amaldi conference, june 2005 1 lock acquisition scheme for the advanced ligo optical configuration...
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Amaldi conference, June 2005 1
Lock acquisition schemefor the Advanced LIGO
optical configuration
Amaldi conferenceJune24, 2005
O. Miyakawa, Caltechand the 40m collaboration
Amaldi conference, June 2005 2
Caltech 40 meter prototype interferometer
Objectives Develop lock acquisition procedure of detuned Resonant Sideband
Extraction (RSE) interferometer, as close as possible to AdLIGO optical design
BSPRM SRM
X arm
Darkport
Brightport
Y arm
Characterize noise mechanisms Verify optical spring and optical
resonance Develop DC readout scheme Extrapolate to AdLIGO via
simulation
Amaldi conference, June 2005 3
AdLIGO signal extraction scheme
Arm cavity signals are extracted from beat between carrier and f1 or f2.
Central part (Michelson, PRC, SRC) signals are extracted from beat between f1 and f2, not including arm cavity information.
f1-f1 f2-f2
Carrier (Resonant on arms)
• Single demodulation• Arm information
• Double demodulation• Central part information
Mach-Zehnder will be installed to eliminate sidebands of sidebands.
Only + f2 is resonant on SRC. Unbalanced sidebands of +/-f2 due
to detuned SRC produce good error signal for Central part.
ETMy
ETMx
ITMy
ITMxBSPRM
SRM
4km
4k
mf2
f1
Amaldi conference, June 2005 4
5 DOF for length control
: L=( Lx Ly) / 2
: L= Lx Ly
: l=( lx ly) / 2
=2.257m: l= lx ly = 0.451m
: ls=( lsx lsy) / 2
=2.15m
Port Dem. Freq.
L L l l l s
SP f1 1 -3.8E-9 -1.2E-3 -1.3E-6 -2.3E-6
AP f2 -4.8E-9 1 1.2E-8 1.3E-3 -1.7E-8
SP f1 f2 -1.7E-3 -3.0E-4 1 -3.2E-2 -1.0E-1
AP f1 f2 -6.2E-4 1.5E-3 7.5E-1 1 7.1E-2
PO f1 f2 3.6E-3 2.7E-3 4.6E-1 -2.3E-2 1
Signal Extraction Matrix (in-lock)
Common of armsDifferential of armsPower recycling cavity
MichelsonSignal recycling cavity
Laser
ETMy
ETMx
ITMy
ITMxBS
PRM
SRM
SPAP
PO
lx
ly
lsx
lsy
Lx =38.55m
Finesse=1235
Ly=38.55m
Finesse=1235Phase Modulationf1=33MHzf2=166MHz
T =7%
T =7%
GPR=14.5
Amaldi conference, June 2005 5
Differences betweenAdvLIGO and 40m prototype
100 times shorter cavity length Arm cavity finesse at 40m chosen to be = to AdvLIGO ( = 1235 )
» Storage time is x100 shorter.
Control RF sidebands are 33/166 MHz instead of 9/180 MHz» Due to shorter PRC length, less signal separation.
LIGO-I 10-watt laser, negligible thermal effects» 180W laser will be used in AdvLIGO.
Noisier seismic environment in town, smaller stack» ~1x10-6m at 1Hz.
LIGO-I single pendulum suspensions are used» AdvLIGO will use triple (MC, BS, PRM, SRM) and quad (ITMs, ETMs)
suspensions.
Amaldi conference, June 2005 6
Lock acquisition procedure towards detuned RSE
ITMy
ITMxBSPRM
SRM
ETMx
ETMy
Shutter
Shutter
Carrier33MHz166MHz
DRMI using DDM Off-resonantarms using DC lock
(POX/TrX),(POY/TrY)
SP166/PRC,AP166/PRC
(POX/TrX) + (POY/TrY), (POX/TrX) – (POY/TrY)
(TrX + TrY), (TrX – TrY) / (TrX + TrY)
Ideas for armcontrol signal
RSE
Done In progressDone
Amaldi conference, June 2005 7
DRMI lock using double demodulation with unbalanced sideband by detuned cavity
August 2004August 2004DRMI locked with carrier resonance (like GEO configuration)DRMI locked with carrier resonance (like GEO configuration)November 2004November 2004DRMI locked with sideband resonance (Carrier is anti resonant preparing for RSE.)DRMI locked with sideband resonance (Carrier is anti resonant preparing for RSE.)
Carrier
33MHz
Unbalanced166MHz
Belongs tonext carrier
Belongs tonext carrier
Carrier33MHz166MHz
ITMy
ITMxBS
PRM
SRM
OSA DDM PD
DDM PD
DDM PD
Typical lock acquisition time : ~10secLongest lock : 2.5hour
Amaldi conference, June 2005 8
Struggling lock acquisition for arm cavities
Problems
1. High recycling gain of ~15 produces 94% coupling between two arms.
2. Very high coupled finesse of ~18000.
3. Slow sampling rate of 16kHz for direct lock acquisition.
So, we have two steps
1. Each arm lock using transmitted light with DC offset. …done
2. Reduce offset to have full resonance of carrier. …in progress
Amaldi conference, June 2005 9
• Error signal is produced by only transmitted light as
• Smaller coupling• Wider linear range than RF error signal.
