Agenda
| Time |
Event |
|
|
12:00 - 12:50
|
Registration desk - welcome and informations |
|
|
12:50 - 13:00
|
Wlecome and forewords - CRISM organizer |
|
|
13:00 - 15:10
|
Local ISM, MeV CRs and Voyager data - Marijke Haverkorn |
|
| 13:00 - 13:40 |
› Observations of Galactic Cosmic Rays in the Very Local Interstellar Medium from Voyager 1 - A. C. Cummings, California Institute of Technology |
|
| 13:40 - 13:20 |
› The influence of cosmic rays on the local ISM as revealed by interstellar chemistry - Nicholas Indriolo, Space Telescope Science Institute |
|
| 14:20 - 14:45 |
› The interstellar magnetic field in the shell of the Local Bubble - Katia Ferrière, Institut de recherche en astrophysique et planétologie |
|
| 14:45 - 15:10 |
› TeV-PeV Cosmic-Ray Anisotropy as a Probe of the Local Interstellar Turbulence - Gwenael Giacinti, Max Planck Institute for Nuclear Physics |
|
|
15:10 - 15:40
|
Coffee break |
|
|
15:40 - 18:00
|
Sources of GCRs and acceleration mechanisms: supernova remnants, pulsar winds, stellar clusters, young stellar objects, multi-wavelength observations - Pasquale Blasi |
|
| 15:40 - 16:20 |
› Interstellar medium studies in direction to gamma-ray sources - Gloria Dubner, Instituto de Astronomia y Fisica del Espacio |
|
| 16:20 - 16:45 |
› Cosmic ray streaming instability in the ISM: analytic predictions vs numerical simulations - Illya Plotnikov, Department of Astrophysical Sciences [Princeton] |
|
| 16:45 - 17:10 |
› Hybrid modeling of CR dynamics in collisionless shocks in multispecies plasma - Julia Kropotina, A.F. Ioffe Physico-Technical Institute |
|
| 17:10 - 17:35 |
› The Galactic population of supernova remnant pevatrons - Pierre Cristofari, Columbia University |
|
|
18:30 - 19:30
|
Cocktail at City Hall - We will go directly by tram after the last talk of the day! |
|
| Time |
Event |
|
|
09:00 - 10:30
|
Sources of GCRs and acceleration mechanisms: supernova remnants, pulsar winds, stellar clusters, young stellar objects, multi-wavelength observations - Olaf Reimer |
|
| 09:00 - 09:40 |
› The non-thermal Life of Supernova Remnants - Damiano Caprioli, University of Chicago |
|
| 09:40 - 10:05 |
› Investigating the high-frequency spectral features of SNRs W44 and IC443 with the Sardinia Radio Telescope. - Sara Loru, INAF - Osservatorio Astronomico di Cagliari |
|
| 10:05 - 10:30 |
› Modeling of the spatially resolved non-thermal emission from the Vela Jr. supernova remnant - Iurii Sushch, Deutsches Elektronen-Synchrotron [Zeuthen] |
|
|
10:30 - 11:00
|
Coffee break |
|
|
11:00 - 12:15
|
Sources of GCRs and acceleration mechanisms: supernova remnants, pulsar winds, stellar clusters, young stellar objects, multi-wavelength observations - Elizabeth Hays |
|
| 11:00 - 11:25 |
› Shock-Cloud Interaction in the Young Supernova Remnants - Hidetoshi Sano, Nagoya University |
|
| 11:25 - 11:50 |
› Cosmic rays from young star clusters: clues from multi-wavelength observations - Siddhartha Gupta, Indian Institute of Science, Raman Research Institute |
|
| 11:50 - 12:15 |
› The naked Orion: a mysterious gamma-ray emission maybe due to Cosmic Ray acceleration - Martina Cardillo, Istituto di Astrofisica e Planetologia Spaziali |
|
|
12:15 - 14:15
|
Lunch |
|
|
14:15 - 15:45
|
Sources of GCRs and acceleration mechanisms: supernova remnants, pulsar winds, stellar clusters, young stellar objects, multi-wavelength observations - Nicholas Indriolo |
|
| 14:15 - 14:55 |
› Protostars as cosmic-ray factories - Marco Padovani, INAF - Osservatorio Astrofisico di Arcetri |
|
| 14:55 - 15:20 |
› Non-linear diffusion of cosmic rays escaping from supernova remnants - Sarah Recchia, AstroParticule et Cosmologie |
|
| 15:20 - 15:45 |
› Voyager probing dark matter - Mathieu Boudaud, Laboratoire de Physique Théorique et Hautes Energies |
|
|
15:45 - 16:15
|
Coffee break |
|
|
16:15 - 18:00
|
GCR data and future studies - David Maurin |
|
| 16:15 - 16:55 |
› Future Prospects for Indirect Searches for Cosmic Rays - Elizabeth Hays, NASA - Goddard Space Flight Center |
|
| 16:55 - 17:35 |
› Experimental results on direct cosmic-ray measurements - Laurent Derome, LPSC |
|
| 17:35 - 18:00 |
