Simulating the evolution and emission of relativistic outflows
Salle de Conférence du Château
Relativistic jets and outflows are astrophysical phenomena that occur at very different spatial scales in various sources linked to high-energy emission, such as AGN, GRBs, X-ray binaries and micro-quasars, as well as pulsars.
The goal of this workshop is to get together experts on the physics of relativistic jets in Galactic and extragalactic objects in France and their associates, to compare our approaches and to reinforce exchanges between the different groups. The workshop will include a few presentations on the currently available observational data and will be primarily focusing on numerical modelling of the evolution of jets and their emission.
This workshop is partly financed by the Centre International d'Ateliers Scientifiques (CIAS) at the Observatoire de Paris. Relativistic jets represent of course a central research topic for the future Cherenkov Telescope Array (CTA) and the workshop has also received partial funding by the Action Fédératrice CTA at the Observatoire de Paris.
-
-
09:00
→
09:30
Welcome and Coffee
-
09:00
Welcome and Coffee 25m
-
09:25
Introduction 5mOrateur: Andreas Zech
-
09:00
-
09:30
→
11:00
Particle acceleration in relativistic jets
-
09:30
Generalised Fermi acceleration 30mOrateur: Martin Lemoine (Institut d'Astrophysique de Paris, CNRS - Sorbonne U)
-
10:00
PIC / MHD simulations of relativistic shocks 30mOrateur: Fabien Casse (APC - Université de Paris)
- 10:30
-
09:30
-
11:00
→
11:30
Coffee break 30m
-
11:30
→
11:50
Particle acceleration in relativistic jets
-
11:30
Electromagnetic cascades in Kerr black hole magnetospheres 20mOrateur: Benjamin Crinquand (IPAG)
-
11:30
-
11:50
→
12:50
AGN - Observations
- 11:50
-
12:20
Observations of jets with geodetic VLBI and link to Gaia 30m
Geodetic VLBI is a powerful technique that has been used for 40 years to monitor the Earth’s rotation and realize the terrestrial and celestial reference frames with an unprecedented precision (< 0.1 mas). Recently, it has permitted the construction of the third realization of the International Celestial Reference Frame (ICRF3) which is currently the most precise celestial reference frame. Recently also, Gaia provided an independent astrometric solution whose precision is, for the first time, comparable to VLBI, opening the way to comparisons of positions at various wavelengths. In this talk, I will show the signature of relativistic jets - and more generally of the source structure - in geodetic VLBI observations, and the systematics and offsets between VLBI and Gaia positions.
Orateur: Sébastien Lambert (SYRTE, Observatoire de Paris)
-
12:50
→
14:00
Lunch break 1h 10m Hall Uranie
Hall Uranie
-
14:00
→
15:25
AGN - Jet models
-
14:00
Jet modelling in AGN and preparation of simulations. 35mOrateur: Christophe Sauty
-
14:35
GRMHD modelling and radiative transfer 20mOrateur: Gaëtan Fichet de Clairfontaine (LUTH Observatoire de Paris)
-
14:55
A jet model for describing the shadows of Sgr A* and M87* 30mOrateur: Frédéric Vincent
-
14:00
-
15:25
→
15:55
AGN - Emission models
-
15:25
Emission modelling with stratified jets 30mOrateur: Gilles Henri (IPAG/Observatoire de Grenoble/UGA)
-
15:25
-
15:55
→
16:25
Coffee break 30m
-
16:25
→
17:15
AGN - Emission models
-
16:25
Time-dependent modeling of the blazar flares 20mOrateur: Anton Dmytriiev (LUTH Observatoire de Paris)
-
16:45
Linking high-energy emission with radio-VLBI jets 30mOrateur: Olivier Hervet (UCSC)
-
16:25
-
09:00
→
09:30
-
-
09:00
→
09:30
Welcome and Coffee
-
09:30
→
10:00
AGN - Emission models
-
09:30
Hadronic emission modelling and multi-messengers 30mOrateur: Dr Matteo Cerruti (Institut de Ciències del Cosmos - Universitat de Barcelona (ICCUB))
-
09:30
- 10:00 → 10:30
-
10:30
→
11:00
GRB - Emission models
-
10:30
Internal shock scenario for GRBs 30mOrateur: Frédéric Daigne (Institut d'Astrophysique de Paris - Sorbonne Université)
-
10:30
-
11:00
→
11:30
Coffee break 30m
-
11:30
→
12:20
GRB - Emission models
-
11:30
Emission modelling at very high energies 30mOrateur: Zeljka Bosnjak (FER - University of Zagreb, Croatia)
-
12:00
Relativistic ejections from binary neutron star mergers. 20mOrateur: Raphaël Duque (Institut d'Astrophysique de Paris)
-
11:30
-
12:20
→
12:50
X-ray/gamma-ray binaries - Observations
- 12:20
-
12:50
→
14:00
Lunch break 1h 10m Hall Uranie
Hall Uranie
-
14:00
→
15:20
X-ray/gamma-ray binaries - jet and emission models
-
14:00
The iInternal shock model applied to X-ray binaries. 30mOrateur: Julien Malzac (IRAP (CNRS/Université de Toulouse/CNES))
-
14:30
An Accretion-Ejection Paradigm for Compact Objects 30mOrateur: Pierre-Olivier Petrucci (IPAG)
-
15:00
Dynamical effects of radiative losses in high-mass microquasars 20mOrateur: Arthur Charlet (CRAL, LUPM)
-
14:00
-
15:20
→
15:50
Coffee break 30m
-
15:50
→
16:30
Conclusions
-
09:00
→
09:30