Hig igh quality ele lectron generation usin ing soli lid or r - - PowerPoint PPT Presentation

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Hig igh quality ele lectron generation usin ing soli lid or r - - PowerPoint PPT Presentation

Hig igh quality ele lectron generation usin ing soli lid or r li liquid target dri riven by X ray la laser Ronghao Hu 1,4 , Zheng Gong 1 , Jinqing Yu 1 , Yinren Shou 1 , Zhengming Sheng 2 , Toshiki Tajima 3 & Xueqing Yan 1 1 Peking


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June 24, 2019 Workshop (Fermilab, Chicago) page 1

Hig igh quality ele lectron generation usin ing soli lid

  • r

r li liquid target dri riven by X ray la laser

Ronghao Hu1,4, Zheng Gong1, Jinqing Yu1, Yinren Shou1, Zhengming Sheng2, Toshiki Tajima3 & Xueqing Yan1†

1 Peking University, China 2 University of Strathclyde, U.K. 3 University of California, Irvine, U.S.A. 4 Sichuan University, China

†x.yan@pku.edu.cn

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June 24, 2019 page 2

Acknowledgement

Workshop (Fermilab, Chicago)

  • Dr. Remi Lehe
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June 24, 2019 page 3 Workshop (Fermilab, Chicago)

Opportunities provided by optical technology

E field(V/m)

1014 1013 1010 108 1012 1011 109

Mourou, G.A., Tajima, T. and Bulanov, S.V., 2006.. Reviews of modern physics, 78(2), p.309.

1 πœˆπ‘› 1 𝑛𝑛 1 π‘œπ‘› 10βˆ’3 π‘œπ‘› 10βˆ’6 π‘œπ‘›

πœ‡ = 2πœŒβ„π‘‘/πœπ›Ώ infrared visible ultraviolet X-ray 𝛿-ray microwave Schwinger limit 1018V/m

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wakefield

June 24, 2019 page 4

Laser wakefield acceleration (LWFA)

Workshop (Fermilab, Chicago)

laser electron

  • S. P. D. Mangles, et al. Nature, 2004, 431(7008): 535–538. 70 MeV 3%
  • C. G. R. Geddes, et al. Nature, 2004, 431(7008): 538–541. 86 MeV 2%
  • J. Faure, et al. Nature, 2004, 431(7008): 541–544. 170 MeV 12%
  • W. P. Leemans, et al. Nature Physics, 2006, 2(10): 696–699. 1 GeV

2.5%

  • X. Wang, et al. Nature Communications, 2013, 4: 1988. 2 GeV

quasi-mono

  • W. P. Leemans, et al. PRL, 2014, 113: 245002. 4.2 GeV

6%

  • A. J. Gonsalves, et al. PRL, 2019, 112: 084801. 8 GeV

quasi-mono energy en-spread

  • T. Tajima, J.M. Dawson,1979. PRL 43(4), p.267.
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June 24, 2019 page 5 Workshop (Fermilab, Chicago)

Facility: Synchrotron light source (Shanghai) Table top light source

Related applications

Accelerating field

Accelection gradient improved 3 orders

𝐹0 = π‘›π‘“π‘‘πœ•π‘ž 𝑓 β‰ˆ 100 π»π‘Š 𝑛 β‹… π‘œ0[1018π‘‘π‘›βˆ’3]

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June 24, 2019 page 6 Workshop (Fermilab, Chicago)

LWFA in solid density material

Reference:

Chen, P. and Noble, R.J., 1987. In Relativistic Channeling (pp. 517-522). Springer, Boston, MA. Chen, P. and Noble, R.J., 1987, May. In AIP Conference Proceedings (Vol. 156, No. 1, pp. 222-227). AIP. Tajima, T. and Cavenago, M., 1987. Physical review letters, 59(13), p.1440. Newberger, B.S. and Tajima, T., 1989. Physical Review A, 40(12), p.6897. Tajima, T., Mahale, N.K., MacKay, W.W., Huson, F.R., Ohnuma, S., Covington, B.C., Payne, J. and Newberger, B.S., 1989. Part. Accel., 32(IFSR-403), pp.235-240. Newberger, B. and Tajima, T., 1989, October. In AIP Conference Proceedings (Vol. 193, No. 1, pp. 290-294). AIP. Dodin, I.Y. and Fisch, N.J., 2008. Physics of Plasmas, 15(10), p.103105. Shin, Y.M., Lumpkin, A.H. and Thurman-Keup, R.M., 2015. Nuclear Instruments and Methods in Physics Research Section B, 355, pp.94-100. Shin, Y.M., Still, D.A. and Shiltsev, V., 2013. Physics of Plasmas, 20(12), p.123106.

