Setup for meV-resolution inelastic X-ray scattering measurements and X-ray diffraction at the Matter in Extreme Conditions endstation at the Linac Coherent Light Source

Review of Scientific Instruments AIP Publishing 89:10 (2018) 10F104

Authors:

EE McBride, TG White, A Descamps, LB Fletcher, K Appel, F Condamine, CB Curry, S Funk, E Galtier, M Gauthier, S Goede, JB Kim, HJ Lee, BK Ofori-Okai, M Oliver, A Rigby, C Schoenwaelder, P Sun, Th Tschentscher, B Witte, U Zastrau, Gianluca Gregori, B Nagler, J Hastings, SH Glenzer, G Monaco

Abstract:

We describe a setup for performing inelastic X-ray scattering and X-ray diffraction measurements at the Matter in Extreme Conditions (MEC) endstation of the Linac Coherent Light Source. This technique is capable of performing high-, meV-resolution measurements of dynamic ion features in both crystalline and non-crystalline materials. A four-bounce silicon (533) monochromator was used in conjunction with three silicon (533) diced crystal analyzers to provide an energy resolution of ∼50 meV over a range of ∼500 meV in single shot measurements. In addition to the instrument resolution function, we demonstrate the measurement of longitudinal acoustic phonon modes in polycrystalline diamond. Furthermore, this setup may be combined with the high intensity laser drivers available at MEC to create warm dense matter and subsequently measure ion acoustic modes.

Analytical estimates of proton acceleration in laser-produced turbulent plasmas

(2018)

Authors:

Konstantin Beyer, Brian Reville, Archie Bott, Hye-Sook Park, Subir Sarkar, Gianluca Gregori

Turbulent hydrodynamics experiments in high energy density plasmas: scientific case and preliminary results of the TurboHEDP project

HIGH POWER LASER SCIENCE AND ENGINEERING 6 (2018) ARTN e44

Authors:

A Casner, G Rigon, B Albertazzi, Th Michel, T Pikuz, A Faenov, P Mabey, N Ozaki, Y Sakawa, T Sano, J Ballet, P Tzeferacos, D Lamb, E Falize, G Gregori, M Koenig

Experimental platform for the investigation of magnetized-reverse-shock dynamics in the context of POLAR

High Power Laser Science and Engineering Cambridge University Press 6 (2018) e43

Authors:

Gianluca Gregori, B Albertazzi, E Falize, E Falize, A Pelka, F Brack, F Kroll, R Yurchak, E Brambrink, P Mabey, N Ozaki, S Pikuz, L Van Box Som, JM Bonnet-Bidaud, JE Cross, E Filippov, R Kodama, M Mouchet, T Morita, Y Sakawa, RP Drake, CC Kuranz, MJE Manuel, C Li, P Tzeferacos, D Lamb, U Schramm, M Koenig

Abstract:

The influence of a strong external magnetic field on the collimation of a high Mach number plasma flow and its collision with a solid obstacle is investigated experimentally and numerically. The laser irradiation (I ∼ 2 × 1014 W · cm−2 ) of a multilayer target generates a shock wave that produces a rear side plasma expanding flow. Immersed in a homogeneous 10 T external magnetic field, this plasma flow propagates in vacuum and impacts an obstacle located a few mm from the main target. A reverse shock is then formed with typical velocities of the order of 15–20 ± 5 km/s. The experimental results are compared with 2D radiative magnetohydrodynamic simulations using the FLASH code. This platform allows investigating the dynamics of reverse shock, mimicking the processes occurring in a cataclysmic variable of polar type.

Axion driven cosmic magneto-genesis prior to the QCD crossover

Physical Review Letters American Physical Society (2018)

Authors:

F Miniati, G Gregori, B Reville, S Sarkar

Abstract:

We present a mechanism for the generation of magnetic field in the early universe prior to the QCD crossover, assuming that the dark matter is made of pseudoscalar axions. Thermoelectric fields arise due to pressure gradients in the primordial plasma resulting from the difference in charge, energy density and equation of state of the quark and lepton components. The axion field is coupled to the EM field and when its spatial gradient is misaligned with the thermoelectric field an electric current is driven. Due to the finite resistivity of the plasma a generally rotational electric field appears. For a QCD axion mass consistent with observational constraints, a magnetic field is thus generated with strength $B \sim 10^{-11 }$ G and characteristic scale $L_B \sim $ 1 pc at present, and viable values for the combination $BL_B^{1/2}$, which is probed in cosmic voids through $\gamma$-ray observations of distant blazars. The amplitude and spatial/temporal scales of the pressure gradients may in principle be inferred through the detection of the concomitant emission of gravitational waves, while experiments are underway to confirm or rule out the existence of axions, with direct consequences for our predictions.