Compression of X-ray free electron laser pulses to attosecond duration

Scientific Reports Nature Publishing Group 5 (2015) 16755-16755

Authors:

James D Sadler, Ricky Nathvani, Piotr Oleśkiewicz, Luke A Ceurvorst, Naren Ratan, Muhammad F Kasim, Raoul MGM Trines, Robert Bingham, Peter Norreys

Abstract:

State of the art X-ray Free Electron Laser facilities currently provide the brightest X-ray pulses available, typically with mJ energy and several hundred femtosecond duration. Here we present one- and two-dimensional Particle-in-Cell simulations, utilising the process of stimulated Raman amplification, showing that these pulses are compressed to a temporally coherent, sub-femtosecond pulse at 8% efficiency. Pulses of this type may pave the way for routine time resolution of electrons in nm size potentials. Furthermore, evidence is presented that significant Landau damping and wave-breaking may be beneficial in distorting the rear of the interaction and further reducing the final pulse duration.

Developed turbulence and nonlinear amplification of magnetic fields in laboratory and astrophysical plasmas.

Proceedings of the National Academy of Sciences of the United States of America National Academy of Sciences 112:27 (2015) 8211-8215

Authors:

Jena Meinecke, Petros Tzeferacos, Anthony R Bell, Robert Bingham, Rob J Clarke, Eugene M Churazov, Robert Crowston, Hugo Doyle, R Paul Drake, Rob Heathcote, Michel Koenig, Yasuhiro Kuramitsu, Carolyn C Kuranz, Daniel Lee, Michael J MacDonald, Chris D Murphy, Margaret M Notley, Hye-Sook Park, Alexander Pelka, Alessandra Ravasio, Brian Reville, Youichi Sakawa, Willow C Wan, Nigel C Woolsey, Roman Yurchak

Abstract:

The visible matter in the universe is turbulent and magnetized. Turbulence in galaxy clusters is produced by mergers and by jets of the central galaxies and believed responsible for the amplification of magnetic fields. We report on experiments looking at the collision of two laser-produced plasma clouds, mimicking, in the laboratory, a cluster merger event. By measuring the spectrum of the density fluctuations, we infer developed, Kolmogorov-like turbulence. From spectral line broadening, we estimate a level of turbulence consistent with turbulent heating balancing radiative cooling, as it likely does in galaxy clusters. We show that the magnetic field is amplified by turbulent motions, reaching a nonlinear regime that is a precursor to turbulent dynamo. Thus, our experiment provides a promising platform for understanding the structure of turbulence and the amplification of magnetic fields in the universe.

Self-similar energetics in large clusters of galaxies

Nature Springer Nature 523:7558 (2015) 59-62

Authors:

Francesco Miniati, Andrey Beresnyak

Charm & MPI: Combining the Best of Both Worlds

Institute of Electrical and Electronics Engineers (IEEE) (2015) 655-664

Authors:

Nikhil Jain, Abhinav Bhatele, Jae-Seung Yeom, Mark F Adams, Francesco Miniati, Chao Mei, Laxmikant V Kale

Simulation of density measurements in plasma wakefields using photon acceleration

Physical Review Accelerators and Beams American Physical Society (APS) 18:3 (2015) 032801

Authors:

Muhammad Firmansyah Kasim, Naren Ratan, Luke Ceurvorst, James Sadler, Philip N Burrows, Raoul Trines, James Holloway, Matthew Wing, Robert Bingham, Peter Norreys