High-current laser-driven beams of relativistic electrons for high energy density research

Author:

Rosmej O NORCID,Gyrdymov M,Günther M M,Andreev N E,Tavana P,Neumayer P,Zähter S,Zahn N,Popov V S,Borisenko N G,Kantsyrev A,Skobliakov A,Panyushkin V,Bogdanov A,Consoli FORCID,Shen X F,Pukhov A

Abstract

Abstract We report on enhanced laser driven electron beam generation in the multi MeV energy range that promises a tremendous increase of the diagnostic potential of high energy sub-PW and PW-class laser systems. In the experiment, an intense sub-picosecond laser pulse of ∼1019 Wcm−2 intensity propagates through a plasma of near critical electron density (NCD) and drives the direct laser acceleration (DLA) of plasma electrons. Low-density polymer foams were used for the production of hydrodynamically stable long-scale NCD-plasmas. Measurements show that relativistic electrons generated in the DLA-process propagate within a half angle of 1 2 ± 1° to the laser axis. Inside this divergence cone, an effective electron temperature of 10–13 MeV and a maximum of the electron energy of 100 MeV were reached. The high laser energy conversion efficiency into electrons with energies above 2 MeV achieved 23% with a total charge approaching 1 μC. For application purposes, we used the nuclear activation method to characterize the MeV bremsstrahlung spectrum produced in the interaction of the high-current relativistic electrons with high-Z samples and measured top yields of gamma-driven nuclear reactions. The optimization of the high-Z target geometry predicts an ultra-high MeV photon number of ∼1012 per shot at moderate relativistic laser intensity of 1019 Wcm−2. A good agreement between the experimental data and the results of the 3D-PIC and GEANT4-simulations was demonstrated.

Funder

Russian Foundation for Basic Research

Deutsche Forschungsgemeinschaft

H2020 Euratom

Ministry of Science and Higher Education of the Russian Federation

Publisher

IOP Publishing

Subject

Condensed Matter Physics,Nuclear Energy and Engineering

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