Rate Eq.

100
201 Rate Equation for Rate Equation for 2 2 - - Level System Level System 2 St.em. Sp.em. Stim.abs. 2 21 2 21 2 12 1 ' ' dN R R R dt dN I Bg v N AN dt c I Bgv N c 2 Rate equation for a 2 - level system is the change in occupance of N per time :

description

Laser

Transcript of Rate Eq.

Page 1: Rate Eq.

201

Rate Equation forRate Equation for22--Level SystemLevel System

2St.em. Sp.em. Stim.abs.

221 2 21 2

12 1

'

'

dNR R R

dt

dN IB g v N A N

dt c

IB g v N

c

2

Rate equation for a 2 - levelsystem is the change inoccupance of N per time :

Page 2: Rate Eq.

202

Rate Equation forRate Equation forEnergy Level Energy Level ““11””

1St.em. Sp.em. St.abs.

121 2 21 2

12 1

'

'

dNR R R

dt

dN IB g v N A N

dt c

IB g v N

c

Page 3: Rate Eq.

203

Capture CrossCapture Cross--SectionSection

12 21

21

Capturecross-section

area

Equation 26-9

'' area

B B

hvB g v

c

Define Capture Cross - Section :

Page 4: Rate Eq.

204

Rewriting Rate Equation Rewriting Rate Equation for Twofor Two--Level System:Level System:

221 2 2 1

121 2 2 1

1 2

'

'

T

dN IA N N N

dt hv

dN IA N N N

dt hv

N N N

Total # of atoms is :

Page 5: Rate Eq.

205

TwoTwo--Level Laser canLevel Laser can’’t t occur because:occur because:

Inversion can’t happen:

Ninv = N2 – N1

= Negative value

Stim. Emiss. + Spon. Emiss.> Stim. Absorp.

Since Capture Cross Section (σ)is the same!

Page 6: Rate Eq.

206

Two (2) Common Laser Two (2) Common Laser SystemsSystems

3 Level

E3

E2

K21 - Lasing

N2

E1

Pump

K32 spon

N1

p

p

I

hv

Nt =N1+ N2+ N3

3 level

4 level

Page 7: Rate Eq.

207

22ndnd Common Laser Common Laser SystemsSystems

4 Level

3

2

Laser

N2

0

N11

NT = N1 + N2 + N3 + N0

Page 8: Rate Eq.

208

44--Level Laser SystemLevel Laser System

3

2

Rate → Laser λ

N2

0

N11Ip

N3

K32

K21

K10

N0

32 21

32 3

3

p

is very fast so e don't reside in .

0

In fact, the assumption is that e in 3 instantaneouslyfalls to level 2.

Figure 26-5, p. 557 (Pedrotti).

Photon from pump must have a capturecros

K K

K N

N

hv

s section.

1

Lifetime

Pumping Rate

Stimulatedemission

p

K

I

R I

K20

K31

K30

Page 9: Rate Eq.

209

Rate Equations for Pumping a Four Rate Equations for Pumping a Four Energy Level System: Change in Energy Level System: Change in

Occupy per TimeOccupy per Time

33 3 3 0

232 3 2 2 2 1'

is

p p

p

IdNK N N N

dt hv

dN IK N K N N N

dt hv

I

View 4 - level structure and write down rate ofchange for each level

Gain from ground

Population Change, Level 3, #/sec

Stimulated emission

131 3 21 2 10 1 2 1

030 3 20 2 10 1 3 0

T 0 1 2 3

3 30 31 32

2 21 20

laser cavity Irradiance

d

dt '

p p

p

N IK N K N K N N N

hv

IdNK N K N K N N N

dt hv

N N N N N

K K K K

K K K

All the atoms in Four Levels :

Page 10: Rate Eq.

210

Rate Equations for Pumping a Rate Equations for Pumping a Four Energy Level System: Four Energy Level System: Change in Occupy per TimeChange in Occupy per Time

/3 2 1

3 2 10

2p

2

1 1 1 1; ; ; point

Capture cross section M for pump photons

watt Pump irradiance,

M

Energy of photons used in pump (joules)

Capture cr

t

p

p

eK K K e

I

hv

Recall K are reciprocal lifetimes :

oss section for Lasing photons @ 'v

Page 11: Rate Eq.

211

44--Level Laser OperationsLevel Laser Operations

2p 0

0 3 0 0 1 2 3

30

3 3 0 33

232

Pump power flux (watt/M ) I does not empty the ground level (N )

; so

0 in steady state population inversion;

1

0

T

RT

p p p pT

p

N N N N N N N N

dNI I

dtI I

K N N N Nhv K hv

dNK

d

Assumption :

3 2 2 2 1

322 2 2 1

3

2

31121 2 10 1 2 1

3

1

2 1

'

'

relate to pump power input

0'

Solve for for the gain or inversion

p pT

p

p

p pT

p

p

IN K N N N

hv

IK IN K N N N

K hv hv

R

IKdN IN K N K N N N

dt K hv hv

R

N N

21 22 1

10 102 1

202

10

population

1

1'

"Population Inversion" Function of optical Power

p p

K KR R

K KN N

K IK

K hv

Page 12: Rate Eq.

