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P. San Miguel Clavería ( presented by S. Corde)

Explore the use of gamma-ray radiation in beam-plasma interaction to diagnose emittance growth in PWFA and beam filamentation instabilities. Discuss experiments, electromagnetic filamentation instabilities, beam emittance, and solutions for emittance preservation. Learn about betatron radiation, beam matching, and the role of plasma wakefield accelerators in accelerating beams efficiently. Delve into the impact of chromaticity spread and methods for measuring and mitigating emittance growth. This study aims to enhance understanding and optimization of beam parameters in plasma wakefield accelerators.

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P. San Miguel Clavería ( presented by S. Corde)

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  1. Gamma-ray radiation in beam-plasma interaction as a diagnostics for emittancegrowth in PWFA and for beamfilamentationinstabilities P. San Miguel Clavería (presented by S. Corde) Sep 16, 2019, EAAC 2019

  2. Part I – E-300 experiment: Energydoubling of narrowenergy spread witnessbunchwhilepreservingemittancewith a high pump-to-witnessenergytransferefficiency in a plasma wakefieldaccelerator • Introduction to PWFA. • Betatron radiation and emittancepreservation. Part II – E-305 experiment: Beamfilamentation and bright gamma-ray bursts • Electromagneticfilamentationinstabilities for particlebeams in plasmas • Exponentialgrowth of gamma-ray production. Experiments to startearly 2020 at the FACET-II facility

  3. Part I: PWFA Introduction • From linear theory:(z = longitudinal direction, x,y = transverse direction) • Plasma density wave. • Wake amplitude is maximized for Plasma acc. gradient ≫ RF cavity acc. gradient (blow-out regime: ) 1

  4. Part I: PWFA Introduction • From linear theory:(z = longitudinal direction, x,y = transverse direction) • Plasma density wave. • Wake amplitude is maximized for Plasma acc. gradient ≫ RF cavity acc. gradient (blow-out regime: ) « 9 GeVenergy gain in a beam-driven plasma wakefieldaccelerator », M Litoset al 2016 Plasma Phys. Control. Fusion 58 034017 Next milestone: Beam Quality 1

  5. PWFA Introduction: Beamemittance Collective variables Beam parameters • Beam radius . • Beam divergence . () • Geometrical emittance: (Tracespace area occupied by the particles) • Normalized emittance: 2

  6. PWFA Introduction: Beamemittance Collective variables Beam parameters • Beam radius . • Beam divergence . () • Geometrical emittance: (Tracespace area occupied by the particles) • Normalized emittance: Linear transverse fields Blow-out regime () . • Beam envelope oscillations at • Beam matching, . • Trace-space ellipse rotation at (unless matched). • is conserved for monoenergetic beams 2

  7. PWFA Introduction: Beamemittance If the beam is not matched and is not monoenergetic… Chromaticity spread is one of the main contributions to the emittance growth in PWFA experiments 3

  8. PWFA Introduction: Beamemittance If the beam is not matched and is not monoenergetic… Chromaticity spread is one of the main contributions to the emittance growth in PWFA experiments Solution: beam matching Matched beam Mismatched beam QuickPIC simulations 3

  9. PWFA Introduction: Beamemittance If the beam is not matched and is not monoenergetic… Chromaticity spread is one of the main contributions to the emittance growth in PWFA experiments Solution: beam matching Matched beam Mismatched beam QuickPIC simulations Can we experimentally measure beam matching? 3

  10. Betatron radiation and emittancepreservation. Radiated energy per betatron period [S. Corde, 2013, Femtosecond X-rays from Laser-Plasma Accelerators,Rev. Mod. Phys. 85, 1 (2013) arXiv:1301.5066. ] E-300 experiment Mismatched propagation Increase in radiated energy QuickPIC Simulations with FACET II beam parameters + radiation post-processing: Liénard-Wiechert potentials with synchrotron approximation 4

  11. Betatron radiation and emittancepreservation. Plasma density profile Beam parameters at trailing waist n/n0 Drive-trailing separation Focal plane separation E-300 experiment z (cm) Scan for different trailing (and drive) focal plane position Trailing focal plane position Trailing focal plane position 5

