Magnetic field formation and

evolution in neutron stars

PHAROS WG4+WG5 meeting and CoCoNuT Meeting 2018

CEA (Saclay, France), November 14-16, 2018

Scientific Programme

Wednesday 14
09:20     Opening
09:30 Francesco Coti Zelati Highly magnetic neutron stars: an observational update
10:30 Jose Pons Magnetic field evolution in magnetars: the influence of the magnetosphere
11:00 Coffee break
11:30 Francisco Castillo Magnetic field evolution in neutron star cores
12:00 Ashley Bransgrove Internal Dynamics of Neutron Star Magnetic Fields
13:00 Lunch break
14:30 Kostas Gourgouliatos Implications of Hall inverse cascades to Central Compact Objects
15:00 Samuel Lander Coupled evolution of inclination angle and spindown in newborn magnetars
15:30 Coffee break
16:00 Alejandro Torres-Forné Towards core-collapse parameter estimation with gravitational-waves
16:30 Tomasz Rembiasz
17:00 Discussion
Thursday 15
09:30 Basile Gallet Dynamo theory and experiments
10:30 Raphaël Raynaud Convective dynamo in protoneutron stars
11:00 Coffee break
11:30 Alexis Reboul-Salze Magnetorotational instability in protoneutron stars
12:00 Matteo Bugli The role of magnetic field topology in core-collapse supernovae simulations
13:00 Lunch break
14:30 Aurélien Pascal Impact of electron capture cross sections on nuclei far from stability on core-collapse supernovae
15:00 Anthea Fantina Cluster distribution and electron-capture rates in core-collapse supernova simulations
15:30 Coffee break
16:00 Rémi Kazeroni Impact of stellar rotation on core-collapse supernovae and the birth of neutron stars
16:30 Bruno Pagani Interplay between heating and rotation in core collapse supernovae
16:50 Discussion
Friday 16
09:30 Koh Takahashi Towards a consistent modeling of magneto-rotating stellar evolution
10:30 Naveen Yadav Pre-explosion dynamics of a supernova progenitor based on 3D modelling
11:00 Coffee break
11:30 Shuai Zha Multi-messenger Signals of Dark Matter Admixed Accretion-Induced Collapse of White Dwarfs
12:00 Niccolò Tomei Mean-field dynamo in relativistic disks accreting onto rotating black holes
13:00 Lunch break
14:30 Discussion
15:30 Coffee break