212

Absorption/Loss Coefficient, Absorption/Loss Coefficient, αα

2

Use this inversion to produce gain in thethe optical irradiance as it propagates. The

incremental change in irradiance (w/M ) is( ) in time going through a volume

w

dII

dz

I V

Change in irradiance :

ith cross section and length

'

# of photons generated

I '

z

A z

hv nI

A

n

hv n

V t

Dividing by Δz :

I + ΔII

ΔA

Page 13: Rate Eq.

213

Change in Irradiance Change in Irradiance through a Volumethrough a Volume

2 1

22 1

'

Each transition produces '

Volume of the gain media

Rate of change eq. of photons

is equal to population rate ( )

( ) slide 205'

I n hv

z t V

hv

V

N N

n IN N V

t h

Page 14: Rate Eq.

214

Absorption CoefficientAbsorption Coefficient

2 1

2 1

2 1 2 1

differential

'

Rate of stimulated emission

Substitute into

'

'

But recall 210; definition

n IN N V

t hv

I

z

I hv IN N V

z V hv

dII N N N N I

dz

dI

dz

2 1

Their absorption is negative

Where is gain coefficient

I

N N

dII

dZ

Page 15: Rate Eq.

215

Typically:Typically:

0 0

0

0

ln

Beer's Law

LI L

I

L

LL

dII

dz

dIdz

I

IL

I

I I e

Page 16: Rate Eq.

216

Gain CoefficientGain Coefficient

2 1

0

Gain coefficient

LL

N N

I I e

How much pumppower is needed?

Page 17: Rate Eq.

217

Laser Power Output Laser Power Output ConditionsConditions

• Set up 2-mirror laser cavity

• Derive output irradiance

– eq. 26-47(Pedrotti, derived inSlides 220-224)

• Stability conditions

• Homogeneous vs. inhomogeneous broadening

Page 18: Rate Eq.

218

Optical TransitionsOptical Transitions

E2 + ΔE2

E1 + ΔE1

γ

Gain Curveγ = σ(N2 – N1)

Max gain for hv = E2 – E1

v

Lasing Energy Levels

Band of energy levels

(E2 – E1)

(E2 + ΔE2) –(E1 – ΔE1)

Corresponds to

(E2 – ΔE2) –(E1 + ΔE1)

Page 19: Rate Eq.

219

Modes of LaserModes of Laser

γ

Gain Curve

γ = σ(N2 – N1)

Max gain for hv = E2 – E1

v

3 Modes must be above gain threshold

2

C

L 2

C

L

Page 20: Rate Eq.

220

Laser CavityLaser Cavity

0

Mirror (100% refl.)output mirror (<100%)

cavity lengthgain media length

Resonants

sin

Electric field must be phase exactlyafter round trip, within cavity

22 2 2 ;

integer

2L

2

L

LL

E E kz t

k L L m

m

m

Lv

c

A.

B.

2

resonants occur @c/2 apart and are called modes

m

cv m

L

L

Page 21: Rate Eq.

221

Threshold ConditionThreshold ConditionCW CW –– Continuous WaveContinuous Wave

2 2 2 1R l

Scattering, etc.

0

00 0

0 2 1

2

2 10

;

; gain coefficient

Round trip intensity from initial location

;

Small signal output (1% coupler); steady state conditi

g

Lg

Lg

LRT

dI dII dz

dz I

I I e N N

IR R e Milonni & Eberly (Wiley, 1988)

I

00

2

2 10

1 2 1 22 1

1 2

onwarrants that the intensity remains constant inside cavity

; 1

1 ; small signal gain coefficient

1ln 2 ln 1 ln

Trig expression, 1 Taylor Exp.

T g

RTRT

LRT

T g

II I

I

IR R e

I

L R R R RR R

R R x

T

1 2

1 2

Steady state - threshhold gain. coefficient - 1

1 other losses per length2

1 1Threshhold gain ln

2

Tg

T Tg

x

R RL

L R R

Page 22: Rate Eq.

222

Ideal 4 Level LaserIdeal 4 Level Laser

31 202 1 p1

3 10

10 10

No simulated emission transitions from 3 to 1 level;k

0 in Equation (207) of force R to z; 0

Atoms in energy level 1 fall to zero (ground state) with zerolifetime, 1/

Optic

kN N

k k

k

2 1

02 2

2

2 320 2 2 2

2 3

2

0

al Gain - Equation 26-37 - from slide 207,

gain 1 ' 1

Where we grouped terms:

'Saturation irradiance

Setting threshold gain

P

s

p p pp T

p

s

N N

R kII hv k

I

R IkR N

k k hv

hvI

0

1 2 Sat.

0

Sat. 1 2

0Sat.

1 2

equal to increase population gainand equal above,

1 1ln

2 1

21

ln 1

21 Irradiance/intensity

ln 1 inside cavity

T

Tg

g

g

L R R I I

LI

I R R

LI I

R R

Page 23: Rate Eq.

223

Laser OutputLaser Output

As we increase γ0 (gain coeff.), it reaches γthreshhold and can’t get above γT

out 2 2

; ; 2

Positive z direction field2 gives output beam

Substitute from previous slide

I I I I I I I

II T I T

I

20pumps p

KI

320 2

3

pumps (Slide 217)p Tp T p

p

NkI N I

k hv

←Transmissionof Mirror 2

Page 24: Rate Eq.

