C. Kamperidis- Table-top laser plasma wakefield electron accelerators
Transcript of C. Kamperidis- Table-top laser plasma wakefield electron accelerators
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Table-top laser
plasma wakefield
electron accelerators
C. KAMPERIDIS
Plasma Physics GroupImperial College London, UK
OLA - CRETE 2008
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Outline
Motivation for table-top/compact particle accelerators
Physics of laser driven wakefield electron accelerators(LWFA)
Ionisation by an intense laser pulse
Particle motion under a laser field / Ponderomotive Force
Plasma waves
Generation of non linear plasma waves
Relativistic plasma wave breaking limit (self-injection)
Energy gain
Energy losses in plasma wave generation
1st Session
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Outline
2nd Session
Propagation of ultra-short, ultra-intense laser pulses in underdense
plasmasNon linearities in plasmasPropagation beyond the Rayleigh length
Schemes of laser driven plasma based electron acceleration
LWFASelf Modulated - LWFA
Experiments performed in multi-TW table-top laser systems
Recent experimental landmarksGeV mono-energetic electron beams from 2D simulations
Conclusions/Applications/The Future
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1st Session Motivation
Review of major state-of-the-art traditional accelerator facilities
Conseil Europen pour la Recherche Nuclaire: www.cern.ch
Large Hadron Collider (LHC) - Multi-TeV proton collision energies
27 km
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1st Session Motivation
DESY synchrotron facility in Hamburg
http://pr.desy.de/e113/indexeng.html
Review of major state-of-the-art traditional accelerator facilities
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1. RF technology is not getting cheaper2010 - proposed ILC (International Linear Collider) will be ready giving500 GeV at an estimated cost of 5 G$
2. RF technology needs a lot of spaceMaximum possible accelerating gradient in RF accelerators (limited by
material electric breakdown): ~ 100 MeV/mILC -> 31.5 MeV/m -> ~15 km
3. RF technology can not deliver ultrashort (~ fsec)electron bunchesILC will deliver e- bunches of 1 psec min
Applications of ~ fsec science : Ultrafast biological probing for example
1st Session Motivation
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Conclusion: Current acceleration techniques havetwo main limits :
1.an upper limit on the accelerating gradient
2.a lower limit the pulse length.
Any new method that can improve any of thesefeatures will open up new possibilities in both highenergy, biomedical physics and many otherapplications.
1st Session Motivation
Possible solution for the future:
THE LASER PLASMA WAKEFIELD
ACCELARATOR (LWFA)
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1st Session The LWFA
The Laser WakefieldThe Laser Wakefield
AcceleratorAccelerator1979 Tajima and Dawson
Same way a boat excites sea wakes
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1st Session Basic EM theory equations *
1
o
S E H E B
= =
ur ur uur ur ur
The Poynting vector represents the energy flux of an EM wave
( ) ( )2
20 0
1 / 377 / peak values
o
I S E E V cm I W cmc
= = =
ur ur
and its amplitude the intensity (W/cm2) of the wave
* Most of the basic theory of laser plasma interactions can be found in E. Clarks talk
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1st Session Physics of the LWFA :
Ionisation by an intense laser pulse
Keld > 1 multiphoton ion.
3 distinct processes :depending on the strength of the external laser field,
for a given atomic state and governed by the Keldysh parameter
Keld < 1 tunneling ion. Keld
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1st Session Physics of the LWFA :
Particle motion under a laser field
Laser field equations
Lorentz force
But first, again some basic equations :
For a single electron, the electric and magnetic fieldcan be expressed in terms of the vector potential as
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1st Session Physics of the LWFA :
Particle motion under a laser field
By replacing in the Lorentz equation we obtain the
equations of motion of our test particle (electron)
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1st Session Physics of the LWFA :
Particle motion under a laser field
where
and is the normalised vector potential
The first term in the longitudinal equation of motion denotes a
gradual, linear drift with time
in useful experimental units,0 in m, I in 1018W/cm2
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Thus, if we transform in frame
moving with velocity
we obtain the famousfigure of 8 motion
1st Session Physics of the LWFA :
Particle motion under a laser field
2
0
4
a c
Laboratory frame
2 oscillation
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1st Session Physics of the LWFA :
Ponderomotive force
Total energy of a relativistic particle
Kinetic energy gained
Averaged kinetic energy (Ponderomotive potential of the field)
of a relativistic particle over a field oscillation period 2/
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1st Session Physics of the LWFA :
Ponderomotive force
And since there is there is net energy gain when
the laser is off, the Ponderomotive potential is related to the Ponderomotive force by
As we will see immediately, the Ponderomotive
force is the responsible force behind the creation ofthe plasma waves, which possess electric fields
with ideal accelerating properties.
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1st Session Physics of the LWFA :
Plasma waves Plasma frequency
When many electrons are present, collectivebehaviour is exhibited
x
x
Static positive (ion)background -ALWAYS
Mobile electrons
Surface charge density
Capacitor-like E-field
Equation of motion
Simple harmonic
oscillation
Oscillation freq.
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1st Session Physics of the LWFA :
Plasma waves Excitation of linear plasma waves
When a plane EM wave travels in free space is characterised by the
dispersion relation =ck, where c=1/(00)1/2
and k=2/For a medium/plasma with and , however the dispersion relation is altered
Assume an infinite and low intensity (i.e. collisions and magnetic effects are neglected) EM wave
The equation of motion of a test free electron within the plasma will be
with
By performing some mathematical manipulations,i.e. integrate the equation of motion over time and solve for velocity,
we can generate expression for current Je
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1st Session Physics of the LWFA :
Plasma waves Excitation of linear plasma waves
1. Propagation of the mode isperpendicular to the initial field E-
oscillation,mode is EM in nature
2. Propagation of the mode is parallel
to the initial field E-oscillation,mode is electrostatic in nature
We can identify two oscillatory excited modesfrom the propagation of the EM wave within the medium/plasma
Exercise : Derive the current Je, use the curl of Faradays law (for EM and E-stat), use
Ampere-Maxwell equation (for EM only) to derive the dispersion relations of the new modes
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1st Session Physics of the LWFA :
Plasma waves Generation of non-linear pw
To estimate how much and in what way a particular EM pulse(having finite durationrather than an infinite wave as before)ofarbitrary strengthwill affect the behaviour of the plasma wave
we will have to express some fundamental quantities such as the
plasma density variation(i.e. oscillation) neandthe electrostatic potential created by this variationin terms of our EM pulse primary quantity,
which is the normalized vector potential = eA/mc2.
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1st Session Physics of the LWFA :
Plasma waves Generation of non-linear pw
Lets assume an EM pulse (of finite duration),
linearly polarised, described by the vector potentialy : oscillation axis
x : propagation axis
Medium : cold, collisionless plasma
Density perturbations n=ne-n0 Electrostatic potential
New expressions for the electric and magnetic fieldsto be used in the Lorentz equation
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1st Session Physics of the LWFA :
Plasma waves Generation of non-linear pw
Equations of motion*
*These equations contain the momentum components px, py,which explicitly introduces the relativistic factor
Normalisations :
Coupling factor
Coulomb gauge,
assuming charge plasma fluid motionaffects instantly
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1st Session Physics of the LWFA :
Plasma waves Generation of non-linear pw
Vector field wave equation,
by replacing Eand Bin Amperes law
Continuity equation(since we are treating
our medium as fluid)
Poisson equation,only in terms of,
due to Coulomb gauge
The longitudinal eq. of motionRelates a fluid quantities (, )
with a field quantity
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1st Session Physics of the LWFA :
Plasma waves Generation of non-linear pw
The previous four equations provide a system where the importantparameters of the plasma wakefield are coupled with the strength
parameter of the EM pulse, albeit in a non easily solvable form
For simplification, we transform in
a frame moving at the groupvelocity of the EM pusle
New coordinatesin comoving frame
Also, assume that EM pulseevolution is negligible compared toplasma frequency, i.e. Quasi-Static
Approximation (QSA)
Thus, any time derivativeis neglected
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1st Session Physics of the LWFA :
Plasma waves Generation of non-linear pw
The four coupled equations can berewritten in the new coordinate
system
The second equation has a very important implication for plasmadensity evolution : when the velocity of the fluid reaches the groupvelocity of the EM pulse (i.e. ->g)
then the plasma density reaches infinity (ne->),black hole formation - impossible
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1st Session Physics of the LWFA :
Plasma waves Generation of non-linear pw
To cut a very long story short, we rearrange the above relations,
and we associate the plasma fluid velocity , and density ntothe electrostatic potential and vector potential , which whenreplaced in Poissons equation give in the new coordinate frame*
*All quantities are still normalised
which is a 2nd
order nonlinear ordinary differential equation for theelectrostatic potential , created by the density variation (n = ne/n0),created by the EM pulse =0()in the QSA and
can be solved numerically.
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1st Session Physics of the LWFA :
Plasma waves Generation of non-linear pw
Physical 1D system : EM pulse, =1m, pulse=100 fsec,
Plasma, n0=1018 cm-3 (p=30m) (i.e. cpulse ~ p)
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1st Session Physics of the LWFA :
Plasma waves Generation of non-linear pw
Important notes : in the Non Linear case, we observe plasma wavelength increase due to relativistic
effects (p->p1/2)
plasma density profile steepening
plasma wake electric field sawtoothing
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1st Session Physics of the LWFA :
Plasma waves Relativistic pw wavebreaking (wb)
Lets remember the second of the final coupled equations
What happens when ->g???
Same thing to a surfer riding a sea wave
Smooth/slow wave steepening,
good ride
Harsh/fast wave steepening,
bad ride
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1st Session Physics of the LWFA :
Plasma waves Relativistic pw wavebreaking (wb)
The mathematical formulation for wavebreaking is rathercomplicated but it suffices to give the final expression of
the natural limiton the electrostatic fields supported by aplasma wave before the wave structure collapses
Cold RelativisticWaveBreaking field
Cold Non-RelativisticWaveBreaking field
Practical units Emax,limit~0.96(ne)1/2,
i.e. ne~1020 cm-3 ->
Emax,limit~10 GV/cm
Laser field factor,equal to 1 when laser is off
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1st Session Physics of the LWFA :
Plasma waves Relativistic pw wb Self-injection
1D Plasma density profile steepening
Adapted from Nature, 431, 515 (2004)
The natural process of driving a non-linear plasma wave towavebreaking acts as automatic electron injector in the
accelerating parts of the plasma wake electric fields
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1st Session Physics of the LWFA :
Plasma waves Relativistic pw wavebreaking (wb)
3D Plasma density profile steepening trajectory crossing /3D Wavebreaking Bubble regime
(identified in Pukhov, A. & Meyer-ter-Vehn, J. Laser wake field acceleration: the highlynon-linear broken-wave regime. Appl. Phys. B 74, 355361 (2002))
Electron density void /
Ion surplass / Plasma bubbleElectron trajectories
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1st Session Physics of the LWFA :
Plasma waves Energy gain of accelerated e-
Natural limitation on acceleration distance *remember the plasma wake electric field points at
the centre of the plasma period/plasma bubble
The dephasing length : the maximum length thatan electron injected at the back of the plasma wake period
will travel before it starts to decelerate due to theelectrostatic fields of the front half of the plasma wake
In the comoving frame (ug),is equal to a length of half
the plasma wavelength p/2
In the laboratory frame,
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1st Session Physics of the LWFA :
Plasma waves Energy gain of accelerated e-
Energy gain in the comoving frame (the wave frame)
By performing a Lorentz transformationon the electron momentum four-vector
Energy gain in the laboratory frame
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1st Session Physics of the LWFA :
Plasma waves Energy losses in Wake generation
Simplistic model : EM energy contained in laser pulseequals E-static energy contained in the plasma wake
Laser EM energy Plasma wake E-static energy
Optimum length for asquare pulse to maximiseplasma wakes amplitude
Valid approximation for allinitial driver laser pulseshape (i.e. sine, square,
guassian)
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1st Session Physics of the LWFA :
Plasma waves Energy losses in Wake generation
Depletion length(for a square pulse)
Dephasing length
Small laser amplitudes
The interaction isdephasing limited
Large laser amplitudes
The interaction isdepletion limited
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1st Session Physics of the LWFA :
Plasma waves Energy losses in Wake generation
Third physical limitation length on the Laser Plasma Interaction
Natural defocusing - Rayleigh length :defined as the length were the cross section of the laser
pulse is doubled (or in simpler terms stays in focus)
Physical example :a laser pulse of=1 m, focused at a
focal spot of w0=20 m, with an achieved0=1, in a plasma with ne=5*10
18 cm-3
ZR= 1.2 mmLd = 2.98 mmLdp = 3.03 mm
Conclusion : WE NEED TO OVERCOME NATURALDEFOCUSING AND EXTEND THE INTERACTION LENGTH
2nd
SESSION
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1st Session Summary of LWFA
1. The ponderomotive force of a laser pulse excites plasma waves
2. Depending on the strength of the laser pulse, a bubble structurecan form withperfect Efield geometry for electron acceleration,i.e. both acceleratingand focusingkeeping a low energy spreadand emittance. This non-linear structure can break, leading to
self-injection of electrons in th`e accelerating parts of thewake
3. Beam loading end of injection, where the electrostatic field ofthe injected electrons cancels the accelerating field of the wake.
4. Dephasing the injected electron beam enters thedecelerating phase of the wake.
LWFA is a 4 step process
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1st Session Physics of the LWFA :
Plasma waves Relativistic pw wb Self-injection
1D Plasma density profile steepening
Adapted from Nature, 431, 515 (2004)
The natural process of driving a non-linear plasma wave towavebreaking acts as automatic electron injector in the
accelerating parts of the plasma wake electric fields
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1st Session Bibliography
E. Esarey, P. Sprangle, J. Krall, and A. Ting,Overview of plasma-based accelerator concepts
IEEE Transactions on Plasma Science 24, 252 (1996)
Paul Gibbon,Short Pulse Laser Interaction with Matter
Imperial College Press, 2005
W. B. Mori,The physics of the nonlinear optics of plasmas atrelativistic intensities for short-pulse lasersIEEE Journal of Quantum Electronics 33, 1942 (1997)
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2nd Session In brief
We will show how we can extend the propagation of alaser pulse beyond the naturally limiting length ofZR , by
exploiting various non-linear phenomena that inevitablyoccur
We will show results from recent experiments + somesimulation movies, visualising in real time what is reallyhappening
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2nd Session Propagation in underdense plasmas :
Non Linearities Refractive index modulations
A plasma is a medium with electric permittivity
and magnetic permeability , different thanthe vacuum equivalents 0, 0
Index of refraction is defined as
The phase velocity of a propagating EM wave is*
*Remember from dispersion relation
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2nd Session Propagation in underdense plasmas :
Non Linearities Refractive index modulations
With appropriate substitutions
Group velocityof EM wavePhase velocityof EM wave
Dependence ofon plasma density (ne), laserfrequency (0), laser intensity (0-as relativisticeffects effectively increase the critical density ncr)
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2nd Session Propagation in underdense plasmas :
Non Linearities Refractive index modulations
Thus can be expanded to first order accordingly
Modulations in these three parameters (ne, 0, 0) lead
to modulation of the index of refraction which in turnleads to modulation ofphand grof the EM pulse
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Physical system : A laser pulse (e.g. gaussian)
enters a homogeneous density plasma region ->Transverse intensity profile induces ponderomotive
radial expulsion of electrons ->
Transverse index of refraction modulationOr respectively transverse modulation in ph
2nd Session Propagation in underdense plasmas :
Non Linearities Refractive index modulations
Induced phenomenon : Self-focusing
Self-focusingacceleration
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Physical system : A laser pulse (e.g. gaussian) has
longitudinal intensity variation (0) ->Longitudinal variation plasma density will inducelongitudinal variation in index of refraction ->
Longitudinal variation in gr
2nd Session Propagation in underdense plasmas :
Non Linearities Refractive index modulations
Induced phenomenon : Self-compression
Self-compression rate (incomoving frame , )
d
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2nd Session Propagation in underdense plasmas :
Non Linearities Refractive index modulations
Induced phenomenon : Self-compression
Image courtesy of A.G.R. Thomas
2 d S i P i i d d l
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2nd Session Propagation in underdense plasmas :
Non Linearities Refractive index modulations
Physical system : A laser pulse (e.g. gaussian) has
longitudinal intensity variation (0) ->Longitudinal variation plasma density will inducelongitudinal variation in index of refraction ->
Longitudinal variation in ph
Induced phenomenon : Photon Acceleration
Frequency change rate (incomoving frame , )
2nd S i P ti i d d l
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2nd Session Propagation in underdense plasmas :
Non Linearities Refractive index modulations
Conclusion: Refractive index gradientsare found in almost all cases of laser
propagation in underdense plasmas, so it is
almost unavoidable not to experience
Self-focusingSelf-compression
Photon acceleration/deceleration
2nd S i P ti i d d l
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2nd Session Propagation in underdense plasmas :
Propagation beyond the Natural Limit (ZR)
If the natural defocusing rate of a laser beam matches the inducedfocusing from any non-linear phenomena (i.e. self-focusing fromtransverse density gradients) then the laser pulse fronts will stay
focused and propagate for an extended length
Natural Defocusing Limit = Rayleigh range ZR=w02/
Adapted from http://upload.wikimedia.org/wikipedia/commons/9/94/Gaussianbeam.png
Typical experimental valuesw0=10 m, =1m ->
ZR=0.3mm
w0=1/e2 intensity radius
2nd Session Propagation in underdense plasmas :
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If the natural defocusing rate of a laser beam matches the inducedfocusing from any non-linear phenomena (i.e. self-focusing from
transverse density gradients) then the laser pulse fronts will stayfocused and propagate for an extended length
2nd Session Propagation in underdense plasmas :
Propagation beyond the Natural Limit (ZR)
2nd Session Propagation in underdense plasmas :
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2nd Session Propagation in underdense plasmas :
Propagation beyond the Natural Limit (ZR)
Two ways to induce a transverse density gradient(i.e. transverse index of refraction gradient)
I) Externally, for example with the use of the so-called gas filled discharge discharge capillaries
II) Internally, i.e. by allowing the laser pulse to self-evolve, see Self-focusing section, due to theunavoidable electron expulsion from axis due to the
radial ponderomotive force of the laser pulse
2nd Session Propagation in underdense plasmas :
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2nd Session Propagation in underdense plasmas :
Propagation beyond ZR External guiding
Transverse parabolicplasma profile
Gas filled discharge discharge capillaries =Hollow tubes of 100s m diameter, filled with gas (i.e. hydrogen)
where an electrical pulse of 100s A and 10s kVpasses, ionises and hydrodynamically expands the plasma
Transverse inverse parabolicindex of refraction
Maximum achieved guidingup to 50 mm
2nd Session Propagation in underdense plasmas :
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2nd Session Propagation in underdense plasmas :
Propagation beyond ZR External guiding
By matching the natural
defocusing rate
By matching the self-focusingacceleration (see Self-focusing
section)
We can derive a matched spotsize, where diffraction is balancedby self-focusing effects due to the
density (refractive index)
transverse gradients
2nd Session Propagation in underdense plasmas :
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2 d Session Propagation in underdense plasmas :
Propagation beyond ZR Relativistic guiding
Respectively, the relativistically corrected index ofrefraction (due to relativistic mass increase) will be
Assume a laser pulse in the mildly relativisticregime, i.e. 0
2
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And since
2 Session Propagation in underdense plasmas :
Propagation beyond ZR Relativistic guiding
Index of refraction profile similar to externally guiding case
Thus by replacing this index of refraction expression in the self-focusing acceleration equation and equate with the natural
diffraction rate (as we did before) we can derive the matched
spot size for relativistic self-guiding
2nd Session Propagation in underdense plasmas :
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2 Session Propagation in underdense plasmas :
Propagation beyond ZR Relativistic guiding
By replacing 0 with
We can derive a critical value for the power of the laserpulse, so that relativistic self-focusing is induced
(!!!) (!!!)
Major Limitation : For relativistic self-guiding to occurthe laser pulse must cover many plasma periods (pe) so
that there is time for self-focusing to evolve
2nd Session Propagation in underdense plasmas :
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2 Session Propagation in underdense plasmas :
Propagation beyond ZR Relativistic guiding
Longestself-guiding channels observed so far: 10.1 mm
Laser pulse : 25J, 500fsec, 50TW, w0=25mm -> Z
R=1.8mm,
0~ 2
2nd Session Propagation in underdense plasmas :
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2 Session Propagation in underdense plasmas :
Summary
So far we have seen that any laser pulse propagating through ahomogeneous plasma density region will be affect by non-linear
phenomena such asself-focusing, self-compression, photon acceleration
Simply put, a pulse of initial strength 0will self-evolve during propagation in
0>
0
Given that the laser pulse is long enough (i.e. claser>>plasma)
Relativistic increase of electron mass leads to transverse density profile,ideal for self-focusing and hence self-guiding over many ZR
2nd Session Schemes of laser driven plasma based
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p
accelerators - LWFA
Typical Experimental values
Laser : 40fsec, 500mJ
w0 : 40m 5 m
I : 3*1017 3*1019 W/cm2
0 : 0.4 3.5
Plasma Density : ne ~ 5*1018 cm-3
Plasma length : Lplasma ~ 3 mm
Single pulse excites plasma waves, which when driven to highamplitudes, wave break, inject electronsin the accelerating phaseson the wake, thus leading toMono-Energeticelectron beams
2nd Session Schemes of laser driven plasma based
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Image courtesy of A.G.R. Thomas
p
accelerators Self Modulated LWFABy utilising the Forward Raman instability, we create a beat pattern that
resonantly can drive a plasma wake to breaking conditions.From that point on it behaves as a usual LWFA
2nd Session Schemes of laser driven plasma based
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p
accelerators SM LWFA Parametric instabilities
The plasma waves grow at the expense of the incoming EMwave, which is called the pump
Parametric instabilities occur only when their growth rate is fasterthan the characteristic evolution of the system, usually determinedby the duration of the EM pulse, i.e. short (
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1. The pump EM field causes the electrons of the plasma to oscillate at
pe
2. Pump photons are scattered from these density oscillations, atfrequencies equal to the sum and difference of the pump frequency
and plasma frequency (pmpe)
3. The interference between the pump and scattered beam causes avariation at the beat frequency (pe) in the overall EM pressure
4. These variations resonantly excite electron density fluctuations, whichin return generate more scattered photons at (pmpe), which beatwith pump photons and so on
Feedback Loop
accelerators SM LWFA Parametric instabilities
2nd Session Schemes of laser driven plasma based
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The Stimulated Raman Scattering (SRS)is the decay of an
incoming photon (pump laser) into another photon (eitherblueshifted or downshifted) and a plasmon
The emitted photon can be either:
co-propagating with the pump beam (Forward Raman Scattering)
counter-propagating (Raman Back Scattering)
can be scattered in any in between angle (Raman Side Scattering)
accelerators SM LWFA Parametric instabilities
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Matching conditions for the feedback loop to grow
Image courtesy of A.G.R. Thomas
accelerators SM LWFA Parametric instabilities
2nd Session Experiments performed Multi-TW
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table top laser systems Recent historical landmarks
First high energy SM-LWFA experiment
Until 2002 all the experimentalresults on electron accelerationsuffered from a large energy
spread, an inherent feature of theSM-LWFA mechanism as it involves
randomised wavebreaking of manyplasma periods
The bubble regime has been identified in 2002 and was madeaccessible only recently with the T3 laser systems that could inducewavebreaking conditions with laser pulses of a few plasma periods
long (i.e. claser
~ plasma
)
Modena, Nature, 377, (1995)
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table top laser systems Recent historical landmarks
First Mono-Energetic LWFA experiments
But in 2004 Nature, 431,3 seminal papers werepublished
The set-up was similar in allexperiments
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Mangles et al,Imperial College, UK:
70 MeV beam
Geddes et al,Lawrence Berkeley, USA:
85 MeV beam
Faure et al,LOA, France:
170 MeV beam
All images taken from Nature, 431
table top laser systems Recent historical landmarks
First Mono-Energetic LWFA experiments
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table top laser systems Recent historical landmarks
First Mono-Energetic GeV experiment
Leemans et al,
Lawrence Berkeley, USA:
1000 MeV beam
Image taken from Leemans et al., Nature Physics, 2 (2006)
Long interaction length, i.e.
33 mm, via guiding through a
Hydrogen filled, discharge
capillary
Note : Maximum electron
acceleration ~ 100 GeV in
km long linear accelerators
2nd Session Experiments performed Multi-TWtable top laser systems Simulations
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table top laser systems Simulations
The code used for the simulations is a 2D Particle-In-Cell, called OSIRIS
Physical system :
Laser - 1J, 30fsec, =800nm, w0=10m, 0=1.79
Plasma -ne=9*1018
cm-3
, Lplasma=10 mm
1st Simulation : Propagation of ultrashort (claser~plasma)
laser pulse in homogeneous underdense plasma - LWFA
Main results :
1. slow evolution(i.e. self-focusingand self-compressionto higher laseramplitudes)
2. stable >250MeV electron beamthat outruns the laser pulse
3. maintaining its Mono-Energetic/low energy spreadfeature
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table top laser systems Simulations
Physical system :Laser 100J, 400fsec, =1054nm, w0=25m, 0=4.3
Plasma -ne=2*1018 cm-3, Lplasma=20 mm
Main results :
1. slow evolution(i.e. self-focusingand self-compressionto higher laseramplitudes) leads to complete pulse break
2. laser pulse is slowly matched to an ideal LWF Accelerator
3. Emax>GeV, >plasma)laser pulse in homogeneous underdense plasma SM-LWFA
2nd Session Conclusions
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The need for new particle acceleration techniques is obligatory,if we want to explore new realms of physics.
However, as more is not always the best, new particleacceleration techniques on a lower energy range (100-1000 MeV)can downsize and reduce the cost of an acceleration machine for
commercial purposes as well
Laser Wakefield Accleration,since 2004 when it wasfirst demonstrated, has drawn the attention (and the
funding) of 100s of research groups all over the world.
However, the reproducibility, stability, emittanceandchargeof the beams produced from LWFA are still one
order of magnitude worse than conventional accelerators.
2nd Session Conclusions : Exotic new research
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Control of electron self-injection Multiple laser beams
Image courtesy of A.G.R. Thomas
The ponderomotive force of a second laser beam (co-,counter- or cross-propagating) can dephase wake electrons and inject them in the wake.
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Control of electron self-injection External Impurities
Al5+->Al6+
IBSI =1.4e17 W/cm2
O5+->O6+
IBSI =4e16 W/cm2
Al9+->Al10+
IBSI =1e18 W/cm2
2nd Session Conclusions : Exotic applications
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Towards a table-top free-electron laserConventional bright x-ray source
180m
Downsized novel x-ray source
How x-rays are produced ???
The applications of suchsynchronised electron/x-ray beams
are numerous. From ultrafastbiomedical (molecular/atomic)imaging, to lithography for the
computer and automotive industry
2nd Session Conclusions : Proton/Ionacceleration applications
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acceleration applications
Main acceleration of protons/ions comes from electron sheathspropagating through and away from the surface of a thin metallictarget hit by a laser pulses similar to those described in this talk
Main applications ofthese protons/ionsCancertreatm
ent
FastIgnitor
(Tatarakis
talkonHiP
ER)
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Thank you for your timeand presence !!!
CollaboratorsRCUK - Basic Technology Grant AlphaX
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A.G.R. Thomas, S.P.D. Mangles, L. Willingale, C. Bellei, S. Kneip, S. Nagel,K. Krushelnick, Z. Najmudin
Plasma Physics Group, Imperial College London, UK
C.D. Murphy, K. Lancaster, P.S. Foster, C.J. Hooker, E.J. Divall,O. Cheklov, P. Norreys, J. Collier
CCLRC Rutherford Appleton Laboratory, UK
J.G. Gallacher, E. Brunetti, M. Wiggins, F. Bode, D.A. Jaroszynski
University of Strathclyde, UK
T.P. Rowlands-Rees, Tom Ibbotson, A.J. Gonslaves, S.M. Hooker
Clarendon Laboratory, University of Oxford, UK
RCUK Basic Technology Grant AlphaX