  12. Betatron radiation and emittancepreservation. Plasma density profile Beam parameters at trailing waist Trailing radiation n/n0 Drive-trailing separation Focal plane separation E-300 experiment z (cm) Scan for different trailing (and driving) focal plane position 5

  13. Betatron radiation and emittancepreservation. Plasma density profile Beam parameters at trailing waist Trailing radiation Drive bunch also emits betatron radition n/n0 Drive-trailing separation Focal plane separation E-300 experiment z (cm) Scan for different trailing (and driving) focal plane position 5

  14. Betatron radiation and emittancepreservation. Beam parameters at trailing waist Trailing radiation Drive-trailing separation Focal plane separation E-300 experiment Drive + trailing radiation Different drive-trailing matching conditions blurs out the correlation between emittance growth and radiated energy. • Solutions: • Spectral/angular information. • Statistical subtraction of drive-only radiation. 6

  15. Betatron radiation and emittancepreservation. Radiation spectra Beam parameters at trailing waist Drive-trailing separation Focal plane separation E-300 experiment Angular distributions 400 300 • Betatron angular profiles very different between the matched trailing beam and the drive beam • Drive angular distribution: different x-y focal plane position makes cross-shaped betatron angular profiles. 300 200 (a.u.) (a.u.) 200 100 100 0 0 7

  16. Part II: BeamFilamentationInstabilities • Transverse beam stability: • If the beam is focused towards a stable equilibrium: stable plasma-wave excitation. • If the beam undergoes transverse instabilities. Plasma return current flows inside the relativistic e- beam. FACET 10 GeV Electron Bunch Evolution during propagation over 1.5 mm of Al (1.8.1023 cm-3 ) Two inter-penetrating e- flows. E-305 experiment Large variety of EM-modes can develop from noise Weibel (CFI), Oblique, Two-stream They break up the beam. Which mode has the fastest growth rate? What is the amplitude of those modes? How do they affect the beam? 8

  17. Part II: BeamFilamentationInstabilities and ɣ-ray generation. Gamma rays in solids Once filamentation instability has developed, beam electrons experience large electromagnetic fields, bending their trajectories, and leading to synchrotron-type gamma-ray emission. Full PIC (CALDER) simulations to model filamentation process and ɣ-ray generation. 3D Calder PIC Simulation E-305 experiment 9

  18. Part II: BeamFilamentationInstabilities and ɣ-ray generation. Gamma rays in solids Once filamentation instability has developed, beam electrons experience large electromagnetic fields, bending their trajectories, and leading to synchrotron-type gamma-ray emission. Peak bunch density is varied keeping bunch charge and emittance constant. Full PIC (CALDER) simulations to model filamentation process and ɣ-ray generation. 3D Calder PIC Simulation E-305 experiment Conversion efficiency 2D Calder PIC Simulation with 10 GeV FACET beam 9

  19. Summary & Conclusions PART I: Betatron radiation and emittance preservation (E-300) • Integrated betatron radiated signal can be used to assess emittance growth due to chromaticity spread in a PWFA accelerator. • Challenge: retrieve betatron radiation emitted by the trailing beam from the drive+trailing radiation PART II: Gamma-ray production during filamentation instabilities (E-305) • Gamma-ray production during beam filamentation instabilities in a beam-solid interaction can provide information about the evolution of the instability. 10

  20. Summary & Conclusions E-300 and E-305 Collaboration: Ecole Polytechnique/LOA: P. San Miguel Claveria, O. Kononenko, G. Raj and S. CordeUCLA: C. Zhang, N. Zan, H. Fujji, K. A. Marsh, W. B. Morri, and C. Joshi SLAC: D. Storey, B. O'Shea, M. Hogan, F. Fiuza and V. Yakimenko CU Boulder: K. Huntstone, M. LitosStonybrook U: N. Vafaei-Najafabadi U. Oslo: E. Adli Tsinghua U.: W. Lu CEA: X. Davoine and L. GremilletMPIK: M. Tamburini and C. H. Keitel Thank you for your attention 11

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