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LSC meeting at LLO, March 2005 1 LIGO- G050195-00-R Advanced LIGO optical configuration investigated in 40meter prototype LSC meeting at LLO Mar. 22, 2005 O. Miyakawa, Caltech and the 40m collaboration

Advanced LIGO optical configuration investigated in 40meter prototype LSC meeting at LLO

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Advanced LIGO optical configuration investigated in 40meter prototype LSC meeting at LLO Mar. 22, 2005 O. Miyakawa, Caltech and the 40m collaboration. Caltech 40 meter prototype interferometer. Objectives - PowerPoint PPT Presentation

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Page 1: Advanced LIGO optical configuration investigated in 40meter prototype LSC meeting at LLO

LSC meeting at LLO, March 2005 1LIGO- G050195-00-R

Advanced LIGO optical configuration

investigated in 40meter prototype

LSC meeting at LLOMar. 22, 2005

O. Miyakawa, Caltechand the 40m collaboration

Page 2: Advanced LIGO optical configuration investigated in 40meter prototype LSC meeting at LLO

LSC meeting at LLO, March 2005 2LIGO- G050195-00-R

Caltech 40 meter prototype interferometer

Objectives Develop lock acquisition procedure of detuned Resonant Sideband

Extraction (RSE) interferometer, as close as possible to Advanced LIGO optical design

BSPRM SRM

X arm

Darkport

Brightport

Y arm

Characterize noise mechanisms Verify optical spring and optical

resonance effects Develop DC readout scheme

Next Rob’s talk Extrapolate to AdLIGO via

simulation etc.

Page 3: Advanced LIGO optical configuration investigated in 40meter prototype LSC meeting at LLO

LSC meeting at LLO, March 2005 3LIGO- G050195-00-R

Important Milestones

20032003Installation of Four TMs and BS:doneLock of FP Michelson :done

20042004Installation of Power Recycling Mirror (PRM) ,Signal Recycling Mirror (SRM) :done Installation Mach-Zehnder to eliminate sideband of sideband :doneDRMI locked with carrier resonance using dither for Michelson DOF. :doneDRMI locked with sideband resonance using Double Demodulation(DDM) :doneOff-resonant lock of signal arm cavity with DRMI :doneOff-resonant lock of both arm cavities with DRMI :doneFull carrier resonant of single arm with DRMI :done

20052005Full RSE :in progress

Arm lock is really really difficult!Arm lock is really really difficult!

Page 4: Advanced LIGO optical configuration investigated in 40meter prototype LSC meeting at LLO

LSC meeting at LLO, March 2005 4LIGO- G050195-00-R

DRMI lock withUnbalanced 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

Lock acquisition After lock: MICH : dither @ 1200 Hz DDM@AP PRC : 33MHz@SP DDM@SP SRC : DDM@PO DDM@PO

Typical lock acquisition time : ~10secLongest lock:2.5hour

Page 5: Advanced LIGO optical configuration investigated in 40meter prototype LSC meeting at LLO

LSC meeting at LLO, March 2005 5LIGO- G050195-00-R

SP33,DDM,+/-33M,+/-166M@SP

DesignLockpoint

SP33Lockpoint0.56 degree (1.7nm)

+166resonant

+/-33 resonant

+/-33 off-resonant

Page 6: Advanced LIGO optical configuration investigated in 40meter prototype LSC meeting at LLO

LSC meeting at LLO, March 2005 6LIGO- G050195-00-R

40m Original design of SP DDM

DesignLockpoint

SP33Lockpoint0.56degree

+166resonance

+33resonance

0 50 100 150 200 250 300 3500

50

100

150

200

250

300

350

Demodulation Phase of f1

Dem

odul

atio

n P

hase

of f

2

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

-0.2

-0.1

-0.1

-0.1

-0.1

-0.1

-0.1

-0.1

-0.1

0

00

0

00

00

00

0

0.1

0.1

0.10.1

0.10.1

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

-0.0

3

-0.03

-0.02

-0.02

-0.0

2

-0.02

-0.02

-0.0

2

-0.02-0

.02

-0.0

1

-0.01

-0.01

-0.0

1

-0.01

-0.0

1

-0.01-0

.01

-0.01

0

0

0

0

0

0

0

0

0

0

0.01

0.010.

01

0.01

0.01

0.010.

