Self-modulation of long particle beams

Slides:



Advertisements
Similar presentations
Using the real lattice and an improved model for the wake field, the extraction jitter can now be calculated more accurately. Assuming an injection jitter.
Advertisements

Erdem Oz* USC E-164X,E167 Collaboration Plasma Dark Current in Self-Ionized Plasma Wake Field Accelerators
The scaling of LWFA in the ultra-relativistic blowout regime: Generation of Gev to TeV monoenergetic electron beams W.Lu, M.Tzoufras, F.S.Tsung, C. Joshi,
Particle acceleration in plasma By Prof. C. S. Liu Department of Physics, University of Maryland in collaboration with V. K. Tripathi, S. H. Chen, Y. Kuramitsu,
Modeling narrow trailing beams and ion motion in PWFA Chengkun Huang (UCLA/LANL) and members of FACET collaboration SciDAC COMPASS all hands meeting 2009.
Chapter 4 Waves in Plasmas 4.1 Representation of Waves 4.2 Group velocity 4.3 Plasma Oscillations 4.4 Electron Plasma Waves 4.5 Sound Waves 4.6 Ion Waves.
Experiment with the Slinky
SPACE CHARGE EFFECTS IN PHOTO-INJECTORS Massimo Ferrario INFN-LNF Madison, June 28 - July 2.
Physics of fusion power Lecture 11: Diagnostics / heating.
Longitudinal motion: The basic synchrotron equations. What is Transition ? RF systems. Motion of low & high energy particles. Acceleration. What are Adiabatic.
Lecture 3: Laser Wake Field Acceleration (LWFA)
ELECTROMAGNETIC RADIATION
Goal: to understand waves Objectives: 1)To learn about Oscillations and vibrations 2)To understand the properties of Waves 3)To learn about Transverse.
2 Lasers: Centimeters instead of Kilometers ? If we take a Petawatt laser pulse, I=10 21 W/cm 2 then the electric field is as high as E=10 14 eV/m=100.
Kinetic Effects on the Linear and Nonlinear Stability Properties of Field- Reversed Configurations E. V. Belova PPPL 2003 APS DPP Meeting, October 2003.
Parameter sensitivity tests for the baseline variant Konstantin Lotov, Vladimir Minakov, Alexander Sosedkin Budker Institute of Nuclear Physics SB RAS,
Stability Properties of Field-Reversed Configurations (FRC) E. V. Belova PPPL 2003 International Sherwood Fusion Theory Conference Corpus Christi, TX,
Details of space charge calculations for J-PARC rings.
Nonlinear interaction of intense laser beams with magnetized plasma Rohit Kumar Mishra Department of Physics, University of Lucknow Lucknow
Simulation of direct space charge in Booster by using MAD program Y.Alexahin, A.Drozhdin, N.Kazarinov.
1 Three views on Landau damping A. Burov AD Talk, July 27, 2010.
Lecture Outline Chapter 13 College Physics, 7 th Edition Wilson / Buffa / Lou © 2010 Pearson Education, Inc.
Nonlinear Optics in Plasmas. What is relativistic self-guiding? Ponderomotive self-channeling resulting from expulsion of electrons on axis Relativistic.
W.Lu, M.Tzoufras, F.S.Tsung, C.Joshi, W.B.Mori
SPATIAL RESOLUTION OF NON- INVASIVE BEAM PROFILE MONITORBASED ON OPTICAL DIFFRACTION RADIATION A.P. Potylitsyn Tomsk Polytechnic University, , pr.
Effect of nonlinearity on Head-Tail instability 3/18/04.
A simple formula for calculating the momentum spread from the longitudinal density distribution and RF form Recycler Meeting March 11, 2009 A. Shemyakin.
Collimator wakefields - G.Kurevlev Manchester 1 Collimator wake-fields Wake fields in collimators General information Types of wake potentials.
Chapter 11 Vibrations and Waves.
MHD wave propagation in the neighbourhood of a two-dimensional null point James McLaughlin Cambridge 9 August 2004.
GWENAEL FUBIANI L’OASIS GROUP, LBNL 6D Space charge estimates for dense electron bunches in vacuum W.P. LEEMANS, E. ESAREY, B.A. SHADWICK, J. QIANG, G.
Physics of Self-Modulation Instability Konstantin Lotov Budker Institute of Nuclear Physics SB RAS, Novosibirsk, Russia Novosibirsk State University, Novosibirsk,
Chapter 10 Rüdiger Schmidt (CERN) – Darmstadt TU , version E 2.4 Acceleration and longitudinal phase space.
Simulations of turbulent plasma heating by powerful electron beams Timofeev I.V., Terekhov A.V.
Wakefield excitation by the train of equidistant bunches Konstantin Lotov Budker Institute of Nuclear Physics SB RAS, Novosibirsk, Russia Novosibirsk State.
Latest results on electron trapping and acceleration Konstantin Lotov, Alexey Petrenko, Alexander Sosedkin, Petr Tuev Budker Institute of Nuclear Physics.
Optimal Beamlines for Beams with Space Charge Effect S.V.Miginsky Budker Institute of Nuclear Physics, Novosibirsk, Russia.
Pushing the space charge limit in the CERN LHC injectors H. Bartosik for the CERN space charge team with contributions from S. Gilardoni, A. Huschauer,
Lecture 4 Longitudinal Dynamics I Professor Emmanuel Tsesmelis Directorate Office, CERN Department of Physics, University of Oxford ACAS School for Accelerator.
Helical Accelerating Structure with Controllable Beam Emittance S.V. Kuzikov 1, A.A. Vikharev 1, J.L. Hirshfield 2,3 1 Institute of Applied Physics RAS,
Ionization Injection E. Öz Max Planck Institute Für Physik.
Matching free space propagation to plasma focusing S. Barber UCLA Dept. of Physics and Astronomy FACET II Workshop October 15, 2015.
LCODE: a code for fast simulations of plasma wakefield acceleration Konstantin Lotov Budker Institute of Nuclear Physics SB RAS, Novosibirsk, Russia Novosibirsk.
OPERATED BY STANFORD UNIVERSITY FOR THE U.S. DEPT. OF ENERGY 1 Alexander Novokhatski April 13, 2016 Beam Heating due to Coherent Synchrotron Radiation.
Collective Effect II Giuliano Franchetti, GSI CERN Accelerator – School Prague 11/9/14G. Franchetti1.
Introduction to Plasma Physics and Plasma-based Acceleration
College Physics, 7th Edition
Theory, observations and mitigation of dancing bunches in the Tevatron
Proton-driven plasma wakefield acceleration in hollow plasma
Electron acceleration behind self-modulating proton beam in plasma with a density gradient Alexey Petrenko.
The 2nd European Advanced Accelerator Concepts Workshop
Laboratoire d’Optique Appliquée
Stefano Romeo on behalf of SPARC_LAB collaboration
101° Congresso della societa italiana fisica
Sven Reiche UCLA ICFA-Workshop - Sardinia 07/02
Wakefield Accelerator
The Strong RF Focusing:
Multiturn extraction for PS2
TRANSVERSE RESISTIVE-WALL IMPEDANCE FROM ZOTTER2005’S THEORY
Beam-beam R&D for eRHIC Linac-Ring Option
De Broglie Analysis and Revision
PHYS 1443 – Section 003 Lecture #19
Lect. 06 phase & group velocities
Influence of energetic ions on neoclassical tearing modes
Lesson 3 Forces and Fields
High-power laser pulse propagation in silica
Gain Computation Sven Reiche, UCLA April 24, 2002
2. Crosschecking computer codes for AWAKE
PHYS 1443 – Section 003 Lecture #20
Lecture 24 ACCELERATOR PHYSICS HT E. J. N. Wilson
Presentation transcript:

Self-modulation of long particle beams in plasma wakefield accelerators Konstantin Lotov Budker Institute of Nuclear Physics SB RAS, Novosibirsk, Russia Novosibirsk State University, Novosibirsk, Russia AWAKE Collaboration

Presented by K.Lotov at EAAC-2015, 16.09.2015 The self-modulation instability (SMI) is a cornerstone effect of the AWAKE experiment, so it is important to understand how does it work and why does it work better with the plasma density step. AWAKE [PoP 18, 103101] Beam portrait (2nd half) Excited field (F)

Presented by K.Lotov at EAAC-2015, 16.09.2015 In AWAKE, the self-modulation instability (SMI) is mixed with many other effects, so we introduce a simpler model AWAKE: Plasma of a finite radius Ion motion is of importance Half-Gaussian beam shape (longitudinal) Nonlinear limitation of the wave growth Radius (sr=1) is neither small, nor large Long beam (~150 wave periods), difficult to simulate, does not fit the screen p+, G=400 (long simulation time) Emittance driven divergence The studied case: Infinite radially uniform plasma Immobile ions Constant current beam: Linear plasma response, “Small” radius (analytics available) Look at first 25 periods (L=160) e+, g=1000 (faster simulations, keeps pace with the light) Small angular spread Units of measure: speed of light c for velocities, electron mass m for masses, initial plasma density n0 for densities, inverse plasma frequency ωp−1 for times, plasma skin depth kp−1 = c/ωp for distances, wavebreaking field E0 = mcωp/e for fields; also use ξ = z − ct. Qualitative behavior is important, not the numbers

The quantities to look at: Presented by K.Lotov at EAAC-2015, 16.09.2015 The quantities to look at: (“ax” means on-axis value) The dimensionless wakefield potential: z=0 F = e(E+[ez, B]) = -F Potential well = bunch (even if not formed yet) Location ξj of the j-th potential well (coordinate of the local maximum), Amplitude Φj after j-th bunch (measured as half-amplitude at ξj ) are functions of propagation distance z Maximum amplitude Φm(z,L) By default, L=160 (24 bunches) z=1000

