Direct Laser Acceleration of Bethe-Heitler positrons in laser-channel interactions

TL;DR

This paper introduces a novel plasma-based method for positron acceleration using a powerful laser in a dense plasma channel, potentially enabling high-energy positron beams for future colliders and laboratory astrophysics.

Contribution

It proposes a new laser-driven positron acceleration scheme with a theoretical model and validation through simulations, demonstrating high energy gain and guiding of positrons.

Findings

Achieved high average energy gain rate of a few TeV/m.

Validated the theoretical model with Quasi-3D PIC simulations.

Produced GeV-level electrons, positrons, and x-rays in the fireball jet.

Abstract

Positron creation and acceleration is one of the major challenges for constructing future lepton colliders. On the one hand, conventional technology can provide a solution, but at a prohibitive cost and scale. On the other hand, alternative, reduced-scale ideas for positron beam generation could bring this dream closer to reality. Here we propose a novel plasma-based positron acceleration method using a powerful laser propagating through a dense and narrow plasma channel. A large amount of electrons is injected within the channel during laser propagation. This electron loading creates static fields in the plasma, enabling positrons to be guided transversely while they directly gain energy from the laser field itself. Within this context, we present a theoretical model to describe how the laser injects the electrons and estimate the beam-loaded effective electron density. We validate our theoretical predictions through Quasi-3D PIC simulations and demonstrate the robustness of this guiding and direct laser acceleration process for positrons. Our approach could pave the way for testing this new positron acceleration scheme at ELI-Beamlines, showcasing unprecedentedly high average energy gain rate of a few TeV/m. The fireball jet produced contains GeV-level electrons, positrons, and x-rays, opening the path towards potential laboratory astrophysics experiments using these beams.