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Low-loss Grating for Coupling to a High-Finesse Cavity. R. Schnabel, A. Bunkowski, O. Burmeister, P. Beyersdorf, T. Clausnitzer*, E. B. Kley*, A. Tünnermann*, K. Danzmann Institut für Atom- und Molekülphysik, Universität Hannover Max-Planck-Institut für Gravitationsphysik - PowerPoint PPT Presentation
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Low-loss Grating for Coupling to a High-Finesse Cavity
R. Schnabel, A. Bunkowski, O. Burmeister, P. Beyersdorf, T. Clausnitzer*, E. B. Kley*, A. Tünnermann*, K. Danzmann
Institut für Atom- und Molekülphysik, Universität HannoverMax-Planck-Institut für Gravitationsphysik
(Albert-Einstein-Institut),*Institut für Angewandte Physik, Universität Jena
LIGO-G050051-00-Z
2Aspen, 21.01.2005, Roman Schnabel
Is it possible to couple light to a cavity without transmission?
1st Order Littrow
Laser
m=0m=-1
2nd Order Littrow
Laser m=-2m=-1
m=0
Laser
3Aspen, 21.01.2005, Roman Schnabel
Is it possible to couple light to a cavity without transmission?
1st Order Littrow
Laser
m=0m=-1
Deep grating structure for high diffraction efficiencies
4Aspen, 21.01.2005, Roman Schnabel
Is it possible to couple light to a cavity without transmission?
2nd Order Littrow
Laser m=-2m=-1
m=0
Advantage: • Cavity finesse is limited by specular reflectivity (>99.99% seems possible)• Low diffraction efficiency• Shallow structures• Low scattering loss
5Aspen, 21.01.2005, Roman Schnabel
Coupler / 2nd Order Littrow
Grating equation:
for d=1450 nm (grating period),=1064 nm, |m|=2.
2.47
sinsin
,Littin
min d
m
Shallow grating (40 to 50nm) structure with HR stack on top
in
Suggested design values for coupling amplitudes:
= 99%,
= 1%,
as small as possible,
(0°)=98%,no transmission at all, low loss
6Aspen, 21.01.2005, Roman Schnabel
Coupler / 2nd Order Littrow
Grating equation:
for d=1450 nm (grating period),=1064 nm, |m|=2.
2.47
sinsin
,Littin
min d
m
Shallow grating (40 to 50nm) structure with HR stack on top
in
Measured (+measurement inferred) values for coupling amplitudes:
≈ 99.4%,
≈ 0.58%,
≈ 0.005%,
(0°) ≈ 98.8%,Overall loss@0° ≈ 0.04%
7Aspen, 21.01.2005, Roman Schnabel
Measured (+measurement inferred) values for coupling amplitudes:
≈ 99.4%,
≈ 0.58%,
≈ 0.005%,
(0°) ≈ 98.8%,Overall loss@0° ≈ 0.04%
Coupler / 2nd Order Littrow
Grating equation:
for d=1450 nm (grating period),=1064 nm, |m|=2.
2.47
sinsin
,Littin
min d
m
Shallow grating (40 to 50nm) structure with HR stack on top
in
A 3-port coupler!
8Aspen, 21.01.2005, Roman Schnabel
Coupler / 2nd Order Littrow
Grating equation:
for d=1450 nm (grating period),=1064 nm, |m|=2.
2.47
sinsin
,Littin
min d
m
in
From >0, >0 and time reversal
consideration one can deduce >0!
What is the lowest possible?
Measured (+measurement inferred) values for coupling amplitudes:
≈ 99.4%,
≈ 0.58%,
≈ 0.005%,
(0°) ≈ 98.8%,Overall loss@0° ≈ 0.04%
A 3-port coupler!
9Aspen, 21.01.2005, Roman Schnabel
FP-Cavity: Coupled 2nd Order Littrow
Cavity free spectral rangeFinesse: F=400
A. Bunkowski et al., Opt. Lett. 29, 2342, (2004)
≈ 0.58%,
(0°)≈ 98.8%,Overall loss@0°≈ 0.04%
10Aspen, 21.01.2005, Roman Schnabel
Coupling Relations of the 2-Port (transmissive) Beamsplitter
a1 a2
b1 b2
b1
b2
S11 S12
S21 S22
a1
a2
,
5S 2 p
*5
S 2 p
5
S 2 p
5S 2p
ii
or
ai ,bi : complex field amplitudes
11Aspen, 21.01.2005, Roman Schnabel
Coupling Relations of the 3-Port (reflective) Beamsplitter
b1
b2
b3
2ei2 1e
i2 0ei0
1ei1 0e
i0 1ei1
0ei0 1e
i1 2ei2
a1
a2
a3
,5
S 3p*
5S 3 p
0
2 212 1
02 1
2 22 1
1 0 2
2 1 0
2and
a1
a2
b1 b3
a3
b2
in
12Aspen, 21.01.2005, Roman Schnabel
Coupling Relations of the 3-Port (reflective) Beamsplitter
and
a1
a2
b1 b3
a3
b2
0 0
1 1/2 arccos 12 20
2 / 200 2 arccos 1
2 / 220
b1
b2
b3
2ei2 1e
i2 0ei0
1ei1 0e
i0 1ei1
0ei0 1e
i1 2ei2
a1
a2
a3
,5
S 3p*
5S 3 p
0
2 212 1
02 1
2 22 1
1 0 2
2 1 0
2
13Aspen, 21.01.2005, Roman Schnabel
3-Port Coupled FP Cavity
c1
c2
c3
5S 3p
1
c2 exp(2i)
0
,
c1 2 exp(i2) 12 exp 2i(1 ) d
c2 1 exp(i1)d
c3 0 12 exp 2i(1 ) d
d 1
0 exp 2i
a1=1
c1 c3
c2
14Aspen, 21.01.2005, Roman Schnabel
= min
c1
c3
c2
> min
c1
c3
c2
3-Port Coupled FP Cavity a1=1
c1 c3
c2
15Aspen, 21.01.2005, Roman Schnabel
3-Port Coupled FP Cavity a1=1
c1 c3
c2
Gratings with minimum 2 provide a dark port (c3=0) for a tuned cavity and enables power recycling.
16Aspen, 21.01.2005, Roman Schnabel
Summary
• A low loss reflective coupler to a cavity of Finesse 400 has been demonstrated.
• Phase relations of the three-port coupler are understood.
• Our results show that low efficiency, 3-port gratings are very promissing for high power interferometers.
17Aspen, 21.01.2005, Roman Schnabel
All-reflective Grating IFO
Proposed by R. Drever
18Aspen, 21.01.2005, Roman Schnabel
3-Port Coupled FP Cavity a1=1
c1 c3
c2