GRB 220101A is interpreted as the product of a pair-instability supernova plus a magnetized rotating core-collapse supernova in a CO-NS binary, extending the BdHN framework to seven episodes with pulsar formation replacing nickel decay in the final stage.
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Evidence for Two SNe Type Triggering GRB 220101A: a Pair SN and a Rotating Magnetized Core Collapse SN
GRB 220101A is interpreted as the product of a pair-instability supernova plus a magnetized rotating core-collapse supernova in a CO-NS binary, extending the BdHN framework to seven episodes with pulsar formation replacing nickel decay in the final stage.