Albert-Einstein-Institute Hannover ET filter cavities for third generation detectors Keiko Kokeyama Andre Thüring
Feb 23, 2016
Albert-Einstein-InstituteHannover
ET filter cavitiesfor third generation detectors
Keiko KokeyamaAndre Thüring
Albert-Einstein-InstituteHannover
Contents
• Introduction of Filter cavities for ET
Part1. Filter-cavity-length requirement
- Frequency dependant squeezing
- Filter cavity length and the resulting squeezing level
Part2. Layout requirement from the scattering light analysis
• SummaryK. Kokeyama and Andre Thüring 17 May 2010, GWADW
Albert-Einstein-InstituteHannover
Contents
• Introduction of Filter cavities for ET
Part1. Filter-cavity-length requirement
- Frequency dependant squeezing
- Filter cavity length and the resulting squeezing level
Part2. Layout requirement from the scattering light analysis
• SummaryK. Kokeyama and Andre Thüring 17 May 2010, GWADW
Albert-Einstein-InstituteHannover
Design sensitivity for ET-C
Lets focus on the ET-C LF
part.
ET-C : Xylophone consists ofET-LF and ET-HF
ET-C LF• Low frequency part of the xylophone• Detuned RSE• Cryogenic• Silicon test mass & 1550nm laser• HG00 mode
1/20
S. Hild et al. CQG 27 (2010) 015003
K. Kokeyama and Andre Thüring 17 May 2010, GWADW
Albert-Einstein-InstituteHannover
To reach the targeted sensitivity, we have to utilize squeezed states of light
We dream of a broadband
QN-reduction by 10dB
A broadband quantum noise reduction requires the frequency dependent squeezing,
therefore filter cavities are necessary
2/20K. Kokeyama and Andre Thüring 17 May 2010, GWADW
Albert-Einstein-InstituteHannover
Contents
• Introduction of Filter cavities for ET
Part1. Filter-cavity-length requirement
- Frequency dependant squeezing
- Filter cavity length and the resulting squeezing level
Part2. Layout requirement from the scattering light analysis
• SummaryK. Kokeyama and Andre Thüring 17 May 2010, GWADW
Albert-Einstein-InstituteHannover
Contents
• Introduction of Filter cavities for ET
Part1. Filter-cavity-length requirement
- Frequency dependant squeezing
- Filter cavity length and the resulting squeezing level
Part2. Layout requirement from the scattering light analysis
• SummaryK. Kokeyama and Andre Thüring 17 May 2010, GWADW
Albert-Einstein-InstituteHannover
Quantum noise in a Michelson interferometer
X1
X2
X1
X2
Quantum noise reduction with squeezed light
X1
X2
Filter cavities can optimize the squessing angles
3/20K. Kokeyama and Andre Thüring 17 May 2010, GWADW
Albert-Einstein-InstituteHannover
ET-C LF bases on detuned signal-recycling
Optical spring resonance
Optical resonance
Two filter cavities are required for an optimum generation of frequency dependent squeezing
In this talk we consider the two input filter
cavities
4/20K. Kokeyama and Andre Thüring 17 May 2010, GWADW
Albert-Einstein-InstituteHannover
Contents
• Introduction of Filter cavities for ET
Part1. Filter-cavity-length requirement
- Frequency dependant squeezing
- Filter cavity length and the resulting squeezing level
Part2. Layout requirement from the scattering light analysis
• SummaryK. Kokeyama and Andre Thüring 17 May 2010, GWADW
Albert-Einstein-InstituteHannover
Requirements defined by the interferometer set-up:
The bandwidths and detunings of the filter cavities
What we can choose
The lengths of the filter cavities
Limitations
Infrastructure, optical loss (e.g. scattering) , phase noise, ...
...And the optical layout (Part2)
5/20K. Kokeyama and Andre Thüring 17 May 2010, GWADW
Albert-Einstein-InstituteHannover
Degrading of squeezing due to optical loss
A cavity reflectance R<1 means loss . The degrading of squeezing is then frequency dependent
At every open (lossy) port vacuum noise couples in
couplingmirror
6/20K. Kokeyama and Andre Thüring 17 May 2010, GWADW
Albert-Einstein-InstituteHannover
The impact of intra-cavity loss
There exists a lower limit Lmin. For L < Lmin the filter cavity is under-coupled and the compensation of the phase-space rotation fails!
