4th CRISM conference

Cosmic Rays and the InterStellar Medium

25 - 29 June 2018
Grenoble (France)

Agenda

Monday, June 25, 2018

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!  

Tuesday, June 26, 2018

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).  

Wednesday, June 27, 2018

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 !
 

Thursday, June 28, 2018

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  

Friday, June 29, 2018

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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