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

0.03

0.03

0.04

0.04

0.04

0.04

-0.1 -0.1-0.1

-0.1

-0.05

-0.0

5

-0.05

-0.05

-0.05

-0.05

-0.050

0 0

0

0

0

0

0

0

0

0

0

0

0.05

0.05

0.05

0.05

0.05

0.05

0.05

0.1

0.1

0.1

0.1

dc=0l+l-ls

+33 : off-resonant-33 : off-resonant+166: resonant-166 : anti-resonant

• l+ and ls plot separated

• Difficult to find PRM position without carrier

Page 7: Advanced LIGO optical configuration investigated in 40meter prototype LSC meeting at LLO

LSC meeting at LLO, March 2005 7LIGO- G050195-00-R

Offset l+ +0.56 deg, ls +0.56 deg

DesignLockpoint

SP33Lockpoint0.56degree

+166resonance

+33resonance

0 50 100 150 200 250 300 3500

50

100

150

200

250

300

350

Demodulation Phase of f1

Dem

odul

atio

n P

hase

of f

2

Double Demodulation at SP

-0.3

-0.3

-0.3

-0.3

-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

00

0

0

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

0.3

0.3

0.3

0.3

-0.06

-0.06

-0.06

-0.04

-0.0

4

-0.0

4

-0.04

-0.04

-0.0

4

-0.04-0

.02

-0.02

-0.02

-0.0

2

-0.02

-0.02

-0.0

2

-0.02

-0.0

2

0

0

0

0

0

0

0

0

0

0

0.02

0.02

0.02

0.02

0.02

0.02

0.02

0.02

0.04

0.04

0.04

0.04

0.04

0.040.04

0.06

0.06

0.06

0.06

-0.1

-0.1

-0.05

-0.0

5

-0.05

-0.05

-0.05

-0.0

5

0

0

0

0

00

0

0

00

0

0

0.05

0.05

0.05

0.05

0.05

0.050.05

0.1

0.1

dc=0l+l-ls

+33 : resonant-33 : resonant+166: resonant-166 : anti-resonant

• l+ and ls plot overlapping

• DC line changed• Easy to find PRM

position using 33MHz resonance

• Like AdLIGO configuration

• Carrier would be off resonant

Page 8: Advanced LIGO optical configuration investigated in 40meter prototype LSC meeting at LLO

LSC meeting at LLO, March 2005 8LIGO- G050195-00-R

40m vs. Ad-LIGO

40m

Ad-LIGO

x6

x2

x3x1.5

x8x17

Page 9: Advanced LIGO optical configuration investigated in 40meter prototype LSC meeting at LLO

LSC meeting at LLO, March 2005 9LIGO- G050195-00-R

Struggling lock acquisition for Arms

Problems

1. Sideband resonance on arm cavities

2. Resonant point shift due to detuned SRC

3. 16kHz sampling rate is too slow for 40m.

4. Coupling between X arm and Y arm

Page 10: Advanced LIGO optical configuration investigated in 40meter prototype LSC meeting at LLO

LSC meeting at LLO, March 2005 10LIGO- G050195-00-R

Which is first ? DRMI lock or Arms lock?

ITMy

ITMxBSPRM

SRM

ETMx

ETMy

• Carrier flash does not matter because DRMI is locked by DDM (beat of sidebands).

• Sideband flash matters.• Can keep locking ~10sec with

lower gain.ITMy

ITMxBSPRM

SRM

ETMx

ETMy

Shutter

Shutter

ETMx

ITMy

ITMxBSPRM

SRM

ETMy

Sideband resonance

Shutter

Shutter

Carrier33MHz166MHz

ITMy

ITMxBSPRM

SRM

ETMx

ETMy

DRMI first

Arms first•PRFPMI : succeeded•RSE : not succeeded!

»Because of resonant point shift due to detuned SRC

Normalized byPRC power

DDM

Page 11: Advanced LIGO optical configuration investigated in 40meter prototype LSC meeting at LLO

LSC meeting at LLO, March 2005 11LIGO- G050195-00-R

Resonant point shift

6x10-2

5

4

3

2

1

0

Nor

mal

ized

tra

nsm

itted

pow

er a

s in

put

[W]

-0.4 -0.2 0.0 0.2 0.4

CARM (XARM) [10-9

m]

Full RSEDRMI + X arm

Resonant point shift • Resonant point shifts in single arm lock because of carrier phase change in detuned SRC

Page 12: Advanced LIGO optical configuration investigated in 40meter prototype LSC meeting at LLO

LSC meeting at LLO, March 2005 12LIGO- G050195-00-R

Digital sampling for 40m RSE configuration

1.0x10-1

0.8

0.6

0.4

0.2

0.0

Nor

mal

ized

pow

er a

s in

put[

W]

-0.4 -0.2 0.0 0.2 0.4

Mirror position [10-9

m]

Full RSEDigital sampling points

with 3x10-6

m@1Hz

Digital sampling with arm transmitted light for RSE• Due to large seismic

motion, 3x10-6m at 1Hz assumed here

• Due to very high combined finesse of arm and PRC ~18000.

• Night is about 10 times better but still not enough.

• Needs wider linear error signal.

» Normalization technique to widen linear range

» Slower mirror motion

Page 13: Advanced LIGO optical configuration investigated in 40meter prototype LSC meeting at LLO

LSC meeting at LLO, March 2005 13LIGO- G050195-00-R

Error signal is produced by transmitted light as

1. to avoid coupling through carrier in central part,

2. to widen linear range.