224

Laser OutputLaser Output

1 2

0 Sat.out 2

1 2

1 2 1 21 2

1 2

1 2 2

1 2 2

1ln 1 Taylor expansion

21

1 2ln

1ln ln1 ln ln

1

1 Loss due tomirror's transmission

+

is 100%, so 1 but there

g

x R Rx x

L II T

R R

R R R RR R

R R

R R T

R R T

0 satout 2

2

are other lossessuch as scattering and spontaneous emission

21

2gL I

I TT

Page 25: Rate Eq.

225

Output Power DerivationOutput Power Derivation

Pedrotti3 26-19. Derive Eq. (26-47) by a procedure similar to that leading to Eq. (26-43).

The linear cavity case is complicated by the fact that the field encounters the gain medium twice in each round-trip with the losses encountered at the mirrors interspersed between passes through the gain medium.

It may be useful to research and then summarize the solution to this problem.

Gain Medium

IoutI2+I1+

I1- I2-

R1 R2, T2L

Right going field: Left going field: dI dI

I Idz dz

Page 26: Rate Eq.

226

Output Power Derivation, cont.Output Power Derivation, cont.

0

Saturation is due to both the right and left going fieldsin the cavity, so we can rewrite Equation (26-40) as:

1 1(1)

1

1 1This relation leads to: 0

Where the abo

S

dI dII II dz I dz

I

dI dI

I dz I dz

2 2

ve expression is used below:

1 1 1ln

ln 0

Therefore: ln

Now find the output irradiance shown in Eq. 26-47.

(2)

(3)

(4)

Solve (

C

out

dI dIdI I

dz I dz I dz I I

dI I

dz

I I C I I e C

I I I

I I C

I T I

3) for and substitute into (2): C

I I II

Page 27: Rate Eq.

227

Output Power Derivation, cont.Output Power Derivation, cont.

2

1

+

0

0

0

22 1 0

1 2 1

1 1

Take (1) for the I equation, separate variables and integrate.

1

1

11

1 1 1ln (5)

Now,

S

I L

SI

S S

dII II dz

I

CI

IdI dz

I I

I CI I L

I I I I I

I I

2 2

1 2

1 1 1

2 2 2

1 1 2 2

11 2 2 2

1

1 2 1 2 2 2

and are the reflectance of the two mirrors, so that

Using the above 3 relationships:

Therefore: and

I I C

R R

R I I

R I I

I I I I

II I I R

R

I I R R C I R

Page 28: Rate Eq.

228

Example Problem, cont.Example Problem, cont.

22 2 1 2

2 1 2

2 20

2 2 1 2

2

2 2 21 2 2 0

11 2

2 21 2 2 0

1 1 2

Substituting these into (5):

1ln

1 1

Solve for I :

1ln 1

1 11 ln

2

S

S

S S

S

II I R R

II R R

I RL

I I I R R

I I RR R R L

I I RR R

I RR R R L

I R R R

2 21 2 1 2 0

1 1 2

2 21 2 0

1 1 2

01 22

21 2

1

1 11 1 2 ln

2

1 11 1 2 ln

2

12 ln

21 1

S

S

Sout

I RR R R R L

I R R R

I RR R L

I R R R

LR RT I

IR

R RR

-- Derivation courtesy

of Kyung Lyong Jang

Page 29: Rate Eq.

229

2 Mirror Laser2 Mirror Laser2

1

1

0 Sat.out 2

2

Mirror 2 is output coupler - T ; from slide 219

Therefore T is a loss if reflectance is not 100%

Also, other losses in cavity

All losses = T scattering absorp.

21

2

iff losse

gL II T

T

2

2 2 2

Sat.out 0 2

0

out Sat.

Sat.

s are much less than T

,

22

Output varies (depends) linearly on

(Small signal gain coefficient).

Different materials have different ( ) saturation lifetimes.

g

T T T

II L T

I I

I

21

Sat.0 0 21

Lifetime

1

2 2

Higher ultraviolet, x-ray, are more difficult to build.

k hvI

v

2

1

Page 30: Rate Eq.

230

0

0 2 1

Small signal gain coefficient depends on

population inversion,

#Pump rate

Sec.

i.e., 3 Level Laser

N

N N

N

Pumprate

Fast decayN2

N1

gain

γ

γT

Threshhold

Gain saturationround trip intensity in

cavity is constant

Pump rate

Pout

2

out

Sat.out 0

out

opt 0

What is the optimum output coupler ( )?

Solve for given loss:

22

0

2

g

g

T

I

ITI L T

T S

I

T

T L

Iout

ToptT2

Outputcoupler

x

Page 31: Rate Eq.

231

Laser Cavity Stability ConditionsLaser Cavity Stability Conditions

1 2

1 11

22

1 2

1 2

1 2

1 2

0 1

1 ; radius of curvature of mirror

1

Confocal cavity

1 1 1 1 0

Concentric Cavity

2

1 2 1 2 1

These are li

g g

Lg r

r

Lg

r

L r r

g g

L r

r r r

g g

Two extremes to get Lasing :

A.

B.

mits to cavity length!

Page 32: Rate Eq.

