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40m Progress, LSC meeting, Ma r. 2004 1 LIGO- G040081-00-R 40m Laboratory Upgrade Progress Report LSC meeting at LIGO Livingston observatory Osamu Miyakawa, Caltech LIGO-G040081-00-R 40m Team: A. Weinstein, S. Kawamura, M. Smith, S. Vass, B. Taylor, J. Heefner, B. Abbott, L. Goggin, F. Kawazoe, S. Sakata, and R. Ward

40 m Laboratory Upgrade Progress Report LSC meeting at LIGO Livingston observatory

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40 m Laboratory Upgrade Progress Report LSC meeting at LIGO Livingston observatory Osamu Miyakawa, Caltech LIGO-G040081-00-R 40m Team : A. Weinstein, S. Kawamura, M. Smith, S. Vass, B. Taylor, J. Heefner, B. Abbott, L. Goggin, F. Kawazoe, S. Sakata, and R. Ward. Objectives. - PowerPoint PPT Presentation

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Page 1: 40 m Laboratory Upgrade Progress Report LSC meeting at LIGO Livingston observatory

40m Progress, LSC meeting, Mar. 2004 1LIGO- G040081-00-R

40m Laboratory UpgradeProgress Report

LSC meeting at LIGO Livingston observatory

Osamu Miyakawa, Caltech

LIGO-G040081-00-R

40m Team:A. Weinstein, S. Kawamura, M. Smith, S. Vass, B. Taylor, J. Heefner, B. Abbott, L. Goggin, F. Kawazoe, S. Sakata, and R. Ward

Page 2: 40 m Laboratory Upgrade Progress Report LSC meeting at LIGO Livingston observatory

40m Progress, LSC meeting, Mar. 2004 2LIGO- G040081-00-R

Objectives

Develop lock acquisition procedure of detuned Resonant Sideband Extraction (RSE),

Characterize noise mechanism, Verify optical spring effect, Develop DC readout scheme, etc.

for Advanced LIGO, LCGT,

and other future GW detectors

Page 3: 40 m Laboratory Upgrade Progress Report LSC meeting at LIGO Livingston observatory

40m Progress, LSC meeting, Mar. 2004 3LIGO- G040081-00-R

Target Sensitivity ofAdvanced LIGO and 40m

Page 4: 40 m Laboratory Upgrade Progress Report LSC meeting at LIGO Livingston observatory

40m Progress, LSC meeting, Mar. 2004 4LIGO- G040081-00-R

Important Achievement (1)Installation of FP Michelson

September, 2003September, 2003

Four TMs and BS: installed

PSL

ETMy

ETMx

ITMy

ITMxBS

MC

Page 5: 40 m Laboratory Upgrade Progress Report LSC meeting at LIGO Livingston observatory

40m Progress, LSC meeting, Mar. 2004 5LIGO- G040081-00-R

Important Achievement (2)Lock Acquisition of FP Michelson

November 2003November 2003 FP Michelson locked Arms locked independently, and

switched to common/differential servo

Digitally controlled suspensions Finesse ~ 1200 Seismic motion ~ 10 - 100 times

noisier than LIGO site UGF ~ 300Hz (limited by A/D and

D/A speed)

~ POX

POY ITMX

ITMY

ETMX

ETMY

BS

SP

RF

PCLaser I

IQ

AP

QI

Page 6: 40 m Laboratory Upgrade Progress Report LSC meeting at LIGO Livingston observatory

40m Progress, LSC meeting, Mar. 2004 6LIGO- G040081-00-R

Important Achievement (3)Spectrum of FP Michelson

November ~ December 2003November ~ December 2003 Displacement spectrum obtained With all the whitening/de-whitening

filters (2 of 4 orders) ON No feedback to laser frequency 2 months noise hunting Noise is limited by electronic noise

of de-whitening filter and frequency noise.

