gamma-quanta of 56Co decay is Ld(O) = ( MO/M)L
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PISN 2018ibb: radioactive emission of [O III] lines
A one-zone radioactive heating model with macroscopic nickel-oxygen mixing reproduces the [O III] luminosity of SN 2018ibb and yields a scaling relation for line strength among PISNe.