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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Case study of four GRBs finds afterglow light curves shaped by ambient density, not prompt fireball composition, with cascade pairs affecting only long GRB early optical emission.
citing papers explorer
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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.
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Do Prompt Gamma-ray Burst Fireball Composition Impact on Afterglow Emission? Cases Study for Long GRBs 080916C/090902B and Short GRBs 090510/130603B
Case study of four GRBs finds afterglow light curves shaped by ambient density, not prompt fireball composition, with cascade pairs affecting only long GRB early optical emission.