The filter‘s coupling mirror reflectance Rc needs to be chosen with respect to
1. the required bandwidth gaccounting for
2. the round-trip loss lRT 3. a given length L
7/20K. Kokeyama and Andre Thüring 17 May 2010, GWADW
Albert-Einstein-InstituteHannover
The impact of shortening the cavity length
Example for ET-C LFdetuning = 7.1 Hz 100 ppm round-trip loss,bandwidth = 2.1 Hz
If L < Lmin ~ 1136 m the filter is under-coupled and the filtering does not work
For L < 568m Rc needs to be >1
The filter cavity must be as long as possible for ET-LF
8/20K. Kokeyama and Andre Thüring 17 May 2010, GWADW
Albert-Einstein-InstituteHannover
Narrow bandwidths filter are more challenging
Assumptions:L = 10 km, 100 ppm round-trip loss,Detuning = 2x bandwidth
Filter cavities with a bandwidth greater than 10 Hz are comparatively easy to realize
9/20K. Kokeyama and Andre Thüring 17 May 2010, GWADW
Albert-Einstein-InstituteHannover
Exemplary considerations for ET-C LF
Filter I:g = 2.1 Hzfres = 7.1 Hz
Filter II:g = 12.4 Hzfres = 25.1 Hz
Filter I:L = 2 kmF = 17845Rc = 99.9748%
Filter I:L = 5 kmF = 7138Rc = 99.9220%
Filter I:L = 10 kmF = 3569Rc = 99.8341%
Filter II:L = 2 kmF = 3022Rc = 99.8023%
Filter II:L = 5 kmF = 1209Rc = 99.4915%
Filter II:L = 10 kmF = 604Rc = 98.9757%
15dB squeezing100ppm RT - loss7% propagation loss
10/20K. Kokeyama and Andre Thüring 17 May 2010, GWADW
Albert-Einstein-InstituteHannover
Contents
• Introduction of Filter cavities for ET
Part1. Filter-cavity-length requirement
- Frequency dependant squeezing
- Filter cavity length and the resulting squeezing level
Part2. Layout requirement from the scattering light analysis
• SummaryK. Kokeyama and Andre Thüring 17 May 2010, GWADW
Albert-Einstein-InstituteHannover
Stray light analysis for four designs
Which design is suitable for ET cavitiesfrom the point of view of the loss
due to stray lights?