232

Laser Line Width orLaser Line Width orLineshapeLineshape g(g(vv’’))

• Not perfectly monochromatic

Two general mechanisms that cause freq. broadening:

– Homogeneous – Physical phenomena in gain media that affect all atoms in the same manner that broaden the frequency response of each atom

– Inhomogeneous – Physical mechanism that affects different groups of atoms in different manners, i.e., He or Ne atoms

Full width at half maxHv ½

Page 33: Rate Eq.

233

•Lifetime Broadening– τ2 is not exact value, but has some spread

– Causes:A. Spontaneous emission

B. Inelastic collision of atoms, which changes its energy (Pressure, temperature of media)

Homogeneous BroadeningHomogeneous Broadening

•Pressure Broadening– Elastic collisions of atoms cause delays in emission

– Typically the dominant cause of homogeneous bonding (vcol)

1 2 Time

τL + ε τL + ε2

2

2

0

col2 1

2 2 1 1 col

Lorentzian line shape

22

1 1 1 2

2

Lifetime , Lifetime , Rate of collisions

H

H

H

g v

vg v

vv v

v v

E E v

Gain Bandwidth :

Page 34: Rate Eq.

234

Recall Gain Cavity:

0Electronic field sin .Round trip has to be in phase (exactly).

22 2 4 2 ( ) ( is integer)

4 2 ; 0, 1, 2;2

Therefore, cavity will have/support any

frequency that ha

E E kz t

vkz k L L L kz m m

cv c

L m m v mc L

v

8

8

s values or modes2

Modes spacing in frequency is 1; apart2

3 10i.e., 1 meter, 1.5 10 Hz

2 1

Homogeneous broadening gain media only allowes lasingat one of these frequencies - single cavity mod

cm

L

cm

L

L v

e!

Page 35: Rate Eq.

235

Homogeneous Gain MediaHomogeneous Gain Media

Only one mode in cavitywith homogeneous broadening

Page 36: Rate Eq.

236

Inhomogeneous BroadeningInhomogeneous Broadening

• Doppler effects (gas laser) causing larger linewidth

–Velocity of Ne atoms are moving with a distribution of velocities which produce a doppler shift in frequency, v (train whistle).

–Velocity of Ne atoms are moving in 4π steradians so only zcomponent is causing frequency shift

Page 37: Rate Eq.

237

InhomogenousInhomogenous BroadeningBroadening

20

14 ln 22

2

1

2

02

26

4 ln 2

Full width at half max

8ln 2

Mass of atom (atomic mass)

6.64 10 kg

D

v v

v

D

D

BD

g v ev

v

k Tv v

Mc

M

Gaussian Lineshape :

Page 38: Rate Eq.

238

Inhomogeneous BroadeningInhomogeneous Broadening

Δvinhomo.> Δvhomo.

Willis Lamb - @OSC Professor

Page 39: Rate Eq.

239

High Intensity is Possible High Intensity is Possible by Pulsed Operationby Pulsed Operation

– Super saturate the cavity; then, switch it on for a short time• Q switch• Mode lock

– Cause population inversion but don’t let it lase

– Average power = continuous wave (CW) operation

Page 40: Rate Eq.

240

Laser Types & WavelengthLaser Types & Wavelength• Gas

– HeNe, CO2

• Solid State– Nd:YAG– Ruby

• Chemical– HF & DF

• Free-Electron– X-ray

• Range– 1nm < λ < 1mm

• Continuous wave – CW Power– 1 mw to 5 megawatts(?)

• Pulsed Power– 1015 joules

• Pulsed Length, shortest– 5 fsec → f = 10-15

• Cavity Lengths – L– Few μm < L < km

Page 41: Rate Eq.

241

LED – Light Emitting Diodes

• Emitted photon goes in 4π steradians

--Courtesy of Tomasz Tkaczy

Page 42: Rate Eq.

242

Surface Emitting LED

--Courtesy of Tomasz Tkaczy

Page 43: Rate Eq.

243

Laser Diodes –Electrical & Optical Properties

• Cavities, mode behavior

• Power – current plot

• Divergence

• Astigmatism

• Polarization

• Laser Diodes as geometrical light sources

--Courtesy of Tomasz Tkaczy

Page 44: Rate Eq.

244

Laser Diode Electronic Properties

--Courtesy of Tomasz Tkaczy

Page 45: Rate Eq.

245

Laser Diode Cavities

--Courtesy of Tomasz Tkaczy

Page 46: Rate Eq.

246

Laser Diode Power-Current Typical Curve

--Courtesy of Tomasz Tkaczy

Page 47: Rate Eq.

247

Laser Diode Mode Behavior

--Courtesy of Tomasz Tkaczy

Page 48: Rate Eq.

248

Laser Diode Polarization

--Courtesy of Tomasz Tkaczy

Page 49: Rate Eq.

249

Laser Diode Divergence

--Courtesy of Tomasz Tkaczy

Page 50: Rate Eq.

250

Laser Diode Divergence

--Courtesy of Tomasz Tkaczy

Page 51: Rate Eq.

251

Circularize by single-prism expansion

--Courtesy of Tomasz Tkaczy

Page 52: Rate Eq.

252

Gaussian Beam ProfilingGaussian Beam Profilingand Propagationand Propagation

• Objectives:

– Review on Gaussian beam intensity profile

– Geometrical approach to Gaussian beam profiling

– Beam propagation

Page 53: Rate Eq.