𝐹0 = π‘›π‘“π‘‘πœ•π‘ž 𝑓 β‰ˆ 100 π»π‘Š 𝑛 β‹… π‘œ0[1018π‘‘π‘›βˆ’3]

Metallic crystals Carbon nanotube

1019~1023cmβˆ’3 βˆ’β†’ 0.3~30 TeV/m

How can the laser light propagate through the overcritical plasma ?

2~3 orders larger than conventional LWFA !

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June 24, 2019 page 7 Workshop (Fermilab, Chicago)

The state-of-the-art X-ray FEL

Germany

  • U. S. A.

Japan Korea Switzerland

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June 24, 2019 page 8 Workshop (Fermilab, Chicago)

The state-of-the-art X-ray FEL

Location

Germany USA USA USA Japan Switzerland South Korea China

Start of commissioning

2016 2009 2019 2020 2011 2016 2016 2025

Accelerator technology

Super- conducting Normal- conducting Normal- conducting Super- conducting Normal- conducting Normal- conducting Normal- conducting Super- conducting

Number of light flashes per second

27 000 120 120 1 000 000 60 100 60 1 000 000

Minimum wavelength of the laser

0.05 nm 0.15 nm 0.05 nm 0.25 nm 0.08 nm 0.1 nm 0.06 nm 0.05 nm

Maximum e- energy

17.5 GeV 14.3 GeV 15 GeV 5 GeV 8.5 GeV 5.8 GeV 10 GeV 8 GeV

Length of the facility

3.4 km 3 km 3 km 3 km 0.75 km 0.74 km 1.1 km

Number of undulators

3 1 3 1 2

Number of stations

6 5 4 3 3

Peak brilliance

5 x 10

33

2 x 10

33

2 x 10

33

1 x 10

32

1 x 10

33

1 x 10

33

1.3 x 10

33

1 x 10

33

European XFEL LCLS LCLS-II, CuRF LCLS-II, SCRF SACLA SwissFEL PAL-XFEL Shine

Possible to witness the solid material as underdense plasma

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June 24, 2019 page 9 Workshop (Fermilab, Chicago)

Research stimulated by acceleration in metallic crystals

Electric field ~𝐔𝐖/𝐝𝐧 Electron energy ~π‡πŸπ– Accelerator-- e+e- colliders

Higher the accelerating gradient lower financial costs on much shorter timescale

Laboratory astrophysics Novel energetic photon source

Neutron star: 104~1011T (magnetars: 108~1011T ) E~100TV/m --> B ~106T Schwinger limit 𝐹𝑑~1018π‘Š/𝑛 𝛿𝐹 𝐹𝑑 ~0.1 for 𝛿~103, 𝐹~1014V/m Radiation reaction; QED effect

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June 24, 2019 page 10 Workshop (Fermilab, Chicago)

Advantage of x-ray LWFA

Length (e.g. laser spot size) Normalized laser amplitude Plasma density Accelerated beam charge Electron beam emittance Electron beam intensity Electron beam brilliance

Laser plasma scaling law

Lower emittance More brilliant

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June 24, 2019 page 11 Workshop (Fermilab, Chicago)

PIC simulation for x-ray LWFA

Wavelength [nm] 800 4 Plasma density [cmβˆ’3] 6.88 Γ— 1018 2.75 Γ— 1023 (250 nc of 1 micron) a0 1.4 1.4 Waist [nm] 103 50 Duration [fs] 10.55 52.74 Γ— 10βˆ’3 Intensity [W/cm2] 4.2 Γ— 1018 1.7 Γ— 1023 Power[TW] 13.2 13.2 I [kA] 1.12 1.12 Q [pC] 3.67 18.3 Γ— 10βˆ’3 Duration[fs] 3.87 19.4 Γ— 10βˆ’3 Emittance y [nm] 361 1.81 Emittance z [nm] 413 2.07 Brightness [A/mβˆ’2] 1.5 Γ— 1016 6 Γ— 1020

Conventional LWFA x-ray LWFA Simulation parameters rescale

More brilliant !

