6-11 November 2022
Hyatt Regency Long Island
America/New_York timezone

Experimental demonstration of Hydrodynamic Optical-Field-Ionized plasma channels at kHz repetition rate

10 Nov 2022, 08:30
20m
Salon D

Salon D

Contributed Oral WG1 Oral: Laser-Plasma Wakefield Acceleration WG1: Laser-Plasma Wakefield Acceleration

Speaker

James Cowley (John Adams Institute for Accelerator Science and Department of Physics, University of Oxford)

Description

Many potential applications of plasma accelerators - such as light sources and future particle colliders - require the stable generation of multi-GeV electron bunches at high (>kHz) repetition rate. A consequent goal for current research into laser-driven plasma accelerators involves the development of waveguides capable of operating at densities of ~1017 cm-3, over lengths of several centimetres or more, guiding laser pulses at kHz repetition rate. Whilst guiding structures such as capillaries are not well suited to this repetition rate due to laser damage and heating, plasma waveguides formed from hydrodynamic optical-field-ionized (HOFI) channels can potentially meet the requirements. Guiding of high intensity laser pulses in HOFI channels has been demonstrated previously at on-axis densities of 1 $\times$ 1017 cm-3 over lengths of >10 cm, whilst in this work we demonstrate experimentally that HOFI channels can be generated at kHz-scale repetition rates for an extended period of time. Using a pump-probe arrangement, we show via transverse interferometry that the properties of two HOFI channels generated 1 ms apart are essentially the same, and that HOFI channels can be generated at a mean repetition rate of 0.4 kHz for a period of 6.5 hours without degradation of the channel properties. The results suggest that HOFI channels are ideal for future high-repetition rate, multi-GeV laser-plasma accelerator stages.

Acknowledgments

This work was supported by the UK Science and Technology Facilities Council (STFC UK) [grant numbers ST/P002048/1, ST/R505006/1]; the Engineering and Physical Sciences Research Council [EP/V006797/1]. This material is based upon work supported by the Air Force Office of Scientific Research under award number FA9550-18-1-7005. This work was supported by the European Union’s Horizon 2020 research and innovation programme under grant agreement No. 653782. This work was supported by ‘la Caixa’ Foundation (ID 100010434) [fellowship code LCF/BQ/PI20/11760027]; Xunta de Galicia (Centro singular de investigacion de Galicia accreditation 2019-2022); European Union ERDF; and the ‘Maria de Maeztu’ Units of Excellence program MDM-2016-0692 and the Spanish Research State Agency.

Primary authors

Aaron Alejo (Instituto Galego de Fisica de Altas Enerxias, Universidade de Santiago de Compostela, Spain) James Cowley (John Adams Institute for Accelerator Science and Department of Physics, University of Oxford) Alexander Picksley (John Adams Institute for Accelerator Science and Department of Physics, University of Oxford) Roman Walczak (John Adams Institute for Accelerator Science and Department of Physics, University of Oxford) Simon Hooker (John Adams Institute for Accelerator Science and Department of Physics, University of Oxford)

Presentation Materials