Reply to: Reconsidering X-ray plasmons

NATURE PHOTONICS 13:11 (2019) 751-753

Authors:

Lb Fletcher, Hj Lee, T Doppner, E Galtier, B Nagler, P Heimann, C Fortmann, S LePape, T Ma, M Millot, A Pak, D Turnbull, Da Chapman, Do Gericke, J Vorberger, G Gregori, B Barbrel, Rw Falcone, C-C Kao, H Nuhn, J Welch, U Zastrau, P Neumayer, Jb Hastings, Sh Glenzer

(Un)-damning Subplots: The Principate of Domitian Between Literary Sources and Fresh Material Evidence

Illinois Classical Studies University of Illinois Press 44:2 (2019) 242-267

Authors:

Tommaso Spinelli, Gian Luca Gregori

Field reconstruction from proton radiography of intense laser driven magnetic reconnection

Physics of Plasmas AIP Publishing 26:8 (2019)

Authors:

CAJ Palmer, PT Campbell, Y Ma, L Antonelli, AFA Bott, Gianluca Gregori, J Halliday, Y Katzir, P Kordell, K Krushelnick, SV Lebedev, E Montgomery, M Notley, DC Carroll, CP Ridgers, Alexander Schekochihin, MJV Streeter, AGR Thomas, ER Tubman, N Woolsey, L Willingale

Abstract:

Magnetic reconnection is a process that contributes significantly to plasma dynamics and energy transfer in a wide range of plasma and magnetic field regimes, including inertial confinement fusion experiments, stellar coronae, and compact, highly magnetized objects like neutron stars. Laboratory experiments in different regimes can help refine, expand, and test the applicability of theoretical models to describe reconnection. Laser-plasma experiments exploring magnetic reconnection at a moderate intensity (IL ∼1014 W cm-2) have been performed previously, where the Biermann battery effect self-generates magnetic fields and the field dynamics studied using proton radiography. At high laser intensities (ILλL2>1018 Wcm-2μm2), relativistic surface currents and the time-varying electric sheath fields generate the azimuthal magnetic fields. Numerical modeling of these intensities has shown the conditions that within the magnetic field region can reach the threshold where the magnetic energy can exceed the rest mass energy such that σcold = B2/(μ0nemec2) > 1 [A. E. Raymond et al., Phys. Rev. E 98, 043207 (2018)]. Presented here is the analysis of the proton radiography of a high-intensity (∼1018 W cm-2) laser driven magnetic reconnection geometry. The path integrated magnetic fields are recovered using a "field-reconstruction algorithm" to quantify the field strengths, geometry, and evolution.

Interpolation of turbulent magnetic fields and its consequences on diffusive cosmic ray propagation

ArXiv 1907.09934 (2019)

Authors:

L Schlegel, A Frie, B Eichmann, P Reichherzer, J Becker Tjus

Thomson scattering cross section in a magnetized, high-density plasma

Physical Review E American Physical Society 99:6 (2019) 063204

Authors:

Archie FA Bott, Gianluca Gregori

Abstract:

We calculate the Thomson scattering cross section in a nonrelativistic, magnetized, high-density plasma—in a regime where collective excitations can be described by magnetohydrodynamics. We show that, in addition to cyclotron resonances and an elastic peak, the cross section exhibits two pairs of peaks associated with slow and fast magnetosonic waves; by contrast, the cross section arising in pure hydrodynamics possesses just a single pair of Brillouin peaks. Both the position and the width of these magnetosonic-wave peaks depend on the ambient magnetic field and temperature, as well as transport and thermodynamic coefficients, and so can therefore serve as a diagnostic tool for plasma properties that are otherwise challenging to measure.