10-17

10-16

10-15

10-14

10-13

10-12

10-11

10-10

10-9

Dis

pla

cem

en

t n

ois

e[m

/Hz1

/2]

101

2 3 4 5 6 7

102

2 3 4 5 6 7

103

2 3 4 5 6 7

104

Frequency[Hz]

11/14/2003 First sensitivity11/18/2003 Tuning alignment, servo11/19/2003 Whitening filter11/25/2003 100Hz oscillation12/23/2003 Dewhitening filter12/30/2003 Oscillation around UGF

Calibration signal

Displacement noise of 40m FPMI12/30/2003

De-whitening filterFrequency noise

Page 7: 40 m Laboratory Upgrade Progress Report LSC meeting at LIGO Livingston observatory

40m Progress, LSC meeting, Mar. 2004 7LIGO- G040081-00-R

Important Achievement (4)Installation of PRM and SRM

February 2004February 2004 Power Recycling Mirror (PRM) , Signal

Recycling Mirror (SRM) installed FPMI re-locked after installation

BSPRM SRM

X arm

Y arm

Darkport

Brightport

PSL

ETMy

ETMx

ITMy

ITMxBSPRM

SEM

MC

Page 8: 40 m Laboratory Upgrade Progress Report LSC meeting at LIGO Livingston observatory

40m Progress, LSC meeting, Mar. 2004 8LIGO- G040081-00-R

Other Achievements

Simple and reliable calibration for PSL frequency noise Mode matching

» ~ 1% tolerance

Estimation of loss on mirror» ~ 90ppm (design 35ppm)

Optical lever» Helped the installation of PRM and SRM

Input matrix of suspension Third Pockel’s-cell for 166MHz modulation Two peak photo detector (133MHz, 199MHz) for double demodulation Replacement of NPRO and re-alignment of power amplifier

» Total power ~12.5W

Page 9: 40 m Laboratory Upgrade Progress Report LSC meeting at LIGO Livingston observatory

40m Progress, LSC meeting, Mar. 2004 9LIGO- G040081-00-R

Signal Extraction Matrix

Laser

ETMy

ETMx

ITMy

ITMxBS

PRM

SEM

SPAP

PO

lx

ly

lsx

lsy

Lx

Ly

L=( Lx Ly)/2

L= Lx Ly

l=( lx ly)/2

l= lx ly

ls=( lsx lsy)/2

Port Dem. Freq.

Dem. Phase

L L l l l s

SP f1 10 1 -3.8E-9

-1.2E-3

-1.3E-6

-2.3E-6

AP f2 271 -4.8E-9

1 1.2E-8

1.3E-3

-1.7E-8

SP f1 f2 189,32

-1.7E-3

-3.0E-4

1 -3.2E-2

-1.0E-1

AP f1 f2 4,81 -6.2E-4

1.5E-3

7.5E-1

1 7.1E-2

PO f1 f2 164,12

3.6E-3

2.7E-3

4.6E-1

-2.3E-2

1

Calculated by FINESSE (A. Freise: http://www.rzg.mpg.de/~adf/)

PO: light from BS to ITMy

Page 10: 40 m Laboratory Upgrade Progress Report LSC meeting at LIGO Livingston observatory

40m Progress, LSC meeting, Mar. 2004 10LIGO- G040081-00-R

Length Tolerances

Acceptable cavity length deviations from the ideal points:

6 cm for l 3 mm for l

3 mm for ls

Direct length measurement for PRC and SRCError of the cavity length PR and SR ~ +/-1mm

Port Dem. Freq.