› The low energy extension of the Pierre Auger Observatory measurements - Vladimir Novotny, Institute of Particle and Nuclear Physics, Faculty of Mathematics and Physics, Charles University |
|
|
19:30 - 21:00
|
Wine testing at "Cave du forté" - Taste and enjoy a few different wines from regional ad French productions at Cave du Forté (4 Place Lavalette, Grenoble)! Finger food provided (cheese, delicatessen, tapas). |
|
| Time |
Event |
|
|
09:00 - 10:30
|
CR transport in the ISM: role of self-generated turbulence, large-scale injected turbulence, direct and indirect observations, modelling and phenomenology, link to dark matter detection - TBD |
|
| 09:00 - 09:40 |
› Phenomenology of CR transport in the Galaxy - Philipp Mertsch, RWTH Aachen University |
|
| 09:40 - 10:05 |
› Recent results with the USINE propagation code - David Maurin, LPSC |
|
| 10:05 - 10:30 |
› Deuteron and Antideuteron Production Simulation in Cosmic-ray Interactions - Diego Gomez, Institute of Physics, UNAM |
|
|
10:30 - 11:00
|
Coffee break |
|
|
11:00 - 11:25
|
CR transport in the ISM: role of self-generated turbulence, large-scale injected turbulence, direct and indirect observations, modelling and phenomenology, link to dark matter detection - Sarah Recchia |
|
| 11:00 - 11:25 |
› Three-dimensional Models of the Interstellar Medium for the Propagation of Cosmic Rays and their Non-Thermal Interstellar Emissions - Troy Porter, Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology |
|
|
11:25 - 12:30
|
Poster session |
|
| 11:25 - 11:28 |
› Implementation of a sub-grid cosmic rays diffusion coefficient and resonnant Alfven waves drift velocity term in the RAMSES code - Loann Brahimi, Laboratoire Univers et particules de Montpellier |
|
| 11:28 - 11:31 |
› Piernik MHD code extension: modelling energy dependent transport of cosmic ray electrons with energy spectrum evolution. - Mateusz Ogrodnik, Nicolaus Copernicus University [Toruń] |
|
| 11:31 - 11:34 |
› Synchrotron signatures from the cosmic-ray driven dynamo - Dominik Wóltański, Toruń Centre for Astronomy |
|
| 11:34 - 11:37 |
› CPIPES - A software for the non-equilibrium ionisation evolution of the supernova and cosmic-rays driven ISM - Miguel de Avillez, Technische Universität Berlin, University of Évora [Portugal] |
|
| 11:37 - 11:40 |
› Variability of the adiabatic parameter in (non-)thermal plasmas - Miguel de Avillez, Technische Universität Berlin, University of Évora [Portugal] |
|
| 11:40 - 11:43 |
› Cosmic rays and superbubbles - Joubaud Théo, AIM |
|
| 11:43 - 11:46 |
› Cosmic Ray Propagation in Super Bubbles - Tolksdorf Tobias, Ruhr-Universität Bochum |
|
| 11:46 - 11:49 |
› Propagation of Galactic Cosmic Rays: the influence of anisotropic diffusion - Ala'a Al-Zetoun, Radboud University Nijmegen |
|
|
12:30 - 14:00
|
Lunch and free afternoon (visit Grenoble, take the cable car to La Bastille, have fun!) |
|
|
14:00 - 15:30
|
Group visit of Grenoble museum - Guided tour (in English) of the museum for those who signed up (it is confirmed, we have more than 10 participants!). More information on the museum at http://www.museedegrenoble.fr/962-english.htm |
|
|
18:30 - 19:30
|
Public outreach conference (in french) - Richard Taillet, professeur en physique à l'université de Savoie, proposera une conférence distrayante sur un sujet qui mêle la physique et la science-fiction. Les scénaristes des films de science-fiction sont souvent amenés à décrire des situations assez éloignées de la vie de tous les jours, et doivent pour cela faire appel à des notions de physique. Le résultat est plus ou moins réussi selon les films, on trouve des erreurs grossières, voire ridicules, ainsi que des scènes très justes et réalistes. Cette conférence abordera le traitement de l'apesanteur dans différents films, en s'appuyant sur de nombreux extraits (2001, Sunshine, Mission to Mars, Inception, Gravity, Interstellar, etc...) ainsi que sur quelques documents d'archives liés à la conquête spatiale.
La conférence est destinée à tous les publics, étudiants ou non, physiciens ou non, le but étant autant de proposer une pause détente que de parler de science et de cinéma !