253

Classical Treatment of Classical Treatment of Gaussian BeamGaussian Beam

• Gaussian beam: Ideally, the irradiance distribution in any transverse plane is a circularly symmetric Gaussian function entered about the beam axis

• 64% between std. dev.• 86.5% energy between ±w

Page 54: Rate Eq.

254

Classical Treatment of Classical Treatment of Gaussian Beam (Cont.)Gaussian Beam (Cont.)

W0 = Beam Waist; smallest radius in that space

Measure distances relative to beam waist@z = 0

Page 55: Rate Eq.

255

Classical Treatment of Gaussian Classical Treatment of Gaussian Beam (Cont.)Beam (Cont.)

• The complex electric field amplitude of Gaussian beam (eq. 27-24 Pedrotti):

2 210 0

02( , ) exp exp tan ( / )

( ) ( ) 2 ( )

E WE z i kz k z z t

w z w z R z

Amplitude Phase

Plane wave

Spherical wave

Phase retardationθ = -π/2 at z = -∞θ = π/2 at z = ∞

2 2

2: Wave numberk

x y

2 22 0

0 2

2

0 0

Beam irradiance:

2( , ) ( , ) exp

( ) ( )

WI z E z I

w z w z

I E

Page 56: Rate Eq.

256

Rayleigh RangeRayleigh Range

20

0

Given without proof:See equation 27-21

Wz

Figure 27-2 (Pedrotti)

Page 57: Rate Eq.

257

Classical Treatment of Gaussian Classical Treatment of Gaussian Beam (Cont.)Beam (Cont.)

0

0

20

0 0 0

2

0 0 20

The axial distance within whichthe beam Intensity drops to ½ and beam radius lies within

a factor of 2 of waist radius

( ) 2

1( , ) exp

2

W

Wz w z W

I z IW

Rayleigh range (Z ) :

Beam diverge

20 0

00 0

*angular spread is fn(wavelength)

and waist is small -- recall Fourier

W*tan if z , we have ( )

Wz w z z

z W

nce angle :

Page 58: Rate Eq.

258

Classical Treatment of Gaussian Classical Treatment of Gaussian Beam (Cont.)Beam (Cont.)

• Definition: Beam radius or beam width w(z): the radial distance of a circle that contains approximately 86% of the power (or irradiance drops down to 1/e2

13.5% of the peak irradiance)2 2

2

00 0 02

0 0

( ) 1 1Wz z

w z W W zz W

• Beam waist W0: where beam radius is minimum, i.e. z = 0 plane– The wavefronts are approximately planar near the beam waist

(See page 239)

x

y

W(z)

20 0

0 0 2 220

0 0

0,1

W zI z I I

z zW z z

2 20

0 2

2,

WI z I e

W z W z

Page 59: Rate Eq.

259

Classical Treatment of Classical Treatment of Gaussian Beam (Cont.)Gaussian Beam (Cont.)

22 20 0

220

0 0 0

10

0

Radius of wavefrontat the Rayleigh waist

Phase

( ) 1 1

@ Rayleigh distance

2( ) 2

( ) tan ( ) 4

z WR z z z

z z

WR z z kW

zz z

z

Radius of Curvature :

Phase retardation :

2 20 0

2

at the Rayleigh waist

( , ) exp exp ( )( ) ( ) 2 ( )

E WE z i kz k z

w z w z R z

Page 60: Rate Eq.

260

Classical Treatment of Gaussian Classical Treatment of Gaussian Beam (Cont.)Beam (Cont.)

2 20

0 2

2

0 00 2

0

2( , ) exp

( ) ( )

(0, )( ) 1 ( )

WI z I

w z w z

W II z I

w z z z

Intensity on z axis :

0 029 2 2

1

I I

zz

0

2

I

Page 61: Rate Eq.

261

Classical Treatment of Classical Treatment of Gaussian Beam (Cont.)Gaussian Beam (Cont.)

20 0

0

2 20

0 2

Beam power: the total power, , carried by a beam is the

integral of the optical irradiance over a given transverse

plane at a distance z:

1( , )2

2

2( , ) exp

( ) ( )

I z d I W

WI z I

w z w z

0

2

2 2

0

0

0

20

2

2 2exp

( ) ( )

Relative power carried by an aperture with a radius r

1( , ) ( , )2

21 exp

( )

r

w z w z

p z I z d

r

w z

x

y

ρ0

Page 62: Rate Eq.

262

Classical Treatment of Classical Treatment of Gaussian Beam (Cont.)Gaussian Beam (Cont.)

0 20

0 20

2

Encircled energy by the Beam width w(z) (radius)normalized contains approximately 86% of thetotal power:

21( , ) ( , )2 1 exp

( )

1, 1 86%

1.5 , 99%

p z I z dw z

p w z ze

p w z z

x

y

ρ0

w0=1

Page 63: Rate Eq.

263

Summary of Gaussian Beam Eq.Summary of Gaussian Beam Eq.

2

2 2

20 0

2 20

0 2

20

0

1/ 2 22

0 020 0

2 2Irradiance: ( , ) exp

( ) ( )

1watts

2

2( , ) exp

( ) ( )

Rayleigh range

( ) 1 1

I zw z w z

I W

WI z I

w z w z

Wz

z zw z W W

W z

1 1 λ= +iq(z) R(z) πw(z)

1/ 2

0 0

2 220 0

0

0 0

( ) 2

( ) 1 1

tan ff

w z W

W zR z z z

z z

W

z W

Page 64: Rate Eq.