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June 24, 2019 page 12 Workshop (Fermilab, Chicago)

PIC simulation of x-ray LWFA

Zhang, X., Tajima, T., Farinella, D., Shin, Y., Mourou, G., Wheeler, J., Taborek, P., Chen, P., Dollar, F. and Shen, B., 2016 Physical Review Accelerators and Beams, 19(10), p.101004.

Nano tube target Uniform material

𝐹𝑦~1014π‘Š/m Laser: 𝑏0 = 4 𝐹𝑧~1016π‘Š/𝑛 Gradient ~ TeV/cm

Self-consistent 2D PIC

Density: π‘œπ‘“~10βˆ’3π‘œπ‘‘ π‘œπ‘“~1024/cm3 Solid material ! ~GeV electron beams micron distance

Emittance 18.7 nm two orders smaller !

πœ‡0 = 1π‘œπ‘›

πœ‡0 = 1πœˆπ‘› 𝑏0 = 4,𝐹𝑧~1013π‘Š/𝑛

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June 24, 2019 page 13 Workshop (Fermilab, Chicago)

Improve the quality of electron beam in LWFA

Improve the quality of electron beam injection acceleration Discontinuous injection Low energy spread Chirp control Emittance control High energy & low energy spread

Self-injection Colliding pulse injection Ionization injection Density down-ramp injection

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June 24, 2019 page 14 Workshop (Fermilab, Chicago)

New injection method for X-ray LWFA Driven x-ray laser parameters

Wavelength [nm] 2.5 (495.9eV) Plasma density [cmβˆ’3] 1.5 Γ— 1023 (0.4g/cm3) a0 1.6 Waist [nm] 100 Duration [as] 100 Intensity [W/cm2] 5.61 Γ— 1023 Power[TW] 88.08 Pulse energy 9.38 mJ

Driven x-ray laser liquid methane jet Laser wakefield

Injected electron (in the second bucket)

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June 24, 2019 page 15 Workshop (Fermilab, Chicago)

The ionization of methane molecules in X-ray laser

⚫ Different from the field ionization and tunnel ionization in optical lasers ⚫ Single-photon absorption is dominant in the X-ray regime ⚫ Ionization starts from the inner shells, because the photoionization cross section are considerably higher for inner shells than for the valence shells. molecular dynamics Monte Carlo XMDYN code Hartree-Fock-Slater code XATOM

http://www.desy.de/~xraypac/ calculate the photoionization cross sections and atomic decay rates, ionization dynamics

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June 24, 2019 page 16 Workshop (Fermilab, Chicago)

The ionization process of methane molecules CH4

For carbon atoms irradiated by photons of 495.9 eV Photoabsorption cross section: 1s orbit: 0.154 Mb 2s orbit: 6.7 Γ— 10βˆ’3 MB 2p orbit: 5.1 Γ— 10βˆ’4 MB

main pulse

XMDYN code calculates the ionization processes

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June 24, 2019 page 17 Workshop (Fermilab, Chicago)

Electron injection in sharp vacuum-plasma transition

𝑦 [πœ‡] 𝑦 [πœ‡] y [πœ‡] y [πœ‡]

PIC simulation

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Refluxing Electron Injection (REI)

First bucket Second bucket

Electron trajectory

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Theory of Refluxing Electron Injection (REI)

PIC simulation

Numerical solutions of equations without modifications after sheet crossing Numerical solutions including quasi static wakefield theory after sheet crossing Trajectories obtained from a PIC simulation with the same parameters

The laser is incident from left to right, and plasma initially locates in the x>0 area. 𝑏0 = 1.2 and π‘œ0 = 0.004π‘œπ‘‘ are used in all subfigures. π‘’π‘žπ‘¦ 𝑒𝑒 = βˆ’πΉ + 𝐺

