Recent progress of laboratory astrophysics with intense lasers
Thanks to a rapid progress of high-power lasers since the birth of laser by TH Maiman in
1960, intense lasers have been developed mainly for studying the scientific feasibility of …
1960, intense lasers have been developed mainly for studying the scientific feasibility of …
Proton imaging of high-energy-density laboratory plasmas
Proton imaging has become a key diagnostic for measuring electromagnetic fields in high-
energy-density (HED) laboratory plasmas. Compared to other techniques for diagnosing …
energy-density (HED) laboratory plasmas. Compared to other techniques for diagnosing …
Dynamo theories
F Rincon - Journal of Plasma Physics, 2019 - cambridge.org
These lecture notes are based on a tutorial given in 2017 at a plasma physics winter school
in Les Houches. Their aim is to provide a self-contained graduate-student level introduction …
in Les Houches. Their aim is to provide a self-contained graduate-student level introduction …
Building high accuracy emulators for scientific simulations with deep neural architecture search
Computer simulations are invaluable tools for scientific discovery. However, accurate
simulations are often slow to execute, which limits their applicability to extensive parameter …
simulations are often slow to execute, which limits their applicability to extensive parameter …
MHD turbulence: a biased review
AA Schekochihin - Journal of Plasma Physics, 2022 - cambridge.org
This review of scaling theories of magnetohydrodynamic (MHD) turbulence aims to put the
developments of the last few years in the context of the canonical time line (from Kolmogorov …
developments of the last few years in the context of the canonical time line (from Kolmogorov …
Magnetic fields in the formation of the first stars–I. Theory versus simulation
CF McKee, A Stacy, PS Li - Monthly Notices of the Royal …, 2020 - academic.oup.com
While magnetic fields are important in contemporary star formation, their role in primordial
star formation is unknown. Magnetic fields of the order of 10− 16 G are produced by the …
star formation is unknown. Magnetic fields of the order of 10− 16 G are produced by the …
Symmetric set of transport coefficients for collisional magnetized plasma
Braginskii extended magnetohydrodynamics is used to model transport in collisional
astrophysical and high energy density plasmas. We show that commonly used …
astrophysical and high energy density plasmas. We show that commonly used …
Saturation mechanism of the fluctuation dynamo in supersonic turbulent plasmas
Magnetic fields in several astrophysical objects are amplified and maintained by a dynamo
mechanism, which is the conversion of the turbulent kinetic energy to magnetic energy. A …
mechanism, which is the conversion of the turbulent kinetic energy to magnetic energy. A …
The data-driven future of high-energy-density physics
High-energy-density physics is the field of physics concerned with studying matter at
extremely high temperatures and densities. Such conditions produce highly nonlinear …
extremely high temperatures and densities. Such conditions produce highly nonlinear …
Micron-scale phenomena observed in a turbulent laser-produced plasma
Turbulence is ubiquitous in the universe and in fluid dynamics. It influences a wide range of
high energy density systems, from inertial confinement fusion to astrophysical-object …
high energy density systems, from inertial confinement fusion to astrophysical-object …