Yen-Yu Chang, Li-Chung Ha, Yen-Mu Chen Chih-Hao Pai Investigato r Jypyng Wang, Szu-yuan Chen, Jiunn-Yuan Lin Contributing Students Institute of Atomic and Molecular Sciences, Academia Sin ica, Taiwan National Central University, Taiwan Production of intense ultrashort mid-IR pulses from a laser-wakefield electron accelerator
32
Embed
Yen-Yu Chang, Li-Chung Ha, Yen-Mu Chen Chih-Hao Pai Investigator Jypyng Wang, Szu-yuan Chen, Jiunn-Yuan Lin Contributing Students Institute of Atomic and.
This document is posted to help you gain knowledge. Please leave a comment to let me know what you think about it! Share it to your friends and learn new things together.
Transcript
Yen-Yu Chang, Li-Chung Ha, Yen-Mu Chen
Chih-Hao Pai
Investigator Jypyng Wang, Szu-yuan Chen, Jiunn-Yuan Lin
Contributing Students
Institute of Atomic and Molecular Sciences, Academia Sinica, TaiwanNational Central University, Taiwan
Production of intense ultrashort mid-IR pulses from a laser-wakefield electron accelerator
Methods for the generation of sub-ps mid-IR pulses
Laser-wakefield electron accelerator operated in the bubble regime
Experimental setup and tomographic measurement
Generation of intense ultrashort mid-infrared pulses in the bubble regime
The spectral profile of the MIR pulse suggests that the MIR pulse is produced by the strong spectral broadening of the pump pulse in the bubble regime.
> 1.85 a continuous distribution extending from the short wavelength side
0
Dependence of MIR spectra on interaction length
The spectral profile of the MIR pulse suggests that the MIR pulse is produced by the strong spectral broadening of the pump pulse in the bubble regime.
The Raman satellite is related to the modulational instability of the pump pulse in the early stage of the bubble regime evolution.
0
The MIR pulse is linearly polarized with the same polarization as the pump pulse. This is consistent with the bubble-regime model since the spectral broadening by phase modulation should preserve the pump laser polarization.
Polarization of the MIR pulse
polarization axis of the pump pulse
(1) coherent transition radiation from the electron bunch passing the plasma-vacuum boundary
(2) Cherenkov-type emission fr
om the electron bunch or the plasma wave
Both are radially polarized.
The data rule out the possibility of other mechanisms
Ref: Leemans et al., Phys. Rev. Lett. 91, 074802 (2003)
The MIR pulse is a flattop distribution with its diameter determined by the clear aperture of the ZnSe vacuum window.
The angular divergence of the MIR pulse is larger than the collection angle (8°) and the total MIR pulse energy should be considerably larger than 3 mJ.
• Code: VORPAL• Laser pulse: energy: 205 mJ central wavelength: 810 nm pulse length: 42 fs beam size: 8 m in FWHM peak laser intensity: 6×1018 W/cm2 linearly polarized in z direction
0 x
moving window
light speed
Lramp
z
• Uniform plasma density: 4.1×1019 cm-3
Lramp = 500 m, flattop = 1.6 mm
flattop
• Size of window: Lx = 64 m Ly = Lz = 100 m• Size of gird: 2560 cells in X 250×250 cells in Y and Z• 4 particles per cell
1. The pump pulse undergoes phase modulation imposed by the plasma wave and relativistic self-phase modulation. As a result, the laser spectrum broadens.
2. The laser pulse with its pulse duration longer than the plasma period breaks up into a pulse train.
3. As a result of spectrum broadening, the laser pulse in the bubble undergoes longitudinal self-compression.
4. As the laser intensity gets higher and higher, a plasma bubble is formed. When the plasma bubble evolves into a certain shape and amplitude, a monoenergetic electron beam can be generated.
5. Since most of the photons in the laser pulse stay in the descending slope of the plasma bubble, the spectrum of the laser pulse is mainly broadened toward the long wavelength side.
Simulation-evolution of plasma wave and laser pulse
intensity profile of the laser pulse
Simulation-MIR spectrum and temporal profile
The duration of the MIR pulse is about 20 fs from the simulation, which indicates that the laser peak power may reach 0.4 TW.
The maximum MIR pulse energy is 7 mJ. The spectrum shows a continuous distribution extended from the shorter wavelength side and the trend agrees well with the experimental data.
intensity profile of the MIR pulse covering 2 - 20 m
The MIR pulse is trapped by the plasma bubble, which enables the MIR pulse to propagate through the plasma.
MIR pulse covering 6 - 10 m
Experimental data suggest that the MIR pulse is produced by the strong spectral broadening of the pump pulse in a laser- wakefield electron accelerator operated in the bubble regime.
Production of an intense MIR pulse with at least 3-mJ pulse energy and ultrashort pulse duration from a laser-wakefield electron accelerator is demonstrated. The output energy is one order of magnitude larger than that of the most intense free electron lasers, and three order of magnitude larger than that of conventional wave mixing.
Summary
Thanks for your attention.
The MIR pulse energy increases with plasma density faster than the emergence of the monoenergetic electron beam. This is consistent with the bubble-regime model as the strong spectral broadening and self-compression is the cause of bubble formation.
The MIR pulse has a lower pump energy threshold than that of the monoenergetic electron beam. This is consistent with the bubble-regime model as the strong spectral broadening and self-compression is the cause of bubble formation.
plasma density: 4.1x1019 cm-3
Dependence of MIR energy on pump energy
Simulation-monoenergetic electron beam
The duration of the MIR pulse is about 20 fs from the simulation, which indicates that the laser peak power may reach 0.4 TW.
The maximum MIR pulse energy is 7 mJ. The spectrum shows a continuous distribution extended from the shorter wavelength side and the trend agrees well with the experimental data.
intensity profile of the MIR pulse covering 2 - 20 m
The MIR pulse is trapped by the plasma bubble, which enables the MIR pulse to propagate through the plasma.