264

Example ProblemExample Problem

• 27-23 The output from a single mode TEM00 Ar+ laser ( λ = 488 nm) has a far field divergence angle of 1 mradand output power of 5 watts.

0

3

0 3

20 0

20 2 2

0

0

tan

0.488(10 )

(10 )

15 watts

2

2 2 51.32 10

0.155

ff

ff

W

W

I W

IW

I

Answer

4

a. What is the spot size at the beam waist?

0.155 mm

b. What is the irradiance at the beam waist?

1.32 10 w/ 2

Answercm

Page 65: Rate Eq.

265

Example, cont.Example, cont.

2 20

0 2

1/2 1/22 2

0 020 0

2 20

0

2( , ) exp

( ) ( )

( ) 1 1

(0.155)

WI z I

w z w z

z zw z W W

W z

Wz

c. What is the irradiance at the center of the beam

at 10 meters from the beam waist?

3

1/2 1/22 2

0 0

4

Answer2

154.6 mm0.488 10

( ) 10,0001 1 64.7

154.6

1.32(10 )(0,10 meters)

65

w z z

W z

I

23.15 w / cm

Page 66: Rate Eq.

266

Gaussian Beam Profiling with Gaussian Beam Profiling with Knife EdgeKnife Edge

16%

84%

w(z)

Beam radius( )

2

w zx

( )

2

w zx

x

y

Knife edge

2

0

Knife Edge

1( , ) ( , ) ( , )

1 21

2 ( )

2( )

x

xt

p x z I y z dy I x z dx

xerf

w z

erf x e dt

Page 67: Rate Eq.

Error Function Table

Page 68: Rate Eq.

268

Geometrical Approach to Geometrical Approach to Gaussian Beam (Cont.)Gaussian Beam (Cont.)

• Standard Deviation (STD) beam radius (z): the radial distance of a circle that contains approximately 63.2% of the power (or irradiance drops down to 1/e 36.8%of the peak irradiance)

1/ 2 1/ 22 2

0 02

0 0

( ) 1 1z z

zk z

x

y

w(z)

(z)

86%

63.2%

1/e2

= 13.5%

1/e= 36.8%

-

Page 69: Rate Eq.

269

Gaussian Beam Encircled EnergyGaussian Beam Encircled Energy• Encircled energy by the STD Beam radius (z):

it contains approximately 63.2% of the power

0

00

2

0

2

2

0

2

1( , ) ( , )2

21 exp

( )

1 exp( )

1( ( ), ) 1 63.2%

1.5* 2 * ( ), 99%

r

p r z I r z rdr

r

w z

r

z

p z ze

p z z

w0=1

(z)

x

y

r0

Page 70: Rate Eq.

270

Spatial Filter (Cont)Spatial Filter (Cont)

• Spatial filter: A pinhole centered on the axis is placed at the Fourier transform plane (image plane) to block high-frequency noise

• The key is to choose the right pinhole size that blocks unwanted noise but maximally passes the laser’s energy

Page 71: Rate Eq.

271

Spatial FilterSpatial Filter• Laser beam picks up intensity variation from scattering

by optical defects and particles in the air, known as spatial noise

• When a Gaussian beam is focused through a positive lens, equivalent to Fourier transform, the image at the focal plane will be mapped inversely proportional to the spatial frequencies

– Ideal Gaussian profile is imaged directly on axis

– Annulus of radius for noisy speckles:

nn dfr /

222

( )00 0 2

0

2( ) where

( )

r

w z

Actual Noise

WI r I e I

w z W

I I r I

0

ˆF

aW

Page 72: Rate Eq.

272

Beam ExpanderBeam Expander

• Afocal system, or inverted telescope– Keplerian beam expander

• A microscope objective is often used for the first positive lens

– Galilean beam expander21_ ffLengthOverall

12 / ffionMagnificat

Page 73: Rate Eq.

273

Spatial Filter (Cont)Spatial Filter (Cont)

• Relative power carried with a circle of radius r0

0 20

0 20

2

21( , ) ( , )2 1 exp

( )

1( ( ), ) 1 86%

(1.5 ( ), ) 99%

r

p r z I z dw z

p w z ze

p w z z

Page 74: Rate Eq.

274

Beam Power & Beam RadiusBeam Power & Beam Radius

• Relative power through a spatial filter with a diameter of D:

/ 2

0

2

0

1( , ) ( , )2

11 exp

2

D

p D z I r z rdr

W D

f

0

3 ( ) ( , ) 99.3%opt opt

fD w z p D z

W Recommended :

Page 75: Rate Eq.

275

Beam ImagingBeam Imaging

Spatial filter

Imaging lens

A small focused spot

Page 76: Rate Eq.

276

Lens LayoutLens Layout

• The approaching wavefront refracts at the lens at different times, depending on its distance from the optical axes (r).

• The delays of the various regions of the wavefront are proportional to the thickness of the lens at each radial zone (r), as shown above for a spherical wave.

1ikA

U er

Page 77: Rate Eq.