Off-resonant DC lock scheme for arm cavity
Off-resonantLock point
Resonant Lock
offsetpower dTransmitte
1
Amaldi conference, June 2005 10
All 5 degrees of freedom under controlledwith DC offset on L+ loop
Both arms locked with DRMIBoth arms locked with DRMI Lock acquisition time ~1 minLock acquisition time ~1 min Lasts ~ 20 minLasts ~ 20 min Can be switched to Can be switched to
common/differential controlcommon/differential controlLL- : AP166 with no offset- : AP166 with no offsetLL+ : Trx+Try with DC offset+ : Trx+Try with DC offset
Yarm lockXarm lock
Arm power
Error signal
Ideal lockpoint
Offset lockOffset lock
Have started trying toreduce offset from L+ loop
But…
Amaldi conference, June 2005 11
Peak changing due to reduction of offset
• Peak started from 1.6kHz and reached to ~450H.
• This peak introduces phase delay around unity gain frequency.
Amaldi conference, June 2005 12
CARM at 218 pm offset (~locking point)
-100
-90
-80
-70
-60
-50
-40
-30
-20
-10
0
1 10 100 1000 10000 100000-200
-150
-100
-50
0
50
100
150
200
dB
Ph
as
e [
De
g]
f [Hz]
CARM optical response, CARM offset at 218 pm
SP33I n1 : dB SP33I n1 : Phase [Deg]
NPTRX n5 : dB NPTRX n5 : Phase [Deg]
UnityGainFrequency
Amaldi conference, June 2005 13
CARM at 118 pm offset
-100
-80
-60
-40
-20
0
20
1 10 100 1000 10000 100000-200
-150
-100
-50
0
50
100
150
200
dB
Ph
as
e [
De
g]
f [Hz]
CARM optical response, CARM offset by 118 pm
SP33I n1 : dB SP33I n1 : Phase [Deg]
NPTRX n5 : dB NPTRX n5 : Phase [Deg]
UnityGainFrequency
Amaldi conference, June 2005 14
CARM offset at 59 pm (losing lock)
-100
-80
-60
-40
-20
0
20
40
1 10 100 1000 10000 100000-200
-150
-100
-50
0
50
100
150
200
dB
Ph
as
e [
De
g]
f [Hz]
CARM optical response, CARM offset by 59 pm
SP33I n1 : dB SP33I n1 : Phase [Deg]
NPTRX n5 : dB NPTRX n5 : Phase [Deg]
UnityGainFrequency
Amaldi conference, June 2005 15
L- optical gain with RSE peak
•Optical gain of L- loopDARM_IN1/DARM_OUT,divided by pendulum transfer function
• No offset on L- loop• 150pm offset on L+ loop
•Optical resonance of detuned RSE can be seen around the design RSE peak of 4kHz.•Q of this peak is about 6.
Design RSEpeak ~ 4kHz
Amaldi conference, June 2005 16
DARM, operating point
-40
-30
-20
-10
0
10
20
30
40
50
60
1 10 100 1000 10000 100000 0
20
40
60
80
100
120
140
160
180
dB
Ph
ase
[D
eg
]
f [Hz]
DARM optical response, CARM at 218 pm offset
APGW n2 : dB APGW n2 : Phase [Deg]
NPTRX n5 : dB NPTRX n5 : Phase [Deg]
Amaldi conference, June 2005 17
Summary
All 5DOFs are locked with some offset on L+. RSE detuning peak was seen. L+ loop has a detuning peak with DC offset and it
introduces phase delay around unity gain frequency with reducing offset.
Fortunately, Advanced LIGO will not have L+ peak problem !
Cavity pole of single arm is around 16Hz from the beginning, far below from unity gain frequency of L+ loop around 300Hz.
Fast frequency control or proper compensative digital filter may fix this problem for 40m.
Hope we succeed in locking full RSE very soon!
Amaldi conference, June 2005 18
DC Readout at the 40m DC Readout eliminates several sources of technical noise
(mainly due to the RF sidebands): – Oscillator phase noise – Effects of unstable recycling cavity. – The arm-filtered carrier light will serve as a heavily
stabilized local oscillator. – Perfect spatial overlap of LO and GW signal at PD.
DC Readout has the potential for QND measurements, without major modifications to the IFO.
We can use a 3 or 4-mirror OMC to reject RF sidebands.» Finesse ~ 500, In-vacuum, on a seismic stack.
The DC Detection diode» an aluminum stand to hold a bare photodiode, and
verified that the block can radiate 100 mW safely.
from SRM
From SRM