Author Affiliations
Abstract
1 Joint Institute for High Temperatures of Russian Academy of Sciences, 13/2 Izhorskaya St., 125412 Moscow, Russia
2 Institute for Open and Transdisciplinary Research Initiative, Osaka University, Suita, Osaka 565-0871, Japan
3 Graduate School of Engineering, Osaka University, Suita, Osaka 565-0817, Japan
4 Institute of Laser Engineering, Osaka University, Suita, Osaka 565-0871, Japan
5 Landau Institute for Theoretical Physics of Russian Academy of Sciences, 1-A Akademika Semenova Ave., Chernogolovka, Moscow Region 142432, Russia
6 LULI, CNRS, CEA, École Polytechnique, UPMC, Université Paris 06: Sorbonne Universités, Institut Polytechnique de Paris, F-91128 Palaiseau Cedex, France
7 Graduate School of Science, Nagoya University, Chikusa Ku, Nagoya, Aichi 4648602, Japan
8 Department of Physics, Experimental Biophysics and Space Sciences, Freie Universität Berlin, Arnimallee 14, 14195 Berlin, Germany
9 SLAC National Accelerator Laboratory, 2575 Sand Hill Road, Menlo Park, California 94025, USA
Understanding the behavior of matter at extreme pressures of the order of a megabar (Mbar) is essential to gain insight into various physical phenomena at macroscales—the formation of planets, young stars, and the cores of super-Earths, and at microscales—damage to ceramic materials and high-pressure plastic transformation and phase transitions in solids. Under dynamic compression of solids up to Mbar pressures, even a solid with high strength exhibits plastic properties, causing the induced shock wave to split in two: an elastic precursor and a plastic shock wave. This phenomenon is described by theoretical models based on indirect measurements of material response. The advent of x-ray free-electron lasers (XFELs) has made it possible to use their ultrashort pulses for direct observations of the propagation of shock waves in solid materials by the method of phase-contrast radiography. However, there is still a lack of comprehensive data for verification of theoretical models of different solids. Here, we present the results of an experiment in which the evolution of the coupled elastic–plastic wave structure in diamond was directly observed and studied with submicrometer spatial resolution, using the unique capabilities of the x-ray free-electron laser (XFEL). The direct measurements allowed, for the first time, the fitting and validation of the 2D failure model for diamond in the range of several Mbar. Our experimental approach opens new possibilities for the direct verification and construction of equations of state of matter in the ultra-high-stress range, which are relevant to solving a variety of problems in high-energy-density physics.
Matter and Radiation at Extremes
2023, 8(6): 066601
Author Affiliations
Abstract
1 ELI Beamlines Facility The Extreme Light Infrastructure ERIC Dolni Brezany Czech Republic
2 Institute of Plasma Physics & Laser Microfusion (IPPLM) Warsaw Poland
3 Southern National Laboratory (LNS) Istituto Nazionale Fisica Nucleare Catania Italy
4 Czech Technical University in Prague Faculty of Nuclear Sciences and Physical Engineering Prague Czech Republic
5 FZU-Institute of Physics Czech Academy of Sciences Prague Czech Republic
6 Institute of Plasma Physics Czech Academy of Sciences Prague Czech Republic
7 Micro-Nano Facility Fondazione Bruno Kessler Trento 38123 Italy
8 Centre for Light-Matter Interactions School of Mathematics and Physics Queen’s University Belfast Belfast UK
Solid-state nuclear track detectors (CR-39 type) are frequently used for the detection of ions accelerated by laser-plasma interaction because they are sensitive to each single particle. To the present day, CR-39 detectors are the main diagnostics in experiments focused on laser-driven proton-boron (p11B) fusion reactions to detect alpha particles, which are the main products of such a nuclear reaction, and to reconstruct their energy distribution. However, the acceleration of multispecies ions in the laser-generated plasma makes this spectroscopic method complex and often does not allow to unambiguously discriminate the alpha particles generated from p11B fusion events from the laser-driven ions. In this experimental work, performed at the PALS laser facility (600 J, 300 ps, laser intensity 1016 W/cm2), CR-39 detectors were used as main detectors for the angular distribution of the produced alpha particles during a p11B fusion dedicated experimental campaign. Additionally, a CR-39 detector was set inside a Thomson Parabola (TP) spectrometer with the aim to calibrate the CR-39 response for low energetic laser-driven ions originating from the plasma in the given experimental conditions. The detected ion energies were ranging from hundreds of keV to a few MeV, and the ion track diameters were measured for etching times up to 9 hours. The goal of the test was the evaluation of the detectors’ ability to discriminate the alpha particles from the aforementioned ions. Within this study, the calibration curves for protons and silicon low energy ions are accomplished, the overlapping of the proton tracks and alpha particles is verified, and a methodology to avoid this problem is realized.