|
|
| Time |
Event |
|
|
09:00 - 10:20
|
CR transport in the ISM: role of self-generated turbulence, large-scale injected turbulence, direct and indirect observations, modelling and phenomenology, link to dark matter detection - Katia Ferrière |
|
| 09:00 - 09:40 |
› Cosmic rays in intermittent random magnetic fields - Anvar Shukurov, Newcastle University |
|
| 09:40 - 10:20 |
› Properties of the turbulent, magnetized interstellar medium - Marijke Haverkorn, Radboud University |
|
|
10:20 - 10:50
|
Coffee break |
|
|
10:50 - 12:30
|
CR transport in the ISM: role of self-generated turbulence, large-scale injected turbulence, direct and indirect observations, modelling and phenomenology, link to dark matter detection - Christoph Pfrommer |
|
| 10:50 - 11:15 |
› Penetration of Cosmic Rays into Dense Molecular Clouds: Role of Diffuse Envelopes - Alexei Ivlev, Max-Planck-Institute für extraterrestrische Physik |
|
| 11:15 - 11:40 |
› Synchrotron emission from the cosmic ray driven galactic winds. - Michal Hanasz, Nicolaus Copernicus University [Toruń] |
|
| 11:40 - 12:05 |
› A 3D view of our Galaxy : gas and Cosmic rays - Quentin REMY, LUPM |
|
| 12:05 - 12:30 |
› Constraining the halo size from possible density profiles of hydrogen gas of Milky Way Galaxy - Sayan Biswas, Post Doctoral Fellow |
|
|
12:30 - 14:30
|
Lunch |
|
|
14:30 - 15:45
|
CR transport in the ISM: role of self-generated turbulence, large-scale injected turbulence, direct and indirect observations, modelling and phenomenology, link to dark matter detection - Alexandre Marcowith |
|
| 14:30 - 14:55 |
› New implications of self-generated turbulence on the cosmic ray propagation in the ISM - Carmelo Evoli, Gran Sasso Science Institute |
|
| 14:55 - 15:20 |
› The Propagation of Cosmic Rays from the Galactic Wind Termination Shock: Back to the Galaxy? - Lukas Merten, Ruhr-Universität Bochum |
|
| 15:20 - 15:45 |
› X-ray Polarization Probes of Turbulence and Cosmic Ray Diffusion in Supernova Remnants - Matthew Baring, Rice University |
|
|
15:45 - 16:15
|
Coffee break |
|
|
16:15 - 17:45
|
Sources of GCRs and acceleration mechanisms: supernova remnants, pulsar winds, stellar clusters, young stellar objects, multi-wavelength observations - Maïka Clavel |
|
| 16:15 - 16:55 |
› The Galactic High-Energy Sky - Olaf Reimer, Institute for Astro- and Particle Physics - Innsbruck University |
|
| 16:55 - 17:20 |
› Implications of the FIR-radio correlation for CR acceleration - Mark Walker, Manly Astrophysics |
|
| 17:20 - 17:45 |
› Cosmic rays in the superwinds of starburst galaxies - Ana Laura Müller, Instituto Argentino de Radioastronomía, Institut für Kernphysik, Karlsruhe Institut of Technology, Instituto de Tecnologı́as en Detección y Astropartı́culas |
|
|
20:00 - 22:30
|
Conference dinner - Conference dinner |
|
| Time |
Event |
|
|
09:00 - 10:05
|
Impact of GCRs: dynamics of the ISM, physics and chemistry of molecular clouds, role in the formation of stars and planets, composition of cosmomaterials - Philipp Mertsch |
|
| 09:00 - 09:40 |
› How cosmic rays shape galaxies - Christoph Pfrommer, Leibniz-Institut für Astrophysik Potsdam |
|
| 09:40 - 10:05 |
› Cooler and smoother – the impact of cosmic rays on the phase structure of galactic outflows - Philipp Girichidis, Leibniz-Institut fuer Astrophysik, Potsdam |
|
|
10:05 - 10:35
|
Coffee break |
|
|
10:35 - 12:15
|
CR transport in the ISM: role of self-generated turbulence, large-scale injected turbulence, direct and indirect observations, modelling and phenomenology, link to dark matter detection - Gloria Dubner |
|
| 10:35 - 11:00 |
› Numerical modelling of the time-dependent ionisation structure and emission due to non-thermal plasmas in the supernova-driven ISM - Miguel de Avillez, Technische Universität Berlin, University of Évora [Portugal] |
|
| 11:00 - 11:25 |
› Galactic Magnetic field from polarized emission at CMB frequencies - Vincent Pelgrims, Laboratoire de Physique Subatomique et Cosmologie |
|
| 11:25 - 11:50 |
› Cosmic Ray Tomography using Low Radio Frequency Observations - Irene Polderman, Radboud University Nijmegen |
|
| 11:50 - 12:15 |
› The warm ionised medium: hotter and denser than you thought - Marisa Geyer, Oxford University/SKA SA |
|
|
12:15 - 14:00
|
Lunch |
|
|
14:00 - 14:50
|
Impact of GCRs: dynamics of the ISM, physics and chemistry of molecular clouds, role in the formation of stars and planets, composition of cosmomaterials - Pierre Hily-Blant |
|
| 14:00 - 14:25 |
› What is the contribution of LECRs to the bright X-ray emission of the molecular clouds at the Galactic center? - Maïca Clavel, Institut de Planétologie et d'Astrophysique de Grenoble |
|
| 14:25 - 14:50 |
› From high-energy to low-energy cosmic rays: mind the gap! - Thierry Montmerle, Institut d'Astrophysique de Paris, IAP |
|
|
14:50 - 15:15
|
Summary talk - P. Blasi |
|
|
15:30 - 15:35
|
Last words: next CRISM? - CRISM organizers |
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