What makes blazar jets cool ?, Anton Dmytriiev
30 juin 2022
30 juin 2022
Blazar flares are perfect phenomena to probe the extreme physics of relativistic outflows. The key method for this task is physical modeling of (...)
Liste des Séminaires
Vous trouverez ci-dessous la liste des séminaires organisés par le Luth.
Vous pouvez voir les enregistrements des précédents séminaires sur notre chaîne sur la plateforme de vidéos en ligne de l’Observatoire de Paris : https://astrotube.obspm.fr/c/luth_seminar/videos
Prochains Seminaires
What makes blazar jets cool ?, Anton Dmytriiev
Scattering Transforms in astrophysics, application to components separation, Erwan Allys
16 juin 2022
16 juin 2022
New statistical descriptions related to the so-called Scattering Transform recently obtained attractive results for several astrophysical (...)
Cosmic-ray confinement and Non-thermal emission in star-forming galaxies, Paula Kornecki
9 juin 2022
9 juin 2022
Cosmic rays (CRs) are responsible for a tight correlation between the star formation rate (SFR) and the radio/gamma-ray luminosity observed in (...)
Friction in superfluids : the curious case of neutron stars, Marco Antonelli
2 juin 2022
2 juin 2022
The defining property of superfluids is their ability to flow without friction. However, the presence of quantized vortices can open new (...)
GRMHD simulations of neutron star mergers with weak interactions, Luciani Combi
31 mai 2022
31 mai 2022
Predicting electromagnetic signals from binary neutron star mergers is a multi-scale, multi-physics problem. The only multi-messenger event (...)
Boundary conditions and energy in general relativity, Simone Speziale
19 mai 2022
19 mai 2022
Even though general relativity lacks a notion of local energy density, Noether theorem can be used to single out a quasi-local energy in many (...)
