Compact Petawatt-Class Laser Wakefield Acceleration with Plasma Telescope
arXiv:2308.04710 · doi:10.1063/5.0202964
Abstract
The compactness of laser wakefield acceleration (LWFA) is limited by its long focal length for high power lasers, e.g., more than 10 meters for 1-peatawatt (PW) laser pulse and up to hundreds of meters for 10-100 PW lasers. The long focal length originates from the low damage threshold of the optical off-axial parabolic (OAP) mirror and consequent large spot size. We propose implementing an OAP plasma mirror (PM) to form a telescope geometry, reducing the beam size and hence constraining the focal length to meter-range for LWFA driven by lasers beyond 1PW. Three-dimensional particle-in-cell simulations are performed to characterize the reflection of a 1-PW laser by the plasma OAP and find that optimal condition is achieved within only 1-m optical length. The new method successfully generates 9GeV electron bunch in the subsequent LWFA stage with consistent acceleration gradients to that of the 1-PW laser via ordinary focusing. The proposed geometry provides a solution of compact LWFAs available for even 100-PW laser systems.
References in corpus (8)
- Generating multi-GeV electron bunches using single stage laser wakefield acceleration in a 3D nonlinear regime
- All-optical Compton gamma-ray source
- A spectral, quasi-cylindrical and dispersion-free Particle-In-Cell algorithm
- Optical Properties of Relativistic Plasma Mirrors
- Achieving extreme light intensities using relativistic plasma mirrors
- Multistage Coupling of Laser-Wakefield Accelerators with Curved Plasma Channel
- Sub-laser-cycle control of relativistic plasma mirrors
- Anomalous Relativistic Emission from Self-Modulated Plasma Mirrors