Search arXiv⌕ Search

arXiv · 2610.23243

High average flux positron sources driven by a mJ-class laser

Abstract

We report on the production and characterisation of MeV-scale positron populations driven by a high-repetition-rate, mJ-class laser system. The positrons are generated via a two-step Bethe--Heitler process driven by laser-wakefield-accelerated electron beams propagating through a mm-scale lead converter. At 10 Hz, approximately 1000 positrons in the 0.8--1.7 MeV energy range were measured over 100 accumulated shots. Stable electron acceleration was demonstrated at 10 Hz, 100 Hz, and 1 kHz using approximately 9 mJ of laser energy in the focal spot, indicating the potential for substantially higher average positron fluxes for laser systems operating at kHz repetition rates and energies of 10s of mJ. Such a positron source allows generating sufficiently high average fluxes of MeV-scale positrons while maintaining low positron yields per pulse and narrow temporal distributions, a regime of particular interest for novel applications in material science and fundamental physics. The measured positron yields and spectra are in good agreement with Monte Carlo simulations, supporting the modelling of the positron-production process and magnetic transport system.

Explore related subjects

Keep this discovery

Explore connections, maps & timelines

BibTeXRIS

T. Foster, D. Papp, C. McAnespie, H. Maguire, J. Csontos, E. Gerstmayr, G. M. Grittani, C. Kamperidis, D. J. Keeble, C. M. Lazzarini, S. Lorenz, T. Lucza, S. Tóth, G. Sarri. 2026-10-16. High average flux positron sources driven by a mJ-class laser. https://arxiv.org/abs/2610.23243

Cite the original work for its findings. Save a collection to share your selection of sources.

KEEP EXPLORING

Related papers

Fundamental limit of intensity scaling for harmonic generation on plasma mirrors

Plasma mirrors have the potential to considerably boost the intensity of ultra-intense laser pulses through high-order harmonic generation, offering a promising route to the extreme fields required for probing the strong-field regime of quantum electrodynamics (SF-QED). This prospect relies on the favorable scaling of harmonic generation with increasing laser intensity, a longstanding assumption that has remained untested at extreme intensities. Combining the first measurements of Doppler harmonic generation approaching $10^{22}\,\mathrm{W/cm^2}$ with advanced particle-in-cell modeling, our study reveals fundamental limitations to this scaling. We notably observe a strong reduction of the harmonic yield as the laser intensity is increased, and show using simulations that this originates from the interaction of the sub-picosecond laser pedestal with the plasma mirror. This pedestal drives a rapid evolution of the plasma surface, through radiation-pressure compression and surface modulations, which progressively suppress harmonic generation. By extending our simulations up to intensities of $10^{23}\,\mathrm{W/cm^2}$, we show that this evolution accelerates strongly with increasing intensity, eventually leading to plasma mirror disruption on the timescale of the main laser pulse itself, making pulse duration, in addition to temporal contrast, a second key parameter for efficient harmonic generation. These results reveal the fundamental limits of the intensity scaling of harmonic generation from plasma mirrors and establish the conditions required to preserve efficient harmonic generation at extreme intensities, providing critical guidance for their use as intensity boosters toward the SF-QED regime.

physics.plasm-ph↗

Predictors of filament coil non-planarity in a dataset of QI stellarators

Stellarator magnetic fields are often realized with non-planar modular coils with their out-of-plane bending being one of the main engineering challenges. We ask whether the non planarity of the fialment can be predicted from the equilibrium alone. We look at a dataset of coils for stellarator equilibira and find that the geodesic torsion of the magnetic field line is a strong and robust predictor in a wide range of coil feasibility requirements. We compare the performance of the geodesic torsion against other equilibrium and surface geometry properties and find it to be a superior predictorv hardly replaceable by other quantities we considered in this dataset. The ranking it induces also reproduces the ordering of four published configurations --- precise QA, precise QI at nfp 2 and 3, and W7-X. Our conclusions suggest that geodesic torsion of the magnetic field line may be considered as a cheap and robust candidate for a stage-one non-planarity proxy.

physics.plasm-ph↗

Reduced Molecular Plasma Kinetics with Non-Boltzmann Vibrational Distribution

Vibrational kinetics can strongly affect energy transfer, chemical kinetics, and discharge behavior in molecular plasmas, but resolving all internal states is often impractical for reactor-scale simulation. Compact, physics-based vibrational closures are particularly needed when complete state-to-state (StS) data are limited. Starting from a detailed $\mathrm{H}_2$ StS plasma-kinetics framework coupled to an electron-Boltzmann calculation, this work develops a reduced vibrational-kinetics formulation. The $\mathrm{H}_2$ vibrational ladder is reduced to two non-Boltzmann groups that evolve their population and internal energy. State-resolved reaction rates and associated energy-exchange terms are projected onto the groups for subsequent tabulation in reactor-scale plasma models. StS-informed samples of the reduced-model are propagated for pulsed RF $\mathrm{H}_2$ plasmas across a scan of pulse-averaged absorbed power and compared with the corresponding StS simulations. Predictions from the sampled models reproduce the bulk plasma response, including electron density, atomic-H density, and $\mathrm{H}_3^+$ density. Discrepancies in $\mathrm{H}^-$ production and the upper-energy-group vibrational temperature persist across the sampled reductions. This indicates a limitation of the present VDF reconstruction rather than the nominal parameter choice. Tail-sensitive processes therefore require a more accurate representation of the vibrational distribution.

physics.plasm-ph↗