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09:00
TBA
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Kenta Hotokezaka
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09:30
Explodability and explosion energies of neutrino-driven supernovae
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Kiril Maltsev
(MPIA)
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09:50
Signatures of the first stars among local extremely-metal-poor descendants
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Francesco Gabrielli
(Uppsala University)
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11:10
Implications for the 12C(α,γ)16O Reaction Rate from G292.0+1.8
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Mitsuki Kubo
(Department of Earth Science and Astronomy, Graduate School of Arts and Sciences, The University of Tokyo)
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11:30
Clues for the Origin of the Heaviest Elements
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Friedrich Thielemann
(University of Basel)
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11:50
Time Evolution of Dust Formation and Infrared Emission in Failed Supernovae
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Kengo Shinoda
(University of tokyo)
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13:30
TBA
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Christine Collins
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14:00
Mapping Helium-Burning Rate Sensitivities for 56Ni Production in Pair-Instability Supernovae
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Hiroki KAWASHIMO
(The University of Tokyo, Komaba)
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15:40
Rethinking chemical evolution
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Ralph Schoenrich
(University College London)
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16:00
Grey M1 Photon Transport in Aenus-ALCAR: Towards 3D Supernovae from Core Collapse to Shock Breakout
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Giorgio La Malfa
(University of Valencia)
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16:20
Illuminating nebular phase supernovae with 3D NLTE radiative transfer modelling
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Bart van Baal
(University of Turku)
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17:00
meeting of Gruber Laureates 2026 with students