Image Details

Choose export citation format:

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 3.

Top: the neutrino spectral energy luminosity at different time slices, with the blue lines for the calculation boundaries and the gray ones for in-between times. The blue curves denote the onset and end of the neutrino calculation, t = 5.74 and 100.59 days after core collapse, respectively, while the gray curves show intermediate epochs. Bottom: the total energy luminosity of SN neutrinos as a function of days from the core collapse. Here, the sum of six neutrino flavors (﹩{\nu }_{e}+{\bar{\nu }}_{e}+{\nu }_{\mu }+{\bar{\nu }}_{\mu }+{\nu }_{\tau }+{\bar{\nu }}_{\tau }﹩) is shown in both panels.

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse