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Laser applications for accelerators
Laser Basics
Yuelin LiAccelerator Systems DivisionArgonne National [email protected]
USPAS 2008 Summer Session, Annapolis, June 23-27, 2008
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2USPAS, 2008
ContentLaser and accelerator historyMap of laser application in acceleratorsLaser basics– Rate equations– Laser configurations– Gaussian beam optics and ABCD law– Laser cavity and laser modes
Laser configurations– Mode-lokcing and q-switch– MOPA – CPA and dispersion
Laser materials Other lasers– Semiconductor lasers– Fiber lasers
Frequency conversion and short wavelength lasers
![Page 3: Laser Basics - USPASuspas.fnal.gov/materials/08UMD/Lecture1.pdfLaser applications for accelerators Laser Basics Yuelin Li Accelerator Systems Division Argonne National Laboratory ylli@aps.anl.gov](https://reader035.vdocuments.site/reader035/viewer/2022070813/5f0c5a037e708231d434f912/html5/thumbnails/3.jpg)
3USPAS, 2008
ContentLaser and accelerator historyMap of laser application in acceleratorsLaser basics– Rate equations– Laser configurations– Gaussian beam optics and ABCD law– Laser cavity and laser modes
Laser configurations– Mode-lokcing and q-switch– MOPA – CPA and dispersion
Laser materials Other lasers– Semiconductor lasers– Fiber lasers
Frequency conversion and short wavelength lasers
![Page 4: Laser Basics - USPASuspas.fnal.gov/materials/08UMD/Lecture1.pdfLaser applications for accelerators Laser Basics Yuelin Li Accelerator Systems Division Argonne National Laboratory ylli@aps.anl.gov](https://reader035.vdocuments.site/reader035/viewer/2022070813/5f0c5a037e708231d434f912/html5/thumbnails/4.jpg)
4USPAS, 2008
Lasers and accelerators at birth
Ancient: Let there be light…………………..1917, theory of stimulated
radiation by Einstein1960, flash-lamp pumped
ruby, Dr. Mainman1964, Nobel Prize, Towne,
Basov, and Prokhorov
Ancient: a cave man’s bow……………….1929, Cyclotron, Lawrence1939, Nobel Prize, Lawrence
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5USPAS, 2008
Today’s lasers and acceleratorsAiming for higher energy/intensity and better control
APS, ANL
(Panofsky, http://www.slac.stanford.edu/pubs/beamline) (http://www.eecs.umich.edu/CUOS)
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6USPAS, 2008
Newest developments
Accelerator-generated lasers: a free-electron laser
Laser as an accelerator: a compact accelerator
Geddes et. al., Phys Plasmas 12, 056709 (2005)
Laser plasma bubble
Laser
Gas jet
Electron beam
-0.4 0.0 0.4268
266
264
τ (ps)
FEL FROG trace
S.P.D. Mangles et al. Nature 431, 535 (2004); C.G.R. Geddes et al. Nature 431, 538 (2004); J. Faure et al. Nature 431, 541 (2004)
Credit: Becker et al, LMU
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7USPAS, 2008
ContentLaser and accelerator historyMap of laser application in acceleratorsLaser basics– Rate equations– Laser configurations– Gaussian beam optics and ABCD law– Laser cavity and laser modes
Laser configurations– Mode-lokcing and q-switch– MOPA – CPA and dispersion
Laser materials Other lasers– Semiconductor lasers– Fiber lasers
Frequency conversion and short wavelength lasers
![Page 8: Laser Basics - USPASuspas.fnal.gov/materials/08UMD/Lecture1.pdfLaser applications for accelerators Laser Basics Yuelin Li Accelerator Systems Division Argonne National Laboratory ylli@aps.anl.gov](https://reader035.vdocuments.site/reader035/viewer/2022070813/5f0c5a037e708231d434f912/html5/thumbnails/8.jpg)
8USPAS, 2008
A map for laser applications in accelerators
Beam generation
Beam Characterizationmonitoring
BeamProcessing treatment
Radiation/particle source generation
• Laser/accelerator synchronization• Laser pulse shaping• Plasma wake wave accelerator
• Laser beam cooling/heating• Laser modulation
• Laser beam scattering• Electroptical sampling • Inverse free-electron laser
• Laser beam scattering• Laser beam timing • Laser modulation
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9USPAS, 2008
ContentLaser and accelerator historyMap of laser application in acceleratorsLaser basics– Rate equations– Laser configurations– Gaussian beam optics and ABCD law– Laser cavity and laser modes
Laser configurations– Mode-locking and Q-switch– MOPA – CPA and dispersion
Laser materials Other lasers– Semiconductor lasers– Fiber lasers
Frequency conversion and short wavelength lasers
![Page 10: Laser Basics - USPASuspas.fnal.gov/materials/08UMD/Lecture1.pdfLaser applications for accelerators Laser Basics Yuelin Li Accelerator Systems Division Argonne National Laboratory ylli@aps.anl.gov](https://reader035.vdocuments.site/reader035/viewer/2022070813/5f0c5a037e708231d434f912/html5/thumbnails/10.jpg)
10USPAS, 2008
Laser
Light Amplification by Stimulated Emission of Radiation
Excited medium
If a medium has many excited molecules, one photon can become many.
This is the essence of the laser. The factor by which an input beam is amplified by a medium is called the gain and is represented by G.
Credit: R. Trebino
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11USPAS, 2008
Rate equations for a two-level system
Rate equations for the densities of the two states:
21 2 2( )dN BI N N AN
dt= − −
12 1 2( )dN BI N N AN
dt= − +
22 2d N BI N ANdtΔ
= − Δ +
Absorption Stimulated emission Spontaneous emission
1 2N N NΔ ≡ −1 2N N N≡ +
If the total number of molecules is N:
2 1 2 1 22 ( ) ( )N N N N NN N
= + − −= −Δ
2d N BI N AN A NdtΔ
= − Δ + − Δ⇒
⇒
2
1
N2
N1
LaserPump
Pump intensity
Credit: R. Trebino
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12USPAS, 2008
Why inversion is impossible in a two-level system
0 2BI N AN A N= − Δ + − Δ
1 / sat
NNI I
Δ =+
/ 2satI A B=
In steady-state:
( 2 )A BI N AN⇒ + Δ =
where:
ΔN is always positive, no matter how high I is!
It’s impossible to achieve an inversion in a two-level system!
⇒
2d N BI N AN A NdtΔ
= − Δ + − Δ
/( 2 )N AN A BI⇒Δ = +
/(1 2 / )N N BI A⇒Δ = +
Isat is the saturation intensity.
2
1
N2
N1
Laser
Credit: R. Trebino
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13USPAS, 2008
A 3-level system
Assume we pump to a state 3 that rapidly decays to level 2.
21 2
dN BIN ANdt
= −
11 2
dN BIN ANdt
= − +
1 22 2d N BIN ANdtΔ
= − +
Absorption
Spontaneous emission
1 2N N NΔ ≡ −1 2N N N≡ +
The total number of molecules is N:
22N N N= −Δ
d N BIN BI N AN A NdtΔ
= − − Δ + − Δ⇒
Fast decay
Laser TransitionRate: A
PumpTransition
Rate: BI
1
23
Level 3 decays fast and so is zero.
12N N N= + Δ
Credit: R. Trebino
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14USPAS, 2008
Population inversion, 3 level system
1 /1 /
sat
sat
I IN NI I
−Δ =
+/satI A B=
In steady-state:
( ) ( )A BI N A BI N⇒ + Δ = −
where:
Now if I > Isat, ΔN is negative!
⇒
( ) /( )N N A BI A BI⇒Δ = − +
Isat is the saturation intensity.
d N BIN BI N AN A NdtΔ
= − − Δ + − Δ
0 BIN BI N AN A N= − − Δ + − Δ
Fast decay
Laser TransitionRate: A
PumpTransition
Rate: BI
1
23
Gain: Ng Δ−∝ σ Credit: R. Trebino
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15USPAS, 2008
Rate equations for a four-level system
Now assume the lower laser level 1 also rapidly decays to a ground level 0.
20 2
dN BIN ANdt
= −
1 0,N ≈
22 2( )dN BI N N AN
dt= − −
2N NΔ ≈ −
Laser Transition
Pump Transition
Fast decay
Fast decay
1
2
3
0As before:
Because0 2N N N≡ +
The total number of molecules is N :
0 2N N N= −d N BIN BI N A N
dtΔ
− = + Δ + Δ
At steady state: 0 BIN BI N A N= + Δ + Δ Credit: R. Trebino
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16USPAS, 2008
Population inversion in a four-level system (cont’d)
0 BIN BI N A N= + Δ + Δ
/1 /
sat
sat
I IN NI I
Δ = −+
/satI A B=where:Isat is the saturation intensity.
Now, ΔN is negative—always!
Laser Transition
Pump Transition
Fast decay
Fast decay
1
2
3
0
⇒
( / ) /(1 / )N BIN A BI AΔ = − +⇒
/( )N BIN A BIΔ = − +⇒
( )A BI N BIN+ Δ = −⇒
Credit: R. Trebino
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17USPAS, 2008
How to build a laser
R = 100% R < 100%
I0 I1
I2I3 Laser medium
I
• Laser medium• Depends on wavelength, pulse duration, power
• Pump it: ASE• Multimode in time and space
• Add resonator: laser oscillation• Mode selection
Credit: R. Trebino
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18USPAS, 2008
The historic ruby laser
Invented in 1960 by Ted Maimanat Hughes Research Labs, it was the first laser.
Ruby is a three-level system, so you have to hit it hard.
Credit: R. Trebino
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19USPAS, 2008
Helmholtz Equation: Gaussian beam optics
)(
2
2
2
22
),,(),,,(
0),,,(
tzki zezyxAtzyxE
tzyxEtc
n
ω−=
=⎟⎟⎠
⎞⎜⎜⎝
⎛∂∂
−∇
02 2
222
2
2
2
2
2
2
=+∂∂
+−⎟⎟⎠
⎞⎜⎜⎝
⎛∂∂
+∂∂
+∂∂ A
cnA
zkiAkA
zxx zzω
Wave equation
Paraxial condition
λπω 2, 2
222
2
2
nc
nkAz
Az z ==
∂∂
<<∂∂
Paraxial Helmholtz equation
022
2
2
2
=∂∂
+⎟⎟⎠
⎞⎜⎜⎝
⎛∂∂
+∂∂ A
zkiA
yx z
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20USPAS, 2008
Gaussian beam optics
022
2
2
2
=∂∂
+⎟⎟⎠
⎞⎜⎜⎝
⎛∂∂
+∂∂ A
zkiA
yx z
yxykxki
yx
ykxkiyx
dkdkezkkazyxA
dxdyezyxAzkka
yx
yx
)(2
)(
),,(4
1),,(
),,(),,(
+
+−
∫∫
∫∫=→
=
π
Fourier transform
Thus ( )
zkkk
i
yxyx
z
yx
yxykxki
zyx
z
yx
yx
ekkazkka
akkk
iaz
dkdkeaz
kiakk
20
22
)(222
22
)0,,(),,(
2
024
1
+−
+
=→
+−=
∂∂
→
=⎥⎦⎤
⎢⎣⎡
∂∂
+−−∫∫π
Paraxial Helmholtz equation
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21USPAS, 2008
Gaussian beam optics
.)0,,(20
2
20
22
00wr
wyx
eAeAyxA−
+−
==
20
22
20
22
40
20
)(0)0,,(
wkk
yxykxkiw
yx
yx
yx
yx
eAw
dkdkeeAkka+
−
+−+
−
=
= ∫∫
π
Fourier transform
Thus
( ) ⎟⎟⎠
⎞⎜⎜⎝
⎛++−
+−+
−
+−
=
=
=
0
2220
2220
22
22
14
020
240
20
20 )0,,(),,(
zzikkw
zkkk
iwkk
zkkk
i
yxyx
yx
z
yxyx
z
yx
eAw
eeAw
ekkazkka
π
π
Let
λπ
20
20
0 2wwkz z ==Rayleigh length (diffraction length)
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22USPAS, 2008
Gaussian beam optics
( )
( ) ( )
ηη
π
ππ
π
izRyxik
zwyxi
zzi
zwyx
zzi
zwyx
zzi
zizwyx
yxykxkikk
zizw
yxykxkiz
zikkw
yxykxki
yx
eezwwAe
zwwA
eezz
Aeziz
A
dkdkeeAw
dkdkeeAw
dkdkezkkazyxA
yxyx
yxyx
yx
−++
−−⎟⎟⎠
⎞⎜⎜⎝
⎛−
+−
⎟⎟⎠
⎞⎜⎜⎝
⎛−
+−−
++
−
+++
−
+⎟⎟⎠
⎞⎜⎜⎝
⎛++−
+
==
+=
+=
=
=
=
−
∫∫
∫∫
∫∫
)(2)(001
)(00
1)(
tan
20
20)/1(
0
0
)(4/1
0
20
)(1
40
202
)(2
22
2
22
02
22
02
22
0
1
020
22
222
00
0
2220
)()(
/1/1
41
41
),,(4
1),,(
0
12
20
2/1
20
2
0 tan1)(1)(zz
zzzzR
zzwzw −=⎟⎟
⎠
⎞⎜⎜⎝
⎛+=⎟⎟
⎠
⎞⎜⎜⎝
⎛+= η
Inverse Fourier transform
Beam radius
0
1tan
20
2
020
20
/11
1/1
1/1
1
zzi
ezz
zzi
zzziz−−
+=
⎟⎟⎠
⎞⎜⎜⎝
⎛−
+=
+
Wave front radius of curvature
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23USPAS, 2008
Gaussian optics: summary
.2
,2
,
,1)(
,)(
exp)(
),(
0
0
20
0
2
00
2
20
0
zb
w
wz
zzwzw
zwr
zwwEzrE
=Θ
=
=
⎟⎟⎠
⎞⎜⎜⎝
⎛+=
⎟⎟⎠
⎞⎜⎜⎝
⎛−=
πλλπ
w0: beam waistz0: Rayleigh rangeb: confocal parameter
• Gaussian distribution is the solution of paraxial Helmholtz equation• TM00 mode
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24USPAS, 2008
Beam propagation: ABCD matrices
⎟⎟⎠
⎞⎜⎜⎝
⎛⎟⎟⎠
⎞⎜⎜⎝
⎛=⎟⎟
⎠
⎞⎜⎜⎝
⎛θθr
DCBAr
''
For a thin lens
⎟⎟⎠
⎞⎜⎜⎝
⎛−
=⎟⎟⎠
⎞⎜⎜⎝
⎛1/101
fDCBA
For free space (drift space)
⎟⎟⎠
⎞⎜⎜⎝
⎛=⎟⎟
⎠
⎞⎜⎜⎝
⎛10
1 dDCBA
![Page 25: Laser Basics - USPASuspas.fnal.gov/materials/08UMD/Lecture1.pdfLaser applications for accelerators Laser Basics Yuelin Li Accelerator Systems Division Argonne National Laboratory ylli@aps.anl.gov](https://reader035.vdocuments.site/reader035/viewer/2022070813/5f0c5a037e708231d434f912/html5/thumbnails/25.jpg)
25USPAS, 2008
Cavity: Optical resonators
Credit: W. Koechner: Solid State Laser engineering, Credit: Wekipedia
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26USPAS, 2008
Stability of laser resonators
.1
,1
,2110
22
11
21
RLg
RLg
RL
RL
−=
−=
<⎟⎟⎠
⎞⎜⎜⎝
⎛−⎟⎟
⎠
⎞⎜⎜⎝
⎛−<
Credit: W. Koechner: Solid State Laser engineering, Credit: Wekipedia
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27USPAS, 2008
High order modes
K
xxxHxxHxxH
xH
128)(24)(
2)(1)(
33
22
1
0
−=
−=
==
⎥⎦
⎤⎢⎣
⎡++−
+−+
−
⎟⎟⎠
⎞⎜⎜⎝
⎛⎟⎟⎠
⎞⎜⎜⎝
⎛=
)()1()(2)(
2
20
0
22
2
22
)(2
)(2
)(),,(
zmnzRyxki
zwyx
mn eezwyH
zwxH
zwwEzyxE
η
Hermite polynomials
The M2 factor
0
2
2 wM
πλθ =
Θ=
M2=1=diffraction limited; M2 >1, M2 times diffractions limited
![Page 28: Laser Basics - USPASuspas.fnal.gov/materials/08UMD/Lecture1.pdfLaser applications for accelerators Laser Basics Yuelin Li Accelerator Systems Division Argonne National Laboratory ylli@aps.anl.gov](https://reader035.vdocuments.site/reader035/viewer/2022070813/5f0c5a037e708231d434f912/html5/thumbnails/28.jpg)
28USPAS, 2008
High order modes
Hermite-Gaussian modesIntensity profile
Guided modes in fibersField
Encyclopedia of Laser Physics and Technologyhttp://www.rp-photonics.com/higher_order_modes.html
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29USPAS, 2008
A cavity and laser oscillator
Resonant condition for cavity: L=nλ
Energetic electrons in a glow discharge collide with and excite He atoms, which then collide with and transfer the excitation to Ne atoms, an ideal 4-level system.
Credit: R. Trebino
Credit: Cundiff, UCB
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30USPAS, 2008
ContentLaser and accelerator historyMap of laser application in acceleratorsLaser basics– Rate equations– Laser configurations– Gaussian beam optics and ABCD law– Laser cavity and laser modes
Laser configurations– Mode-locking and Q-switch– MOPA – CPA and dispersion
Laser materials Other lasers– Semiconductor lasers– Fiber lasers
Frequency conversion and short wavelength lasers
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31USPAS, 2008
Mode locking: what
Credit: Cundiff, UCB
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32USPAS, 2008
Mode locking: how
Introduce amplitude or phase modulation/control
Active mode locking• Acousto-optic modulator, drive with RF
Passive mode locking • Saturable absorption• Nonlinear lensing + aperture• Nonlinear polarization rotation + polarizer
Mode locking: result
Shorter pulse, high intensity, larger bandwidthSingle modeAccurate timing at round trip time
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33USPAS, 2008
Ti: Sapphire oscillator: an example
Femtolasers: Fusion(28”x12”x3”)
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34USPAS, 2008
Q-switch
LTQ πν 2
=
Q factor of a resonator
T: round trip time; ν: optical frequency; I: fraction power loss per round trip
Q switch: reducing the loss
Active: accousto-optical, electro-optical, and mechanicalPassive: saturable absorbers
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35USPAS, 2008
Compressing,Shaping,
Conversion,diagnosing
filteringstretching, shaping,filtering
A MOPA systemMaster Oscillator – Power Amplifier
An oscillator usually does not have enough energy, thus needs amplificationA MOPA is expected to carry over the characteristics of an OSCPulse duration is limited at 10 ps due to damage
Master Oscillator Pre-amp Power amp Post
processing
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36USPAS, 2008
A MOPA example: Flash drive laser
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37USPAS, 2008
Chirped pulse amplification
To be able to amplify a short pulse.
Oscillator Stretcher Amplifier Regen/multipass + power Compressor
shaping
fs- ps ps - ns fs - ps
ps- ns
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38USPAS, 2008
A CPA example
S. Backus et al, Rev. Sci. Instrum. 69, 1207 (1998).
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39USPAS, 2008
How to stretch/compress a pulse: adding second order phase
A transform-limited Gaussian pulse in the time and frequency domain
⎥⎥⎦
⎤
⎢⎢⎣
⎡⎟⎠⎞
⎜⎝⎛Δ
−=⇔⎥⎥⎦
⎤
⎢⎢⎣
⎡⎟⎠⎞
⎜⎝⎛−=
2
0
2
0 21exp)(
21exp)(
ωωω
τEEtEtE
S. Backus et al, Rev. Sci. Instrum. 69, 1207 (1998).
Add a second order phase, which is to ‘chirp’ a pulse
⎥⎥⎦
⎤
⎢⎢⎣
⎡+⎟
⎠⎞
⎜⎝⎛Δ
−=′ 22
0 21exp)( ω
ωωω iaEE
What is the new pulse form in the time domain? How does the frequency change as function of time? (Home work)
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40USPAS, 2008
Stretcher and compressor
S. Backus et al, Rev. Sci. Instrum. 69, 1207 (1998).
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41USPAS, 2008
Stretcher and compressor
S. Backus et al, Rev. Sci. Instrum. 69, 1207 (1998).
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42USPAS, 2008
Dispersions
S. Backus et al, Rev. Sci. Instrum. 69, 1207 (1998).
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43USPAS, 2008
ContentLaser and accelerator historyMap of laser application in acceleratorsLaser basics– Rate equations– Laser configurations– Gaussian beam optics and ABCD law– Laser cavity and laser modes
Laser configurations– Mode-lokcing and q-switch– MOPA – CPA and dispersion
Laser materials Other lasers– Semiconductor lasers– Fiber lasers
Frequency conversion and short wavelength lasers
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44USPAS, 2008
Laser materials
What we care– Lasing mechanism: four-level systems is always preferred– Lasing wavelength: tunable is better– Lasing bandwidth: bigger is better but not always– Pump requirement: visible preferred– Gain lifetime: longer is better– Damage threshold: higher is better– Saturation flux: higher is better– Heat conductivity: as high as possible– Thermal stability: as small as possible– Form: solid is always preferred
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45USPAS, 2008
Laser materials
Host + active ions Host
– Crystalline solids (Sapphire, Garnets, Fluoride, Aluminate, etc.)• Difficult to grow to large size• Narrow line width thus lower lasing threshold, and narrow absorption
band • Good thermal conductivity
– Glass (property varies by make, and processing)• Easy to make in large size and large quantities• No well defined bonding field thus larger line width and higher lasing
threshold, large absorption band• Lower thermal conductivity thus severe thermal birefringence and
thermal lensing, lower duty cycleActive ions
– Rare earth ions: No. 58-71, most importantly, Nd3+, Er3+…– Transition metals: Ti3+, Cr3+,
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46USPAS, 2008
Laser material: Ti: Saaphire (Al2O3:Ti3+)
• Giving shortest pulse so far• Wonderful tunability• Good thermal properties• Short gain lifetime (has to be
pumped by a ns-pulsed green laser)
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47USPAS, 2008
Laser material (Nd:YAG)
• High saturation flux• Narrow bandwidth (0.15 nm), thus
long pulse (>10 ps), high gain• Good thermal properties• Long gain lifetime (diode pump)
Absorption spectrum
Fluorescent spectrum
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48USPAS, 2008
Laser material: (Nd:Glass)
• High saturation flux• large bandwidth (20 nm), thus short
pulse (<1 ps),• Poor thermal• Long gain lifetime (diode pump)• Only for big lasers now (PW or MJ)
Absorption spectrum
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49USPAS, 2008
Laser Material: Nd:YLF
• High saturation flux• Narrow bandwidth (0.15 nm), thus
long pulse (>10 ps), high gain• Good thermal properties• Long gain lifetime (diode pump)• Difficult to handle
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50USPAS, 2008
Laser materials: summary
-0.57.3dn/dT (10-6/°C)
1.51.551.81.76n
10107.5Thermal expansion coef(10-6/°C)
0.060.00840.140.5Thermal conductivity( w cm-1 K-1)
.434.5 0.60.9Saturation flux(J/cm2)
1.80.46.53Emission cross section (10-19
cm2)
1220.15220 Line width (nm)
1047,105310541064780 Peak wavelength (nm)
4853302303.2Fluorescence life time (μs)
Nd:YLFLiY1.0-xNdxF4
Nd:Glass (Kigre Q-88)
Y3Al5O12:Nd
Nd:YAGY3.0-xNdxAL5O12
Ti:SaAl2O3:Ti
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51USPAS, 2008
ContentLaser and accelerator historyMap of laser application in acceleratorsLaser basics– Rate equations– Laser configurations– Gaussian beam optics and ABCD law– Laser cavity and laser modes
Laser configurations– Mode-lokcing and q-switch– MOPA – CPA and dispersion
Laser materials Other lasers– Semiconductor lasers– Fiber lasers
Frequency conversion and short wavelength lasers
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52USPAS, 2008
Semiconductor laser: laser diode
Credit: http://www.olympusmicro.com/
• Convert current into light, can be tuned by junction temperature• Used mostly for pumping other lasers, also CD and DVD players• VCSELs and VECSELs (virtical cavity surface emission
lasers and virtical exteranl cavity surface emission lasers)• Also for seeding pulse fiber lasers (next page)
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53USPAS, 2008
Mode-locked semiconductor lasers:(using V)
• Can achieve sub picosecond pulse duration• 500 mW power• Widely tunable• Very high rep rate, up to 100 GHz
Opt. Express 16, 5770 (2008)
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54USPAS, 2008
Pump for lasersFlash lamps: – Converts electrical power to light– Cheap, low pumping efficiency, and poor
stability. – Still opted for situations when high energy
capacity is the key (NIF), suitable for ruby laser, Nd:Glass, Nd:YAG, Nd:YLF, etc.
Laser diodes: – converts electrical current into light– High efficiency, high stability especially in CW
mode. – Opted now for most off the shelf KHz system
and fiber lasers Pump lasers (Nd:YAG or Nd: YLF)– Both pumped by flash lamps and diodes– Normally for Ti: Sapphire system.
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55USPAS, 2008
Fiber lasers
Power progress in fiber laser sources
Teodoro et al, Laser Focus World, Nov. 2006
Peak Power over 1 MW
Average power over 2 kW
limited by available pump
Credit: David Richardson
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56USPAS, 2008
Laser configuration: Fiber lasers
Can be a straight MOPA or a CPA Low threshold, high efficiency, high rep rate, high powerNo thermal problem, good stabilityRelatively large bandwidth for CPA fiber
Credit: David RichardsonJ. Limpert et al., 'High-power ultrafast fiber laser systems,' IEEE Xplore 12, 233 (2006).
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57USPAS, 2008
Fiber laser wavelength
Credit: David Richardson
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58USPAS, 2008
Fiber laser capabilities
Credit: David Richardson
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59USPAS, 2008
Fiber laser architecture
Credit: David Richardson
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60USPAS, 2008
A short pulse MOPA fiber laser example1 GHz, 20 ps, 321 W average and 13 kW peak power
Dupriez et al, http://www.ofcnfoec.org/materials/PDP3.pdf
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61USPAS, 2008
A CPA fiber laser example 73 MHz, 220 fs, 131 W average and 8.2 MW peak power
Roeser et al., Opt. Lett. 30, 2754 (2005)
J. Limpert et al., 'High-power ultrafast fiber laser systems,' IEEE Xplore 12, 233 (2006).
1 μm, 1 mJ, 1 ps, 50 kHz has been achieved, F. Roeser et al, Opt. Lett. 32, 3294 (2007)
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62USPAS, 2008
ContentLaser and accelerator historyMap of laser application in acceleratorsLaser basics– Rate equations– Laser configurations– Gaussian beam optics and ABCD law– Laser cavity and laser modes
Laser configurations– Mode-lokcing and q-switch– MOPA – CPA and dispersion
Laser materials Other lasers– Semiconductor lasers– Fiber lasers
Frequency conversion and short wavelength lasers
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63USPAS, 2008
Maxwell equation in a medium
The induced polarization, P, contains the effect of the medium:
0 0 0
0
0
BE Et
E PB Bt t
μ ε μ
∂∇ ⋅ = ∇× = −
∂∂ ∂
∇ ⋅ = ∇× = +∂ ∂
rr r r r
r rr r r r
The induced polarization in Maxwell’s Equations yields another term in the wave equation:
As we’ve learned, this is the “Inhomogeneous Wave Equation.”The polarization is the driving term for a new solution to this equation.
2 2 2
02 2 2 2
1E E Px c t dt
μ∂ ∂ ∂− =
∂ ∂
Credit: R. Trebino
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64USPAS, 2008
Maxwell equation in a nonlinear medium
Credit: R. Trebino
What are the effects of such nonlinear terms? Consider the second-order term:
2ω = 2nd harmonic!
Harmonic generation is one of many exotic effects that can arise!
(1)0ε χ⎡ ⎤= ⎣ ⎦c X
*
*2222
( ) ,
( )
exp( ) ex
2exp(2 ) exp(
p
2
(
)
)
E
E i t
i t E
E i t
i t
t
t E
ω ω
ω ω
∝
−∝
+ −
+ +
X
X
Since
(1) (2) 2 (3) 30 ...ε χ χ χ⎡ ⎤= + + +⎣ ⎦c X X X
Nonlinear optics is what happens when the polarization is the resultof higher-order (nonlinear!) terms in the field:
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65USPAS, 2008
[ ] [ ][ ] [ ]
* *1 2 1
* *1 2 1 2 1 2 1 2
2 *
2
2 21 2
2 1 2
2
2
1 2
2 2
21 1 1
2
*1
2
2 exp (
exp(2 ) exp(
2 exp (
exp(2 ) exp( 2 )
) 2 exp
) 2 ex
2 )
(
p
( )
)
(
2
)
2
E i t E
E
E E i t E E i t
i t
E
E i t E E i t
E t
E E
i t E i t
ω ω
ω ω
ω ω ω
ω
ω
ω
ω
ω
+
+
∝
+
+
+ −
+ − +
+
+
−
+
+ −
− −
Sum and difference frequency generation
Suppose there are two different-color beams present:
*1 1 1 1
*2 2 2 2exp( ) e exp( ) exp( ) x (( )) pE i t E i t E i t E i tE t ω ω ωω + − −∝ + +
Note also that, when ωi is negative inside the exp, the E in front has a *.
2nd-harmonic gen
2nd-harmonic gen
Sum-freq gen
Diff-freq gen
dc rectification
So:
Credit: R. Trebino
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66USPAS, 2008
Credit: R. Trebino
Conservation laws and phase matching
Unfortunately, may not correspond to a light wave at frequency ωsig!
Satisfying these two relations simultan-eously is called "phase-matching."
sigkr
1 2 3 4 5 sigω ω ω ω ω ω+ + − + =
1 2 3 4 5 sigk k k k k k+ + − + =r r r r r r
Energy must be conserved:
Momentum must also be conserved:
sigkr
ωsig
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67USPAS, 2008
Phase matching and conversion efficiency
Small signal second harmonic conversion efficiency
2/30
30
200
222
22222
2
2222
46.58
,2
sin
2
2sin
nd
ncd
C
lLcILC
kL
kL
ILCI
effeff
c
λλεπ
πωωω
==
=
⎟⎠⎞
⎜⎝⎛ Δ
Δ
=
Δk=4π/λ1(n1-n2): difference in wave umberL: crystal lengthlc=π/Δk, coherence length (when phase is matched)deff: effective nonlinear coefficient, in m/V
Credit: W. Koechner: Solid State Laser engineering,
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68USPAS, 2008
Conversion efficiency at small signal
The small signal conversion efficiency and effect of phase mismatch
clLcLC
2sin 222 πη =
Credit: W. Koechner: Solid State Laser engineering,
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69USPAS, 2008
Quasi phase matching
Quasi-phase matching Achieve phase matching by modulating the spatial nonlinear property
Tune the interaction here
Encyclopedia of Laser Physics and Technologyhttp://www.rp-photonics.com
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70USPAS, 2008
Quasi-phase matching: Periodically poling crystals
The most popular technique for generating quasi-phase-matched crystals is periodic poling of ferroelectric nonlinear crystal materials
Credit: www.raicol.com/products.asp
Wavelength Range: 400-4000 nmDimensions:
Thickness: up to 1 mm Width (typical): 2 mm Length: up to 30 mm
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71USPAS, 2008
Pump depletion and signal saturation
Phase match, with pump depletion
,2
sintanh 2/122 ⎟⎟
⎠
⎞⎜⎜⎝
⎛=
clLcCLIII π
ωωω
Consider frequency quadrupling– At low pump power, highly nonlinear
Consider frequency quadrupling– At high pump power, linear, desired
4224
22
ωωω
ωω
IIIII
∝∝⇒
∝
ωωω
ωω
IIIII
∝∝⇒
∝
24
2
linearsaturation
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72USPAS, 2008
Frequency conversion: High order harmonics generation
Atoms as the nonlinear mediaEmission due to multiple photon absorption of electrons bounded to an atomCarry over the spatial coherence of the driving laserOf short pulse duration comparable or shorter than the drive laser up to attosecondsCurrently at ~10 nm.
H. Kaptyn et al., 'Harnessing Attosecond Science in the Quest for Coherent X-rays,' Science 317, 775 (2007).
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73USPAS, 2008
High order harmonics generation: phase matching
Phase mismatching due to group velocity difference or continuous signal emission or group velocity mismatchCan be accomplished by modulating the interaction via modulated laser propagation or counter propagating beams
H. Kaptyn et al., 'Harnessing Attosecond Science in the Quest for Coherent X-rays,' Science 317, 775 (2007).
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74USPAS, 2008
Short wavelength lasers
Plasma base soft-x-ray lasers– Still a traditional laser based on population inversion, but in hot dense
plasma to accommodate the high energy difference between atomic levels, wavelength from 1 nm to 100 nm.
– Can be pumped by laser, discharge, and bombs– Challenges: tunability and capability for shorter wavelengths,
stabilities– J. Hecht, “The history of X-ray lasers,” Optics & Photonics News 19,
26 (2008); Y. Wang et al., Nature Photonics 2, 94 (2008)
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75USPAS, 2008
Short wavelength lasers
X-ray Free electron lasers: 0.1 nm, high brightness, high transverse coherence, etc. Design with cavity going onMany projects going on