Typical behavior of the maximum amplitude Presented by K.Lotov at EAAC-2015, 16.09.2015 Typical behavior of the maximum amplitude Uniform plasma: 5 stages 1 stage: wakefield structure changes from that of the seed perturbation to that of fastest instability growth. 2 stage: nearly exponential growth (analytically tractable) 3 stage: non-exponential growth 4 stage: fast field decrease 5 stage: almost constant wakefield Here optimum step = steep increase of the plasma density by 8.5% at z = 360. [PRL 107, 145003] Important characteristics: maximum wakefield Φa, established wakefield Φf

Efficiency of long beams in the uniform plasma Presented by K.Lotov at EAAC-2015, 16.09.2015 Efficiency of long beams in the uniform plasma The longer the beam, the smaller is the ratio established/maximum field L=160 Long beams are inefficient in uniform plasmas

The map of density steps Presented by K.Lotov at EAAC-2015, 16.09.2015 The map of density steps The density step must happen at the exponential stage of the instability (not at full bunching) Smooth density increase acts as a sharp step -> length of the transition area is not important There are local maxima at multiples of the optimum step magnitude dn

The optimum step magnitude Presented by K.Lotov at EAAC-2015, 16.09.2015 The optimum step magnitude the optimum step makes the beam exactly one plasma period longer, if measured in local plasma wavelengths first two bunches play a special role in the self-modulation simulations of LHC beam (Phys. Plasmas 18, 103101)

Wave excitation, consequences of the linear theory Presented by K.Lotov at EAAC-2015, 16.09.2015 Wave excitation, consequences of the linear theory Bunch contribution depends on bunch location in the potential well of the master wave decelerated, no focusing amplitude growth, same phase focused, no acceleration same amplitude, phase advance decelerated and focused both amplitude growth and phase advance Complex wave amplitude

Motion of beam particles, how we look at: Presented by K.Lotov at EAAC-2015, 16.09.2015 Motion of beam particles, how we look at: Important: r, ξ, pr Not important: ϕ, pϕ, pz – not considered How to relate with potential wells? Separatrix: We look at −160 < ξ <−147.8 (23rd, 24th bunches) We plot beam particles in (r, ξ, pr)-space and look how they move

Motion of beam particles, the uniform plasma Presented by K.Lotov at EAAC-2015, 16.09.2015 Motion of beam particles, the uniform plasma Potential wells move backward with respect to the beam (already well known fact, vph<c) Why? The wave can grow, only if potential wells contain more decelerated particles than accelerated ones. The potential well attracts (radially) equal numbers of particles to decelerated and accelerated phases. If vph=c, then the densest parts of the beam are at well bottoms, no wave drive. If the well shifts back after attracting particles, then the densest part is decelerated. This is the most efficient way of wave excitation, so it wins against other perturbations

Motion of beam particles, the uniform plasma Presented by K.Lotov at EAAC-2015, 16.09.2015 Motion of beam particles, the uniform plasma As the instability develops, potential wells must move with respect to the beam, trap beam particles at one side and release at the other. This is the exponential stage of wave growth, but it finishes when the beam density is strongly disturbed. What after that? Potential well has no more particles “to eat”, but the wave continues to grow and move (3rd stage), since absence of incoming (accelerated) particles is favorable for wave growth z=0..1000

Motion of beam particles, the uniform plasma Presented by K.Lotov at EAAC-2015, 16.09.2015 Motion of beam particles, the uniform plasma At the field maximum, particle void area approaches the decelerating phase… … but the well continues to move, since: - defocused particles need time to leave, - preceding bunches evolve slower. z=1200

Motion of beam particles, the uniform plasma Presented by K.Lotov at EAAC-2015, 16.09.2015 Motion of beam particles, the uniform plasma At the established state, only a small fraction of beam particles remains in potential wells. (Potential wells are where there are no particles). z=10000

Motion of beam particles, the density step Presented by K.Lotov at EAAC-2015, 16.09.2015 Motion of beam particles, the density step Higher plasma density, shorter plasma wavelength, = a “force” resisting further elongation of the wave period, Proper force => no motion of potential wells note: the number of periods does not change stepped-up uniform stepped-up uniform

Motion of beam particles, the density step Presented by K.Lotov at EAAC-2015, 16.09.2015 Motion of beam particles, the density step Asymmetric well population, how? uniform leading edges are defocused trailing edges are focused bunches move backward in ξ and destroyed in zero Ieff region focused - defocused stepped-up head bunches move like in uniform plasma tail bunches fully survive, but are inefficient middle bunches do the job stepped-up

Instead of conclusion: understanding is good, Presented by K.Lotov at EAAC-2015, 16.09.2015 Instead of conclusion: understanding is good, but which findings are practically useful? Magnitude of the step: Location of the step: stage of the exponential wave growth Beam behavior in the stepped-up plasma is far from the optimal, there is a room for improvements (e.g., with more sophisticated density profiles)

Thank you