277

0

0

( ) ( ) ( ) (3.4)

( 1) ( )

k r k t t r nkt r

kt k n t r

where k(t0 – t(r)) is the phase delay caused by the free space region and it is assumed that the lens is surrounded by air (n = 1).

The wavefront’s velocity in the lens is slower than in air, so the section of the wavefront not in the glass will overtake the section that is in the glass.

Page 78: Rate Eq.

278

0

0

2 0

1 0

2 1

( )

( )

The emerging wavefront is given by:

(3.5)

where the input wavefront was

(3.6)

so the output wavefront is

(3.7)

Since the phase change ( ) is a functionof thickness,

ik r

ik

ik r

U U e

U U e

U U e

k rt

1 2 3( ) ( ) ( ) (3.8)

, at a given zone of radius , thelens can be divided into three sections in orderto find the thickness, ( ). Therefore, thethickness as a function of zone radius, , is:

wher

t r t r t t r

r

t rr

2e is the "edge thickness" of the lens.t

Page 79: Rate Eq.

279

Dividing the Thick Lens into Dividing the Thick Lens into Three SectionsThree Sections

Page 80: Rate Eq.

280

x2 + y2 + z2 = R2 if @ coord center.Equation of a spherical surface in 3-Dfor center z = +R (rotational symetric system)

2 2 2 2

2 2

2 2 2

2 2

( )

define z S(r) r x

( ( ) )

( )

x y z R R

y

s r R R r

s r R R r

Circular symmetryuse negative sign (-) due to sign conventionfrom surface to r-axis is to left.

How much shift do we get to plane through vertex?

Z

r

R

s(r)

Spherical Surface

Center ofCurvature (CC)

Sag of Spherical Surface

Page 81: Rate Eq.

281

2 2

1/ 22 2

1/ 22

2

324

22 4

2 2 3

( )

1

Since is small and / is squared,

1 can be expanded by a Taylor's series.

3

1 1 ...2 2 2! 2 3!

s r R R r

s r R R r

rs r R R

R

r r R

yyfRy R

R

Taylor Series/Maclaurin Series :

2 4 6

2 4 3 6

2 2

0

!

3( ) (1 ...

2 8 2 3!

We'll use the first two terms:

This is the lost distance( ) sag

by paraxial approx.....2 2

Where is:

1curvature

n n

n

y y ys y R R

R R R

y y Cs y

R

C

CR

Sag (Cont.)

Page 82: Rate Eq.

282

1 3

1/ 22 21 10 1 1

1 10

1/ 22 23 30 2 2

( )

( )

( )

The thickness ( ) and ( ) are related to the sag of aspherical surface, which can be expressed as:

(3.9)

(3.10)

Rewriting the equations:

t r t r

t r t r

R R

R R

t r t R

t r t r

1/ 22

1 21

1/ 22

3 30 2 22

1 2

1 1

( ) 1 1

(3.11)

(3.12)

Assuming the lens radius ( ) is small compared to thesurface radii ( and ), a Taylor series approximationcan be made fo

r

R

rt r t R

R

rR R

2

11

2

2

10

3 30

( )2

( )2

r the square root parts of Equations 3.11and 3.12, and using the first two terms of that expansiongives:

(3.13)

(3.14)

rt r t

R

rt r t

R

Page 83: Rate Eq.

283

2

01 2

2

0 01 2

2

2

2

01

0

Now Equation 3.8 becomes:

1 1( ) (3.15)

2

So the phase term, Equation 3.4 becomes:

1 1( ) 1 (3.16)

2

(3.17)

2

1 11

2

rt r t

R R

rk r kt k n t

R R

rknt k

f

rknt k n

R R

1 2

(3.18)*

Where we will define:

(3.19) 1 1 1

( 1)*

nf R R

Page 84: Rate Eq.

284

WavefrontsWavefronts

2 1 2 1R R z z

2 1 2 1q q z z

Page 85: Rate Eq.

285

Compare Gaussian toCompare Gaussian toSpherical Wave!Spherical Wave!

2 2

0tan

2 2

2

20

22 2 0

0 2

;

Radius of curvature is function of distance:

1

Waist as a function of distance is:

1

Due to these Gaussian properties

k kzi i iz i kz t i kz tR z r

R z Kr

E e e e E e e

zR z z

z

zW z W

z

02

, the distance alongrays are measured in imaginary terms;

. Follow Pedrotti 584-586.

1 1ori q z z iz

q z R z W z

complexradius of curvature

Page 86: Rate Eq.

286

Lens Coupling Gaussian BeamLens Coupling Gaussian Beam

Lens system just like transferring spherical beam following 1st order optics

2 1

2 1

2 1

1 1 1

f

Lens(es) can be represented by a matrix:

y

q q

yA B

C D

f

Page 87: Rate Eq.

287

Complex Radius of Curvature Complex Radius of Curvature of Gaussian Beamof Gaussian Beam

22

2

2 1 1 2 1 1

2 21 1

1 1

1 12 1

21

Radius of curvature of the beam is related to paraxialparameters:

So through a lens system, the radius of curvature ofa beam is:

1

yR

yR

y Ay B Cy D

yAR B CR D

AR By

CR D

1

11

1

1 12 2

1 1

1

;

AR B

CR D

AR B Aq BR q

CR D Cq D

Page 88: Rate Eq.
Page 89: Rate Eq.

