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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 …
[HTML][HTML] National Diagnostic Working Group (NDWG) for inertial confinement fusion (ICF)/high-energy density (HED) science: The whole exceeds the sum of its parts
JD Kilkenny, WW Hsing, SH Batha… - Review of Scientific …, 2023 - pubs.aip.org
The National Diagnostic Working Group (NDWG) has led the effort to fully exploit the major
inertial confinement fusion/high-energy density facilities in the US with the best available …
inertial confinement fusion/high-energy density facilities in the US with the best available …
The high energy density scientific instrument at the European XFEL
U Zastrau, K Appel, C Baehtz, O Baehr… - Synchrotron …, 2021 - journals.iucr.org
The European XFEL delivers up to 27000 intense (> 1012 photons) pulses per second, of
ultrashort (≤ 50 fs) and transversely coherent X-ray radiation, at a maximum repetition rate …
ultrashort (≤ 50 fs) and transversely coherent X-ray radiation, at a maximum repetition rate …
Turbulent magnetic reconnection generated by intense lasers
Y **, J Zhong, X Wang, B Han, W Sun, Y Zhang… - Nature Physics, 2023 - nature.com
Turbulent magnetic reconnection is believed to occur in astrophysical plasmas, and it has
been suggested to be a trigger of solar flares. It often occurs in long stretched and …
been suggested to be a trigger of solar flares. It often occurs in long stretched and …
Electron–ion temperature ratio in astrophysical shocks
JC Raymond, P Ghavamian, A Bohdan… - The Astrophysical …, 2023 - iopscience.iop.org
Collisionless shock waves in supernova remnants and the solar wind heat electrons less
effectively than they heat ions, as is predicted by kinetic simulations. However, the values of …
effectively than they heat ions, as is predicted by kinetic simulations. However, the values of …
Data-driven discovery of reduced plasma physics models from fully kinetic simulations
At the core of some of the most important problems in plasma physics—from controlled
nuclear fusion to the acceleration of cosmic rays—is the challenge to describe nonlinear …
nuclear fusion to the acceleration of cosmic rays—is the challenge to describe nonlinear …
Electron polarization in ultrarelativistic plasma current filamentation instabilities
Plasma current filamentation of an ultrarelativistic electron beam im**ing on an overdense
plasma is investigated, with emphasis on radiation-induced electron polarization. Particle-in …
plasma is investigated, with emphasis on radiation-induced electron polarization. Particle-in …
Downstream high-speed plasma jet generation as a direct consequence of shock reformation
Shocks are one of nature's most powerful particle accelerators and have been connected to
relativistic electron acceleration and cosmic rays. Upstream shock observations include …
relativistic electron acceleration and cosmic rays. Upstream shock observations include …
Magnetic field amplification by the Weibel instability at planetary and astrophysical shocks with high Mach number
Collisionless shocks are ubiquitous in the Universe and often associated with a strong
magnetic field. Here, we use large-scale particle-in-cell simulations of nonrelativistic …
magnetic field. Here, we use large-scale particle-in-cell simulations of nonrelativistic …
Theory of electron injection at oblique shock of finite thickness
A theory of electron injection into diffusive shock acceleration (DSA) for the generation of
cosmic-ray electrons at collisionless shocks is presented. We consider a recently proposed …
cosmic-ray electrons at collisionless shocks is presented. We consider a recently proposed …