Off-resonant lock scheme for arm cavity

Off-resonantLock point

Resonant Lock

offsetpower dTransmitte

1

Page 14: Advanced LIGO optical configuration investigated in 40meter prototype LSC meeting at LLO

LSC meeting at LLO, March 2005 14LIGO- G050195-00-R

Off resonant Arm lock with DRMI

DRMI with single arm lockDRMI with single arm lock Not so difficultNot so difficult Last ~10 minLast ~10 min Lock acquisition time ~1 Lock acquisition time ~1

minmin Switched to POX/POY Switched to POX/POY

signal normalized by signal normalized by transmitted light transmitted light

Full carrier was stored in Full carrier was stored in each arm cavity separately.each arm cavity separately.

Both arms lock with DRMIBoth arms lock with DRMI Off-resonant carrier on arm Off-resonant carrier on arm

cavitiescavities Last < 1 minLast < 1 min Locked only 2 timesLocked only 2 times

Yarm lockXarm lock

Arm power

Error signal

Ideal lockpoint

Offset lockOffset lock

Page 15: Advanced LIGO optical configuration investigated in 40meter prototype LSC meeting at LLO

LSC meeting at LLO, March 2005 15LIGO- G050195-00-R

Coupling between Lx and Ly

Laser

ETMy

ETMx

ITMy

ITMxBSPRM

SRM

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.

Lx Ly l l l s

SP f1 1 9.4E-1 -1.2E-3 -1.3E-6 -2.3E-6

AP f2 9.4E-1 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

POX/POY lock

Common of arms(CARM)Differential of arms(DARM)Power recycling cavityMichelsonSignal recycling cavity

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

CARM/DARM lock

• Coupling is 94% when carrier is resonant.

» Off-resonant lock for arms

POX

POY

Page 16: Advanced LIGO optical configuration investigated in 40meter prototype LSC meeting at LLO

LSC meeting at LLO, March 2005 16LIGO- G050195-00-R

The way to RSE

DRMI lock first using DDM

Full RSE lock

Both arms lock with offsetusing transmitted light

Arm lock first with offsetusing transmitted light

Switch to POX/POYsignal with the offset

Reduce offset

Switch to CARM/DARMsignal with the offset

Resonantpoint shift

Coupling betweenLx and Ly

Clear samplingProblem and

linear range problem

Page 17: Advanced LIGO optical configuration investigated in 40meter prototype LSC meeting at LLO

LSC meeting at LLO, March 2005 17LIGO- G050195-00-R

Way from off-resonant lock to com/diff lock

Off-resonantLock point

+/-0.2nm10

-5

10-4

10-3

10-2

10-1

Nor

mal

ized

tra

nsm

itted

pow

er a

s in

put

[W]

-0.4 -0.2 0.0 0.2 0.4

CARM (XARM) [10-9

m]

Full RSEFPMI(PRC,SRC misaligned)

RSE vs FPMI

Page 18: Advanced LIGO optical configuration investigated in 40meter prototype LSC meeting at LLO

LSC meeting at LLO, March 2005 18LIGO- G050195-00-R

Normalized SP166 for CARM

Dem.phase accuracy~10degre for 166MHz~0.1degree for 33MHz

Off-resonantLock point

+/-0.2nm10

-5

10-4

10-3

10-2

10-1

No

rma

lized

tra

nsm

itte

d p

ow

er

as

inp

ut

[W]

-0.4 -0.2 0.0 0.2 0.4

CARM (XARM) [10-9

m]

-0.2

-0.1

0.0

0.1

0.2

Full RSEFPMI(PRC,SRC misaligned)Raw error signal of SP166SP166 normalized by (TrX + TrY)SP166 normalized by PRC power

Normarized SP166

Page 19: Advanced LIGO optical configuration investigated in 40meter prototype LSC meeting at LLO

LSC meeting at LLO, March 2005 19LIGO- G050195-00-R

e2e SIMULATION: 4Om/AdvLIGO package optical configuration

IFO Central partIFO with Arms

ETMY

ETMX

PRM

ITMX

SRM

ITMY

BS

Page 20: Advanced LIGO optical configuration investigated in 40meter prototype LSC meeting at LLO

LIGO- G050195-00-R

e2e SIMULATION: 4Om/AdvLIGO package

Example:DARM @ AP 166 MHz

TWIDDLE and E2E comparison

• E2E validation of DC fields comparing with TWIDDLE

results: good agreement !

• E2E transfer functions simulations (and comparison with TWIDDLE ones) of DOF at SP, AP and PO shaking the end mirrors with white noiseat different demodulation frequencies : (33,133,166,199) MHz

I signal

Q signal

TWIDDLE

E2E

TWIDDLE

E2E