289

Focus of a Gaussian Beam with LensFocus of a Gaussian Beam with Lens

2

1

21 0

2 2

2 220 0

2 2 2222

20

0

Complex radius of curvature of laser beam

1 1

Solve this by two boundary conditions:

@ Waist,

1

@ Coupling Mirror ( )

1 1 ( )

i

q R W

R

iq W

R

z WR z z

zz

Wz

a)

Page 90: Rate Eq.

290

Solving:Solving:

220

2 22

220

9

26 2

0

13 40

4 140 13

40

20

1

22 2 2

2 0 20

02 1

00.7 1

632.8 10 0.7

21 7.09 10 0

0.7

1 5.03 10 0

1.85710 3.692 10

5.03 10

0 4.38 10 meter

0.9524

( ) [1 ] 5

WR z

z

W

W

W

W

W

Wq i i

zW z W

z

4.44(10 ) meter

Page 91: Rate Eq.

291

1

2

2

3

3

1 0.7

0 1

1 0

1 1 11

2 1.5 1.5

1 0.004

0 1

1 0

11.5 1 1.5

0.64

1

0 1

1 0 1 01 1 0.004

0.5 0.5 20 1 0 11.5

0.64 3 3

R

R

A B

C D

b) Optical system transfer

1 0.7

0 1

1 0.53 0.7 0.63

0.53 0.63

Since complex radius of curvature, can't set 0 forsolving for .

B

Page 92: Rate Eq.

292

9

2 24

1 0

11 2

1

2

1 632.8 101.0499

4.38 10

0.9524

1 0.53 0.952 0.7 0.63

0.53 0.9524 0.63

0.505 0.952 0.7 0.63

0.63 0.505

Multipy by c.c.

i i iq W

Aq Bq i q

Cq D

iq

i

i

i

2c) What is complex radius of curvature q ?

2 2 2

2

2

of denominator

0.318 0.6 0.44 0.3970.255 0.481 0.354 0.318

0.63 0.505

0.041 0.652 0.954

0.652

0.0613 1.463

ii i

q

iq

q i

Page 93: Rate Eq.

293

Complex Radius of CurvatureComplex Radius of Curvature

22 2

2

9

2 22

7

22

1

but

6.32.8 10

2.01 10

q iR W

R

q iW

i

W

2d) q @beam waist of focused beam

Page 94: Rate Eq.

294

-7

22

42

Real:

0.0613 0

0.0613m

Imaginary parts:

2.01 101.463

3.7 10 m beam waist

W

W

e) Setting real and imaginary part equal

Page 95: Rate Eq.

295

Collimation of Gaussian BeamCollimation of Gaussian Beam

0

20

0

Lens for lasers are easier, no chromaticabberations

"Collimated distance" is between 2 adjacentRayleigh locations, or transverse size has

increased by 2 of waist 2

2 2

W

Wz

Page 96: Rate Eq.

296

Focusing a Gaussian BeamFocusing a Gaussian Beam

2 1

2 1 21 2

1

2 1 21 1 2

12

111

201

1

1 01 1

10 1 0 11

f

1f f

11

f f

1f f

11

f f

As before in example problem:

@ waist,

z z

z z zz z

A B

z C D

z z zq z z

Aq Bq

zCq Cq

Wq i R

2

022 @ waist,

Solving for beam waist and distance in focusing space.

Wq i R

z

Page 97: Rate Eq.

297

Focused Gaussian BeamFocused Gaussian Beam

22

0112 2 2

02 01

21

2 222 01

1

01 02

222201

0 1

020

1 1 11

f f

f ff

f

Focal length Raleigh rangeFocal length is small (large power)

f

2f

W

Wz

W W

zz

Wz

W W

WZ z

W

Assumptions :

From the above :

1

01

02

Recall if lens diameter 2

2F/#

2.44 F/# is larger for uniform irradianceacross lens

W

W

Recall diffraction :

Page 98: Rate Eq.

298

Example:Example:

1 2

1 2

1 2

1 2

A HeNe 5 mW laser has a cavity of 34 cm lengthwith concave mirrors of radius 10 m 10m

632.8nm

0 1 Stable cavity condition

0.34 0.341 ; 1

10 10

R R

g g

g g

g g

1) Is the cavity stable/viable for Lasing?

1 2

0.066 0.066 0.004356; stable

1Center length symmetry

2

17 cmz z

2) Where is the beam waist?

Page 99: Rate Eq.

299

Example, cont.Example, cont.

20

2 2

20

2

220

0

20

92 8

0

40

10 1

0.17

10 0.17 10.17

100.17 1 1.6711

0.17

1.29 m Raleigh range

1.29 632.8 1026 10

5.1 10 0.51 mm

zR z z

z

z

z

z

z

W

W

W

03) What is the spot size at the beam waist? W

Page 100: Rate Eq.

300

Example, cont.Example, cont.

22 2

0 20

22

2

0 0ff2

0 00

9ff

1

170.51 1 0.2646

129

0.514 mm

)?

tan2

632.8 10

2 0.5

zW z W

z

W z

W W

z WW

ff

4) Determine the spot size on the mirrors?

5) Determine the beam full angular divergence (

3

4ff

ff

1 10

3.95 10 rad 0.395 mr2

0.79 mr