Bulletin of the American Physical Society
60th Annual Meeting of the APS Division of Plasma Physics
Volume 63, Number 11
Monday–Friday, November 5–9, 2018; Portland, Oregon
Session YP11: Poster Session IX: The crossover between high-energy-density plasmas and ultracold neutral plasmas ; Supplemental; Post-Deadline Abstracts (9:30am-12:30pm)
Friday, November 9, 2018
OCC
Room: Exhibit Hall A1&A
Abstract ID: BAPS.2018.DPP.YP11.34
Abstract: YP11.00034 : Stacked-pulse driven laser-plasma electron accelerator for compact gamma-ray sources.*
Presenter:
Serge Youri Kalmykov
(University of Nebraska-Lincoln)
Authors:
Serge Youri Kalmykov
(University of Nebraska-Lincoln)
Xavier Davoine
(CEA, DAM, DIF)
Bradley A. Shadwick
(University of Nebraska-Lincoln)
Driving a laser-plasma accelerator (LPA) with an incoherent superposition (stack) of multi-TW optical blocks of different colors opens the way to GeV-scale electron acceleration in a mm-length, dense plasma (n0 ∼ 1019 cm-3), without resorting to single-shot PW facilities. Stack-driven LPA affords production of electron beams (e-beams) at a kHz repetition rate, at a manageable average laser power. Immunity of the stack to self-compression (i) avoids deformation (elongation) of the accelerating bucket (a ``bubble'' of electron density), keeping the e-beam background-free through dephasing, and (ii) delays dephasing, thereby doubling electron energy against the predictions of standard scaling. In our PIC simulations, quasi-monoenergetic e-beams (or trains of such beams, in a single shot) have a 5-D brightness 1016 - 1017 A/m2 and mean energy tunable up to 1 GeV without changing the target. These unconventional beams, inaccessible with standard acceleration techniques, emit highly collimated, quasi-monochromatic, gigawatt γ-ray pulses via Thomson scattering process, in the range 3 - 17 MeV, each pulse corresponding to a distinct energy band (with ∼ 106 photons per band) [S. Y. Kalmykov et al., New J. Phys. 20, 023047 (2018).]
*Supported in part by NSF Grant PHY-1535678.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.YP11.34
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