CRISM2014
24-27 June 2014
Montpellier, France
published June 10, 2015
Montpellier, France
published June 10, 2015
Cosmic rays are a major component of the interstellar medium. They share an equivalent energy density with the magnetic field and the interstellar gas. At low energies cosmic rays possibly take an active part in the dynamics of the structures of the interstellar medium. They contribute to its ionisation. They produce a force through their pressure gradient over the magnetised fluid. They generate plasma waves and magnetic turbulence. This turbulence has in turn an important role in the evolution of molecular gas and in the star formation cycle. At high energies cosmic rays are identified by their interaction with the molecular gas and produce neutral and charged pions and secondary particles (gamma rays, electron-positron and neutrinos). Cosmic rays are also responsible for the spallation nucleosynthesis of light and stable and radioactive elements. They are likely associated with the remnants of supernovae. A large fraction of these supernovae explode as a result of the collapse of the core of massive stars. Massive stars, their evolution and the way they shape their environment appear also to have a central role in the cosmic ray production. Cosmic rays turn out to be a key ingredient in the local and global dynamics of the interstellar medium. But this is only very recently since this component started to be integrated in the modeling of the interstellar medium evolution. The main objective of this international workshop is to contribute to a better account of the multiple effects of the energetic component of the interstellar medium.
| Session The cosmic ray spectrum |
|---|
|
Direct detection of cosmic rays: Recent observational progresses
|
|
A database of charged cosmic rays (CRDB) and constraints on the interstellar flux
|
|
The highest galactic cosmic ray energies
|
|
Proton analysis with AMS-02 and solar modulation level
|
| Cosmic Ray sources:Theory |
|
Origin of Cosmic Rays
|
|
High energy emission from massive star clusters
|
|
Hydrodynamics of Young Supernova Remnants and the Implications for their Gamma-ray emission
|
|
The impact of magnetic turbulence spectrum on particle acceleration in SNR IC443
|
|
Cosmic Rays in star forming galaxies
|
|
3D simulations of the emission from young supernova remnants including particle acceleration
|
| Session multi-wavelength |
|
An observational view of particle acceleration in cosmic ray sources
|
|
Hadronic TeV emission of the supernova remnant W51C observed with the MAGIC Telescopes?
|
|
Particle acceleration in the stellar graveyard and the case of young SNRs
|
|
A Catalogue of High-Energy Observations of Galactic Supernova Remnants
|
|
SNR and molecular cloud associations as seen by H.E.S.S
|
|
Gamma Rays from supernova remnants
|
|
TeV sources in the Cygnus region observed with VERITAS
|
|
The cosmic-ray, dust, and gas content of the local Chamaeleon clouds + reports on Voyager results
|
|
Gas towards the gamma-ray sources HESS J1731-347 and HESS J1729-345
|
| Plasma instabilities and cosmic rays |
|
Cosmic Ray driven instabilities
|
|
Propagation of cosmic rays into diffuse clouds
|
|
Cosmic ray driven winds
|
|
Relativistic cosmic-ray back-reaction instabilities along the background magnetic field
|
|
Magnetic field structure from cosmic ray driven dynamo in spiral galaxies
|
| Low energy cosmic rays |
|
Cosmic-Ray Ionization of Molecular Clouds
|
|
Wind-driven Exclusion of Cosmic Rays in the Protoplanetary Disk Environment
|
|
Cosmic-ray induced ionization of a molecular cloud shocked by the W28 supernova remnant
|
|
The role of cosmic rays on magnetic field diffusion and the formation of protostellar discs
|
|
Cosmic Ray Transport in the Astrospheres of Solar Twins
|
|
Cosmic-ray heating of molecular cloud cores
|
|
Localized SiO emission triggered by the passage of the W51C supernova remnant shock
|
| The turbulent interstellar medium |
|
nd
|
|
Recent results from Herschel
|
|
Wide-Field Polarimetry: A Unique Probe of Interstellar Turbulence
|
|
Synchrotron emission from molecular clouds
|
|
X-shape magnetic fields in galactic halos
|
|
APEX observations of non-stationary magneto-hydrodynamical shocks in W44
|
|
Irradiated shocks in the W28 A2 star-forming region: sites of cosmic-ray acceleration ?
|
| The galactic center |
|
Non-Thermal Radiation from the Inner Galaxy
|
|
Low-Energy Cosmic Rays in the Galactic Center Region
|
|
Can Cosmic Rays Interacting With Molecular Clouds Explain the Galactic Center Gamma-Ray Excess?
|
| Cosmic Ray propagation |
|
Cosmic Ray propagation close to their acceleration site
|
|
Propagation of high-energy cosmic-ray electrons in the interstellar medium
|
|
Picard: A new Code for The Galactic Cosmic Ray Propagation Problem
|
|
A solution to the cosmic ray anisotropy problem
|
|
Charged-particle heating in imbalanced MHD turbulence
|
|
Cosmic-ray diffusion in magnetized turbulence
|
|
Cosmic Ray propagation in local magnetic fields
|
