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Statut |
Confirmé |
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Série |
SEM-GRECO |
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Domaines |
astro-ph |
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Date |
Lundi 30 Novembre 2020 |
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Heure |
11:00 |
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Institut |
IAP |
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Salle |
Webinar (contact pitrou@iap.fr for details) |
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Nom de l'orateur |
Pascal |
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Prenom de l'orateur |
Aurélien |
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Addresse email de l'orateur |
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Institution de l'orateur |
LUTH, Observatoire de Paris |
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Titre |
The role of neutrinos in supernovae and neutron star formation |
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Résumé |
If the main features of the core-collapse supernova mechanism are now understood, some important details about the microphysics are still subject to a lot of uncertainties. In particular, neutrinos are playing a key role in the core-collapse mechanism but interactions rates between neutrinos and dense matter are still poorly understood. In this talk, I will start by reviewing what we actually know about core-collapse supernovae and neutron star formation by focusing on the role of neutrinos. Then I will present a code for proto-neutron star evolution and some studies we have been conducting on the influence of neutrino - dense matter interactions on core-collapse and (proto-)neutron star cooling. |
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Numéro de preprint arXiv |
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Commentaires |
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Fichiers attachés |
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