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Interaction-powered Type Ibn Supernovae as a Transient PeVatron Candidate: The Case of SN 2023uqf

  • Authors: Ryo Sawada, Yusuke Inoue, Yosuke Ashida

Ryo Sawada et al 2026 The Astrophysical Journal Letters 1005 .

  • Provider: AAS Journals

Caption: Figure 2.

RHD-derived shock evolution used as input to the neutrino calculation. Top: forward-shock radius Rsh(t). Middle: shock velocity Vsh(t). Bottom: CSM density encountered by the shock ρCSM(Rsh(t)). The vertical dashed line marks tonset = 5.74 days, after which collisionless acceleration is allowed in the neutrino calculation.

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