Dem. Phase

L L l l l s

SP f1 3341

-7.6E-9

-1.2E-3

-4.1E-6

-2.3E-6

AP f2 230 -1.3E-9

13.0E-

81.3E-

3-1.7E-

8

SP f1 f2

162,73

-6.5E-4

3.5E-4

1-5.6E-

21.3E-

1

AP f1 f2

173,218

1.5E-3

4.2E-4

-2.1 1-2.4E-

1

PO f1 f2

329,153

1.1E-3

2.7E-3

2.6-1.6E-

11

Example: Signal matrix with l deviation of 1 cm

S. Kawamura, “Signal Extraction Matrix of the 40m Detuned RSE Prototype”, LIGO-T040010-00-R (2004)

Page 11: 40 m Laboratory Upgrade Progress Report LSC meeting at LIGO Livingston observatory

40m Progress, LSC meeting, Mar. 2004 11LIGO- G040081-00-R

Double Demodulation

0 50 100 150 200 250 300 3500

50

100

150

200

250

300

350

Demodulation Phase of f1

Dem

odul

atio

n Pha

se o

f f2

Double Demodulation at SP- 0.4

- 0.4

-0.4

- 0.4

- 0.4

- 0.3

- 0.3

- 0.3

- 0.3

- 0.3

-0.3

- 0.3

- 0.2

- 0.2

- 0.2

- 0.2

- 0.2

- 0.2

- 0.2

- 0.1

- 0.1

- 0.1

- 0.1

- 0.1

-0.1

- 0.1

-0.1

0

0

0

0

0

0

0

0

0

0

0

0.1

0.1

0.1

0.1

0.1

0.1

0.1

0.1

0.1

0.2

0.2

0.2

0.2

0.2

0.2

0.2

0.2

0.3

0.3 0.3

0.3

0.3

0.3

0.4

0.4

0.4

0.4

- 0.04

- 0.04

- 0.04

- 0.04

- 0.03

-0.0

3

- 0.03

- 0.03

-0.03

- 0.03

- 0.02

- 0.02

- 0.0

2

- 0.02

- 0.02

- 0.02

- 0.02

-0.02

-0.0

1

- 0.01

-0.01

- 0.01

-0.01

-0.01

- 0.01

-0.0

1

- 0.01

0

0

0

0

0

0

0

0

0

0

0.01

0.01

0.01

0.01

0.01

0.01

0.01

0.01

0.01

0.02

0.02

0.02

0.02

0.02

0.02

0.02

0.02

0.03

0.03

0.03

0.03

0.030.03

0.04

0.04

0.04

0.04

- 0.1

- 0.1

- 0.1

- 0.1

-0.05

- 0.05

- 0.05

- 0.05

- 0.05

- 0.05

- 0.05

0

0 0

0

0

0

0

0

0

0

0

0

0

0.05

0.05

0.05

0.05

0.050.05

0.05

0.1

0.1

0.1

0.1

dc=0l+l-ls

Double Demodulation used for l+, l-, and ls

Demodulation phases optimized to suppress DC and to maximize desired signal[S.Kawamura, “Signal Extraction Matrix of the 40m Detuned RSE Prototype”, LIGO-T040010-00-R (2004)]

Page 12: 40 m Laboratory Upgrade Progress Report LSC meeting at LIGO Livingston observatory

40m Progress, LSC meeting, Mar. 2004 12LIGO- G040081-00-R

Lock Acquisition of Detuned RSE

Central part: not disturbed by lock status change of arm cavity Question: Not disturbed by flash of SBs or SBs of SBs in arms? Promising: TAMA using 3rd harmonic demodulation in PRFPMI

ETMy

ETMx

ITMy

ITMxBSPRM

SEM

2. lock arm cavities1. lock central part using beat signal between f1 and f2

Page 13: 40 m Laboratory Upgrade Progress Report LSC meeting at LIGO Livingston observatory

40m Progress, LSC meeting, Mar. 2004 13LIGO- G040081-00-R

Lock Acquisition of Central Part

Ideal Procedure: Lock one by one

[for example]

Step 1: Lock l+ robustly

Step 2: Lock l- robustly

Step 3: Lock ls

Find primary signal not disturbed by the other two DOFs Find secondary signal not disturbed by the residual DOF