Laser and Particle Beams
2023, 2023(1): 3125787
Author Affiliations
Abstract
1 Merchant Marine College Shanghai Maritime University Shanghai 201306 China
2 Center for Ultimate Energy Shanghai Tech University Shanghai 201210 China
Laser-driven wakefield acceleration (LWFA) has attracted lots of attention in recent years. However, few writers have been able to make systematic research into the bow waves generated along with the wake waves. Research about the bow waves will help to improve the understanding about the motion of the electrons near the wake waves. In addition, the relativistic energetic electron density peaks have great potential in electron acceleration and reflecting flying mirrors. In this paper, the bow waves generated in laser-plasma interactions as well as the effects of different laser and plasma parameters are investigated. Multidimensional particle-in-cell simulations are made to present the wake waves and bow waves by showing the electron density and momentum distribution as well as the electric field along x and y directions. The evolution of the bow wave structure is investigated by measuring the open angle between the bow wave and the wake wave cavity. The angle as well as the peak electron density and transverse momentum is demonstrated with respect to different laser intensities, spot sizes, plasma densities, and preplasma lengths. The density peak emits high-order harmonics up to 150 orders and can be a new kind of “flying mirror” to generate higher order harmonics. The study on the bow waves is important for further investigation on the electron motion around the wake waves, generation of dense electron beams, generation of high-order harmonics, and other research and applications based on the bow waves.
Laser and Particle Beams
2023, 2023(1): 9414451
Author Affiliations
Abstract
1 Joint Institute of High Temperature of Russian Academy of Sciences, Moscow125412, Russia
2 Joint Institute of High Temperature of Russian Academy of Sciences, Moscow125412, Russia
3 Keldysh Institute of Applied Mathematics, Russian Academy of Sciences, Moscow 125047, Russia
4 Beijing National Laboratory of Condensed Matter Physics, Institute of Physics, Chinese Academy of Sciences, Beijing 100080, China
5 Beijing National Laboratory of Condensed Matter Physics, Institute of Physics, Chinese Academy of Sciences, Beijing 100080, China
6 Department of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai200240, China
In this work, we optimized a clean, versatile, compact source of soft X-ray radiation $(E_{\text{x}\text{-}\text{ray}}\sim 3~\text{keV})$ with an yield per shot up to $7\times 10^{11}~\text{photons}/\text{shot}$ in a plasma generated by the interaction of high-contrast femtosecond laser pulses of relativistic intensity $(I_{\text{las}}\sim 10^{18}{-}10^{19}~\text{W}/\text{cm}^{2})$ with supersonic argon gas jets. Using high-resolution X-ray spectroscopy approaches, the dependence of main characteristics (temperature, density and ionization composition) and the emission efficiency of the X-ray source on laser pulse parameters and properties of the gas medium was studied. The optimal conditions, when the X-ray photon yield reached a maximum value, have been found when the argon plasma has an electron temperature of $T_{\text{e}}\sim 185~\text{eV}$, an electron density of $N_{\text{e}}\sim 7\times 10^{20}~\text{cm}^{-3}$ and an average charge of $Z\sim 14$. In such a plasma, a coefficient of conversion to soft X-ray radiation with energies $E_{\text{x}\text{-}\text{ray}}\sim 3.1\;(\pm 0.2)~\text{keV}$ reaches $8.57\times 10^{-5}$, and no processes leading to the acceleration of electrons to MeV energies occur. It was found that the efficiency of the X-ray emission of this plasma source is mainly determined by the focusing geometry. We confirmed experimentally that the angular distribution of the X-ray radiation is isotropic, and its intensity linearly depends on the energy of the laser pulse, which was varied in the range of 50–280 mJ. We also found that the yield of X-ray photons can be notably increased by, for example, choosing the optimal laser pulse duration and the inlet pressure of the gas jet.
clean X-ray source gas jets laser plasma laser–gas interaction soft X-rays 
High Power Laser Science and Engineering
2020, 8(2): 02000e26
Author Affiliations
Abstract
1 ELI Beamlines, Institute of Physics, 5. května 835, 252 41 Dolní B?e?any, Czech Republic
2 Institute of Applied Physics of the Russian Academy of Sciences (IAP RAS), 46 Ul’yanov Street, 603950 Nizhny Novgorod, Russia
3 LULI—CNRS, Ecole Polytechnique, CEA: Université Paris-Saclay
4 UPMC Univ Paris 06: Sorbonne Universities, F-91128 Palaiseau Cedex, France
5 Research Center Toptec, Institute of Plasma Physics, Sobotecká 1660, 511 01 Turnov, Czech Republic
6 Joint Institute for High Temperatures Russian Academy of Science (JIHT RAS), Moscow 125412, Russia
7 Division of Electrical, Electronic and Information Engineering, Graduate School of Engineering, Osaka University, Osaka, Japan
8 Central Laser Facility, STFC Rutherford Appleton Laboratory, Didcot OX11 0QX, United Kingdom
9 Department of Physics SUPA, University of Strathclyde, Glasgow G4 0NG, United Kingdom
10 European XFEL GmbH, Holzkoppel 4, 22869 Schenefeld, Germany
The design of ellipsoidal plasma mirrors (EPMs) for the PEARL laser facility is presented. The EPMs achieve a magnification of 0.32 in focal spot size, and the corresponding increase in focused intensity is expected to be about 8. Designing and implementing such focusing optics for short-pulse (<100 fs) systems paves the way for their use in future high-power facilities, where they can be used to achieve intensities beyond 1023 W/cm2. A retro-imaging-based target alignment system is also described, which is used to align solid targets at the output of the ellispoidal mirrors (with a numerical aperture of 0.75 in this case).
Matter and Radiation at Extremes
2019, 4(2): 024402

关于本站 Cookie 的使用提示

中国光学期刊网使用基于 cookie 的技术来更好地为您提供各项服务,点击此处了解我们的隐私策略。 如您需继续使用本网站,请您授权我们使用本地 cookie 来保存部分信息。
全站搜索
您最值得信赖的光电行业旗舰网络服务平台!