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

THE MATRYOSHKA RUN. II. TIME-DEPENDENT TURBULENCE STATISTICS, STOCHASTIC PARTICLE ACCELERATION, AND MICROPHYSICS IMPACT IN A MASSIVE GALAXY CLUSTER

The Astrophysical Journal American Astronomical Society 800:1 (2015) 60

Quantitative single shot and spatially resolved plasma wakefield diagnostics

Physical Review Special Topics: Accelerators and Beams American Physical Society 18:8 (2015)

Authors:

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

Abstract:

Diagnosing plasma conditions can give great advantages in optimizing plasma wakefield accelerator experiments. One possible method is that of photon acceleration. By propagating a laser probe pulse through a plasma wakefield and extracting the imposed frequency modulation, one can obtain an image of the density modulation of the wakefield. In order to diagnose the wakefield parameters at a chosen point in the plasma, the probe pulse crosses the plasma at oblique angles relative to the wakefield. In this paper, mathematical expressions relating the frequency modulation of the laser pulse and the wakefield density profile of the plasma for oblique crossing angles are derived. Multidimensional particle-in-cell simulation results presented in this paper confirm that the frequency modulation profiles and the density modulation profiles agree to within 10%. Limitations to the accuracy of the measurement are discussed in this paper. This technique opens new possibilities to quantitatively diagnose the plasma wakefield density at known positions within the plasma column.

THE ZURICH ENVIRONMENTAL STUDY (ZENS) OF GALAXIES IN GROUPS ALONG THE COSMIC WEB. V. PROPERTIES AND FREQUENCY OF MERGING SATELLITES AND CENTRALS IN DIFFERENT ENVIRONMENTS**Based on observations collected at the European Southern Observatory, La Silla Chile. Program ID 177.A-0680.

The Astrophysical Journal American Astronomical Society 797:2 (2014) 127

Authors:

A Pipino, A Cibinel, S Tacchella, CM Carollo, SJ Lilly, F Miniati, JD Silverman, JH van Gorkom, A Finoguenov