ITMy

ITMxBSPRM

SEM

Step 1Step 2Step 3

Page 14: 40 m Laboratory Upgrade Progress Report LSC meeting at LIGO Livingston observatory

40m Progress, LSC meeting, Mar. 2004 14LIGO- G040081-00-R

Quality of l+ Signal (dc=0, l+:Max)

-150 -100 -50 0 50 100 150-0.01

-0.008

-0.006

-0.004

-0.002

0

0.002

0.004

0.006

0.008

0.01

l+

Erro

r Sign

al

No- arm detuned RSE, DDM at SP, phase1=189, phase2=33 (dc=0)

Err

or

sig.

Page 15: 40 m Laboratory Upgrade Progress Report LSC meeting at LIGO Livingston observatory

40m Progress, LSC meeting, Mar. 2004 15LIGO- G040081-00-R

l+@SP, no offset

Signals for f1 resonance appear

Page 16: 40 m Laboratory Upgrade Progress Report LSC meeting at LIGO Livingston observatory

40m Progress, LSC meeting, Mar. 2004 16LIGO- G040081-00-R

Dependence of l+ Signal on Demodulation Phases

-150 -100 -50 0 50 100 150-0.01

-0.008

-0.006

-0.004

-0.002

0

0.002

0.004

0.006

0.008

0.01

l+

Erro

r Sig

nal

No- arm detuned RSE, DDM at SP, phase1=189 (dc=0), phase2: swept

phase2=0phase2=32 (dc=0)phase2=60phase2=88 (symmetric)phase2=120phase2=150phase2=180

-150 -100 -50 0 50 100 150-5

-4

-3

-2

-1

0

1

2

3

4

5x 10- 3

l+

Erro

r Sig

nal

No- arm detuned RSE, DDM at SP, phase1:Swept, phase2=32 (symmetric)

phase1=180 (max)phase1=210phase1=240phase1=270phase1=300phase1=330phase1=360

88

Err

or s

ig.

Err

or s

ig.

Page 17: 40 m Laboratory Upgrade Progress Report LSC meeting at LIGO Livingston observatory

40m Progress, LSC meeting, Mar. 2004 17LIGO- G040081-00-R

Quality of l+ Signal (Symmetric, dc0)

-150 -100 -50 0 50 100 150-5

-4

-3

-2

-1

0

1

2

3

4

5x 10- 3

l+

Erro

r Sign

al

No- arm detuned RSE, DDM at SP, phase1=180, phase2=32 (symmetric)88

Err

or

sig.

Page 18: 40 m Laboratory Upgrade Progress Report LSC meeting at LIGO Livingston observatory

40m Progress, LSC meeting, Mar. 2004 18LIGO- G040081-00-R

l+@SP, Symmetric

Four SBs resonate at different points

Good signal obtained when +f2 resonates

Signal for –f2 resonance has an opposite polarity

Disturbed when +f2 and –f2 resonate at the same point

Signals for f1 resonance can be cancelled by proper DDM phases, which coincide with the phases for symmetric signal

Page 19: 40 m Laboratory Upgrade Progress Report LSC meeting at LIGO Livingston observatory

40m Progress, LSC meeting, Mar. 2004 19LIGO- G040081-00-R

l+ Signal lockable surface

• l+ lock points makes one surface

• Gain change<3

Page 20: 40 m Laboratory Upgrade Progress Report LSC meeting at LIGO Livingston observatory

40m Progress, LSC meeting, Mar. 2004 20LIGO- G040081-00-R

l+ Signal lockable surface

• Lock point surface covers pretty much (~80%) of all the l-, ls parameters

• Feedback l+ signal to laser frequency for fast locking (Feed around)

Page 21: 40 m Laboratory Upgrade Progress Report LSC meeting at LIGO Livingston observatory

40m Progress, LSC meeting, Mar. 2004 21LIGO- G040081-00-R

Quality of l- Signal

-150 -100 -50 0 50 100 150-1

-0.8

-0.6

-0.4

-0.2

0

0.2

0.4

0.6

0.8

1x 10- 3

l-

Erro

r Sign

al

No- arm detuned RSE, DDM at AP, phase1=4 , phase2=81 (dc=0)

Err

or

sig.

