0000000000614699

AUTHOR

V. Lelasseux

showing 3 related works from this author

Detailed characterization of laboratory magnetized super-critical collisionless shock and of the associated proton energization

2021

Collisionless shocks are ubiquitous in the Universe and are held responsible for the production of nonthermal particles and high-energy radiation. In the absence of particle collisions in the system, theory shows that the interaction of an expanding plasma with a pre-existing electromagnetic structure (as in our case) is able to induce energy dissipation and allow shock formation. Shock formation can alternatively take place when two plasmas interact, through microscopic instabilities inducing electromagnetic fields that are able in turn to mediate energy dissipation and shock formation. Using our platform in which we couple a rapidly expanding plasma induced by high-power lasers (JLF/Titan…

Nuclear and High Energy PhysicsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesmagnetic fieldQC770-798shock waves01 natural sciencesAtomic and Molecular Physics and OpticsPhysics - Plasma Physics010305 fluids & plasmasPlasma Physics (physics.plasm-ph)Settore FIS/05 - Astronomia E AstrofisicaNuclear Energy and Engineering[PHYS.PHYS.PHYS-PLASM-PH]Physics [physics]/Physics [physics]/Plasma Physics [physics.plasm-ph]Nuclear and particle physics. Atomic energy. Radioactivity0103 physical sciencesPhysics::Space PhysicsElectrical and Electronic Engineering010306 general physics
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Laboratory evidence for proton energization by collisionless shock surfing

2021

Charged particles can be accelerated to high energies by collisionless shock waves in astrophysical environments, such as supernova remnants. By interacting with the magnetized ambient medium, these shocks can transfer energy to particles. Despite increasing efforts in the characterization of these shocks from satellite measurements at Earth’s bow shock as well as powerful numerical simulations, the underlying acceleration mechanism or a combination thereof is still widely debated. Here we show that astrophysically relevant super-critical quasi-perpendicular magnetized collisionless shocks can be produced and characterized in the laboratory. We observe the characteristics of super-criticali…

Shock waveProtonAstrophysics::High Energy Astrophysical PhenomenaGeneral Physics and AstronomyFOS: Physical sciences01 natural sciencesAccelerationSettore FIS/05 - Astronomia E Astrofisica0103 physical sciencesBow shock (aerodynamics)010306 general physics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsMechanicsplasmasPhysics - Plasma PhysicsCharged particleComputer Science::Computers and Society[PHYS.PHYS.PHYS-GEN-PH]Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]Magnetic fieldShock (mechanics)Plasma Physics (physics.plasm-ph)Supernova13. Climate actionPhysics::Space PhysicsPhysics::Accelerator Physics
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Particle energization in colliding subcritical collisionless shocks investigated in the laboratory

2022

Context. Colliding collisionless shocks appear across a broad variety of astrophysical phenomena and are thought to be possible sources of particle acceleration in the Universe. Aims. The main goal of our experimental and computational work is to understand the effect of the interpenetration between two subcritical collisionless shocks on particle energization. Methods. To investigate the detailed dynamics of this phenomenon, we performed a dedicated laboratory experiment. We generated two counter-streaming subcritical collisionless magnetized shocks by irradiating two Teflon (C2F4) targets with 100 J, 1 ns laser beams on the LULI2000 laser facility. The interaction region between the plasm…

Plasma Physics (physics.plasm-ph)Settore FIS/05 - Astronomia E Astrofisica[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph][SDU]Sciences of the Universe [physics]Space and Planetary ScienceAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and Astrophysicsshock wavesinterplanetary mediumPhysics - Plasma Physicsacceleration of particles
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