π‘ž

𝑒𝑦 𝑒𝑒 = π‘žπ‘¦ 𝛿 𝐺

π‘ž = βˆ’ 1

4𝛿 πœ–π‘2 πœ–π‘¦ 𝛿 = 1 + π‘žπ‘¦

2 + 𝑏2/2

𝐹 = ࢱ

βˆ’βˆž 𝑦

π‘œπ‘— 𝑦 βˆ’ π‘œπ‘“ 𝑦 𝑒𝑦 = 𝑦𝐼 𝑦 βˆ’ 𝑦0

π‘žπ‘¦ 𝑒, 𝑦0 = βˆ’π‘žπ‘› cos[πœ•π›Ώ(𝑒 βˆ’ 𝑦0/𝑀𝑒 βˆ’ 𝑒0)] 𝑦 𝑒, 𝑦0 = 𝑦0 βˆ’ πœ€π‘› sin[πœ•π›Ώ(𝑒 βˆ’ 𝑦0/𝑀𝑒 βˆ’ 𝑒0)]

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Theory of Refluxing Electron Injection (REI)

𝑦0 + πœ€π‘› sin[πœ•π›Ώ(𝑒𝑑𝑑 βˆ’ 𝑦0/𝑀𝑒 βˆ’ 𝑒𝑠𝑓 βˆ’ 𝑒0)] = πœ€π‘› βˆ’ πœ€π‘› sin[πœ•π›Ώ(𝑒𝑑𝑑 βˆ’ πœ€π‘›/𝑀𝑒 βˆ’ 𝑒0)] 𝑒𝑠𝑓 = 2π‘ž0/𝑦0 + 2arccos(π‘ž0/π‘žπ‘›)/πœ•π›Ώ Refluxing time: 𝑒𝑑𝑑 = 𝑒0 + 𝑦0/𝑀𝑒 + 𝑒𝑠𝑓 + arcsin 𝐡/ 2 + 2 sin 𝐢 βˆ’ 𝐷 /πœ•π›Ώ 𝐡 = 1 βˆ’ 𝑦0/πœ€π‘› 𝐢 = πœ•π›Ώ[(πœ€π‘› βˆ’ 𝑦0)/𝑀𝑒 βˆ’ 𝑒𝑠𝑓] 𝐷 = arcsin[cos(𝐢) / 2 + 2 sin 𝐢 ] π‘žπ‘ π‘“ = π‘žπ‘› cos[πœ•π›Ώ(𝑒𝑑𝑑 βˆ’ 𝑦0/𝑀𝑒 βˆ’ 𝑒𝑠𝑓 βˆ’ 𝑒0)] The momentum of refluxing electron at sheet crossing time 𝑒𝑑𝑑: π‘žπ‘ π‘“ βˆ’ π‘žπ‘‘π‘ž > 0 Injection condition : Separatrix momentum

πœ‡ πœ‡ πœ‡

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The quality of the injected electron beam

bunch size evolution Transverse emittance Transverse phase space Longitudinal phase space

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The quality of the electron bunch from REI

Beam parameters of REI after propagating about 6 micron in plasma obtained from 3D PIC simulations

4~5 orders higher than the state-of-art electron sources

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June 24, 2019 page 23 Workshop (Fermilab, Chicago)

Summary

  • High acceleration gradient in solid wakefield accelerator driven by x-ray laser
  • Reflux electron injection dynamics is investigated theoretically
  • Ultra-high brilliance of the accelerated electron beam
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June 24, 2019 page 24 Workshop (Fermilab, Chicago)

Thanks for your attention !

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Backup sli lides

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Multi dimensional effects of REI

Sometimes in 3D situation, if the laser intensity is relatively large, the reflux electron Injection may take place in the first bucket of the wakefield. 𝑦 [πœ‡] 𝑦 [πœ‡] 𝑧 [πœ‡] 𝑧 [πœ‡]

[πœ‡]

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Electron distribution versus real space

Real space distribution Real space distribution

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The dependence of REI on plasma density distribution

Injected charge in second bucket for different 𝑏0 and plasma density π‘œ0. The red line is the theoretical threshold calculated by solving MAX(π‘žπ‘ π‘“ βˆ’ psp) = 0 Injected charge in second bucket for different a0 and boundary ramp length Injected charge in second bucket for different a0 and density ratio

  • f a transition from plasma with

density π‘œπ‘žπ‘ π‘“ to plasma with π‘œ0

π‘œπ‘žπ‘ π‘“ Ramp length π‘œ0