Page 22: 40 m Laboratory Upgrade Progress Report LSC meeting at LIGO Livingston observatory

40m Progress, LSC meeting, Mar. 2004 22LIGO- G040081-00-R

Dependence of l- Signal on ls

No good signal obtained except for ls around resonant

Page 23: 40 m Laboratory Upgrade Progress Report LSC meeting at LIGO Livingston observatory

40m Progress, LSC meeting, Mar. 2004 23LIGO- G040081-00-R

l- Signal Divided byAP signal with different Dem. Phase

-150 -100 -50 0 50 100 150

-1

-0.8

-0.6

-0.4

-0.2

0

0.2

0.4

0.6

0.8

1

x 10- 3

l-

Erro

r Sig

nal

No- arm detuned RSE, DDM at AP, phase1=96, phase2=81 (Symmetric)

-150 -100 -50 0 50 100 150-1

-0.8

-0.6

-0.4

-0.2

0

0.2

0.4

0.6

0.8

1x 10- 3

l-

Erro

r Sig

nal

No- arm detuned RSE, DDM at AP, phase1=4 , phase2=81 (dc=0)

Divided by

Hint: H. Grote at GEO

Err

or

sig

.

Err

or

sig

.

Page 24: 40 m Laboratory Upgrade Progress Report LSC meeting at LIGO Livingston observatory

40m Progress, LSC meeting, Mar. 2004 24LIGO- G040081-00-R

Dependence of Dividedl- Signal on ls

Page 25: 40 m Laboratory Upgrade Progress Report LSC meeting at LIGO Livingston observatory

40m Progress, LSC meeting, Mar. 2004 25LIGO- G040081-00-R

Dependence of Dividedl- Signal on l+

Page 26: 40 m Laboratory Upgrade Progress Report LSC meeting at LIGO Livingston observatory

40m Progress, LSC meeting, Mar. 2004 26LIGO- G040081-00-R

Quality of ls Signal

-150 -100 -50 0 50 100 150-0.1

-0.08

-0.06

-0.04

-0.02

0

0.02

0.04

0.06

0.08

0.1

ls

Erro

r Sign

al

No- arm detuned RSE, DDM at PO, phase1=164, phase2=12 (dc=0)

Err

or

sig.

Page 27: 40 m Laboratory Upgrade Progress Report LSC meeting at LIGO Livingston observatory

40m Progress, LSC meeting, Mar. 2004 27LIGO- G040081-00-R

Dependence of ls Signal on l+

No good signal obtained except for l+ around resonant

Page 28: 40 m Laboratory Upgrade Progress Report LSC meeting at LIGO Livingston observatory

40m Progress, LSC meeting, Mar. 2004 28LIGO- G040081-00-R

Looking for Good Signal …

Have tried many things, but not significant improvement… f1-dem, f2-dem Dither For l+:

Single sideband f2, AM f2

NR pm, am, single sideband f3:

(f2-f3)-dem, (f1+f3)-dem

On the surface of l+ For l-, ls:

Signal divided by the following:

2f1-dem, 2f2-dem, DDM with different dem phases, (f2-2f1)-dem

On the surface of l+

Page 29: 40 m Laboratory Upgrade Progress Report LSC meeting at LIGO Livingston observatory

40m Progress, LSC meeting, Mar. 2004 29LIGO- G040081-00-R

Summary

Lots of achievements; experiment on 40m going very fast and smoothly

Almost ready to try lock acquisition Lock acquisition: not so easy Need more investigation for lock acquisition

Hope we succeed in locking detuned RSE very soon!