The head-on collision between electrostatic shocks is studied via multi-dimensional Particle-In-Cell simulations. A strong magnetic field develops after the interaction, which causes the shock velocities to drop significantly. This transverse magnetic field is generated by the Weibel instability, which is driven by pressure anisotropies due to longitudinal electron heating while the shocks approach each other. The possibility to explore the physics underpinning the shock collision in the laboratory with current laser facilities is discussed
International audienceContemporary lasers allow us to create shocks in the laboratory that propagate...
A collisionless Weibel-instability mediated shock in a self-generated magnetic field is studied usin...
A collisionless Weibel-instability mediated shock in a self-generated magnetic field is studied usin...
The work presented in this thesis belongs to the general framework of Laboratory Astrophysics. We ad...
This thesis presents experimental, computational, and theoretical work studying shock formation and ...
This thesis presents experimental, computational, and theoretical work studying shock formation and ...
We examine with a particle-in-cell (PIC) simulation the collision of two equally dense clouds of col...
We examine with a particle-in-cell (PIC) simulation the collision of two equally dense clouds of col...
WOS:000341271100005 (Nº de Acesso Web of Science)A new magnetic field generation mechanism in electr...
Many astrophysical systems are effectively “collisionless,” that is, the mean free path for collisio...
Many astrophysical systems are effectively “collisionless,” that is, the mean free path for collisio...
Many astrophysical systems are effectively “collisionless,” that is, the mean free path for collisio...
Plasma outflow from Gamma Ray Bursts, Supernovas and from relativistic jets in general, interacts wi...
International audienceContemporary lasers allow us to create shocks in the laboratory that propagate...
International audienceContemporary lasers allow us to create shocks in the laboratory that propagate...
International audienceContemporary lasers allow us to create shocks in the laboratory that propagate...
A collisionless Weibel-instability mediated shock in a self-generated magnetic field is studied usin...
A collisionless Weibel-instability mediated shock in a self-generated magnetic field is studied usin...
The work presented in this thesis belongs to the general framework of Laboratory Astrophysics. We ad...
This thesis presents experimental, computational, and theoretical work studying shock formation and ...
This thesis presents experimental, computational, and theoretical work studying shock formation and ...
We examine with a particle-in-cell (PIC) simulation the collision of two equally dense clouds of col...
We examine with a particle-in-cell (PIC) simulation the collision of two equally dense clouds of col...
WOS:000341271100005 (Nº de Acesso Web of Science)A new magnetic field generation mechanism in electr...
Many astrophysical systems are effectively “collisionless,” that is, the mean free path for collisio...
Many astrophysical systems are effectively “collisionless,” that is, the mean free path for collisio...
Many astrophysical systems are effectively “collisionless,” that is, the mean free path for collisio...
Plasma outflow from Gamma Ray Bursts, Supernovas and from relativistic jets in general, interacts wi...
International audienceContemporary lasers allow us to create shocks in the laboratory that propagate...
International audienceContemporary lasers allow us to create shocks in the laboratory that propagate...
International audienceContemporary lasers allow us to create shocks in the laboratory that propagate...
A collisionless Weibel-instability mediated shock in a self-generated magnetic field is studied usin...
A collisionless Weibel-instability mediated shock in a self-generated magnetic field is studied usin...