Session

S3

24 Aug 2026, 15:20

Conveners

S3

  • Seokhoon Yun (KNU)

Presentation materials

There are no materials yet.

  1. Edoardo Vitagliano (Max Planck Institute for Physics)
    24/08/2026, 15:20

    While it is way too early to make a final judgement, it is noteworthy that searches at LHC and direct detection experiments reported null results, therefore boosting the ever growing interest in sub-GeV dark sector candidates. Owing to their high temperature and density, the cores of proto-neutron stars, remnant of core-collapse supernovae and neutron star mergers, can be factories of axions...

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  2. Chui-Fan Kong (IBS-CTPU-PTC)
    24/08/2026, 16:00

    Core-collapse supernovae are powerful probes of physics beyond the Standard Model (BSM). In this talk, I will show how the circumstellar medium (CSM) affects supernova-based BSM searches using dark photons as an example. The decay product of dark photon can heat up CSM and lead to extra blackbody emission. Using the early-time observations of SN 2023ixf, we derive the strongest constraint on...

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  3. Mr Ju Hyeong Kang (Pusan National University)
    24/08/2026, 16:40

    We investigate supernova cooling bounds on an MeV-scale dark Z boson with mass mixing. For a dark Z much lighter than the Standard Model Z boson, the kinetic mixing contribution to its coupling with the neutral current is strongly suppressed, while the mass mixing contribution remains sizable. This allows the dark Z to be efficiently produced in the dense medium of a core-collapse supernova...

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