Triangular - ConventionalLinear
Rectangular Bow-tie
11/20K. Kokeyama and Andre Thüring 17 May 2010, GWADW
Albert-Einstein-InstituteHannover
Scattering Angle and Fields
TriangularLinear
Rectangular Bow-tie
12/20K. Kokeyama and Andre Thüring 17 May 2010, GWADW
Albert-Einstein-InstituteHannover
# f0 f Scat field Scat power
Counter-propagating
1 Small 0 Rigorous field Large
2 Large 0 Rigorous field Small
3 Small Gauss tail small?
4 Large Spherical wave approx.
Small
Normal-propagating
5 Small Gauss tail small?
6 Large Spherical wave approx.
Small
Scattering Field Category
13/20K. Kokeyama and Andre Thüring 17 May 2010, GWADW
Albert-Einstein-InstituteHannover
# f0 f Scat field Scat power
Counter-propagating
1 Small 0 Rigorous field Large
2 Large 0 Rigorous field Small
3 Small Gauss tail small?
4 Large Spherical wave approx.
Small
Normal-propagating
5 Small Gauss tail small?
6 Large Spherical wave approx.
Small
Scattering Field Category
13/20K. Kokeyama and Andre Thüring 17 May 2010, GWADW
Albert-Einstein-InstituteHannover
#1
Counter-Propagating, Small f0, f~0
C1 =A<ETEM00•m(x,y) •E*TEM00>
Coupling factor
14/20K. Kokeyama and Andre Thüring 17 May 2010, GWADW
Albert-Einstein-InstituteHannover
# f0 f Scat field Scat power
Counter-propagating
1 Small 0 Rigorous field Large
2 Large 0 Rigorous field Small
3 Small Gauss tail small?
4 Large Spherical wave approx.
Small
Normal-propagating
5 Small Gauss tail small?
6 Large Spherical wave approx.
Small
Scattering Field Category
15/20K. Kokeyama and Andre Thüring 17 May 2010, GWADW
Albert-Einstein-InstituteHannover
#2
Counter-Propagating, Large f0, f=0
Coupling factor
C2= A<ETEM00•m(x,y) •E*TEM00>
15/20K. Kokeyama and Andre Thüring 17 May 2010, GWADW
Albert-Einstein-InstituteHannover
# f0 f Scat field Scat power
Counter-propagating
1 Small 0 Rigorous field Large
2 Large 0 Rigorous field Small
3 Small Gauss tail small?
4 Large Spherical wave approx.
Small
Normal-propagating
5 Small Gauss tail small?
6 Large Spherical wave approx.
Small
Scattering Field Category
16/20K. Kokeyama and Andre Thüring 17 May 2010, GWADW
Albert-Einstein-InstituteHannover
#3Counter-Propagating,Large f (at 2nd scat)
C3=<ETEM00tail •E*TEM00> C4 =<ESphe •E*TEM00>
#4Counter-Propagating,Small f (at 2nd scat)
16/20K. Kokeyama and Andre Thüring 17 May 2010, GWADW
Albert-Einstein-InstituteHannover
# f0 f Scat field Scat power
Counter-propagating
1 Small 0 Rigorous field Large
2 Large 0 Rigorous field Small
3 Small Gauss tail small?
4 Large Spherical wave approx.
Small
Normal-propagating
5 Small Gauss tail small?
6 Large Spherical wave approx.
Small
Scattering Field Category
17/20K. Kokeyama and Andre Thüring 17 May 2010, GWADW
Albert-Einstein-InstituteHannover
#5Normal-Propagating,Large f (at 2nd scat)
#6Normal-Propagating,Small f (at 2nd scat)
C5=<ETEM00tail •E*#TEM00> C6 =<ESphe •E*#
TEM00>
17/20K. Kokeyama and Andre Thüring 17 May 2010, GWADW
Albert-Einstein-InstituteHannover
K. Kokeyama and Andre Thüring 17 May 2010, GWADW
Liner Cavity
TriangularCavity
Rectangular Cavity
Bow-tie Cavity
#1 (big scat) 0 A•C1 0 4A•C1
#2 (small scat) 0 2A•C2 4A•C2 0
#3 (Gauss tail. cp) 0 0 2•C3 Negligible
#4 (sphe. cp) 0 0 2•C4 Negligible
#5 (Gauss tail. np) 0 0 2•C5 Negligible
#6 (sphe, np) 0 0 2•C6 Negligible
Total
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18/20
Albert-Einstein-InstituteHannover
Liner Cavity
TriangularCavity
Rectangular Cavity
Bow-tie Cavity
#1 (big scat) 0 A•C1 0 4A•C1
#2 (small scat) 0 2A•C2 4A•C2 0
#3 (Gauss tail. cp) 0 0 2•C3 Negligible
#4 (sphe. cp) 0 0 2•C4 Negligible
#5 (Gauss tail. np) 0 0 2•C5 Negligible
#6 (sphe, np) 0 0 2•C6 Negligible
Total
Preliminary Results
19/20K. Kokeyama and Andre Thüring 17 May 2010, GWADW
Albert-Einstein-InstituteHannover
• We have shown that the requirement of the filter-cavity length which can accomplish the necessary level of squeezing
• We have evaluated the amount of scattered light from the geometry alone to select the cavity geometries for arm and filter cavities for ET.
• As a next step coupling factors between each fields and the main beam should be calculated quantitatively so that total loss and coupling can be estimated.
• At the same time the cavity geometries will be compared with respect to astigmatism, length & alignment control method
Summary
20/20K. Kokeyama and Andre Thüring 17 May 2010, GWADW