ligo- g040310-00-r sensing and control, spie conference, june 2004 1 sensing and control of the...

17
Sensing and control, SPIE conference, June 2004 1 LIGO- G040310-00-R Sensing and control of the Advanced LIGO optical configuration SPIE conference at Glasgow June 23, 2004 O. Miyakawa, Caltech B. Abbott, R. Bork, P. Fritschel, L. Goggin, J. Heefner, A. Ivanov, S. Kawamura, F. Kawazoe, C. Mow-Lowry, A. Ourjoumtsev, S. Sakata, M. Smith, K. Strain, R. Taylor, D. Ugolini, S. Vass, R. Ward, A. Weinstein

Upload: matthew-gray

Post on 04-Jan-2016

214 views

Category:

Documents


1 download

TRANSCRIPT

Page 1: LIGO- G040310-00-R Sensing and control, SPIE conference, June 2004 1 Sensing and control of the Advanced LIGO optical configuration SPIE conference at

Sensing and control, SPIE conference, June 2004 1LIGO- G040310-00-R

Sensing and control ofthe Advanced LIGO optical

configuration

SPIE conference at GlasgowJune 23, 2004

O. Miyakawa, Caltech

B. Abbott, R. Bork, P. Fritschel, L. Goggin, J. Heefner, A. Ivanov,S. Kawamura, F. Kawazoe, C. Mow-Lowry, A. Ourjoumtsev, S. Sakata,

M. Smith, K. Strain, R. Taylor, D. Ugolini, S. Vass, R. Ward, A. Weinstein

Page 2: LIGO- G040310-00-R Sensing and control, SPIE conference, June 2004 1 Sensing and control of the Advanced LIGO optical configuration SPIE conference at

Sensing and control, SPIE conference, June 2004 2LIGO- G040310-00-R

Signal and power enhancement using Fabry-Perot cavity in each arm

Power enhancement using Power Recycling

Optical configuration forGravitational wave interferometer

Gravitational wave detection using Michelson interferometer

BS

FP cavity

FP

ca

vit

y

Laser

PRM

BS

FP cavity

FP

ca

vit

y

Laser

Page 3: LIGO- G040310-00-R Sensing and control, SPIE conference, June 2004 1 Sensing and control of the Advanced LIGO optical configuration SPIE conference at

Sensing and control, SPIE conference, June 2004 3LIGO- G040310-00-R

LIGO:Power recycled FPMI

» Optical noise is limited by Standard Quantum Limit (SQL)

AdvLIGO:GW signal enhancement using Detuned Resonant Sideband Extraction

» Can overcome the SQL QND detector

» Two dips by optical spring, detuning

Advanced LIGO optical configuratoin

Detuning

PRM

BS

FP cavity

FP

ca

vit

y

Laser

GW signal

Power

Standard Quantum Limit

Page 4: LIGO- G040310-00-R Sensing and control, SPIE conference, June 2004 1 Sensing and control of the Advanced LIGO optical configuration SPIE conference at

Sensing and control, SPIE conference, June 2004 4LIGO- G040310-00-R

Caltech 40 meter prototype interferometer

Objectives Develop lock acquisition procedure of suspended-mass

detuned Resonant Sideband Extraction (RSE) Characterize noise mechanism Verify optical spring effect Develop readout scheme

for Advanced LIGO and other future GW detectors

BSPRM SRM

X arm

Y arm

Darkport

Brightport

Page 5: LIGO- G040310-00-R Sensing and control, SPIE conference, June 2004 1 Sensing and control of the Advanced LIGO optical configuration SPIE conference at

Sensing and control, SPIE conference, June 2004 5LIGO- G040310-00-R

Length sensing and control

Phase lock

Feedback~

Locked

Sidebands (probe for carrier)

Carrier

L

Sig

nal[

a.u.

]

Unlocked

PD

EOM:Modulation

Mixer :Demodulation~

Oscillator~MHz

L

Error signal

Lock point

Locking area

Page 6: LIGO- G040310-00-R Sensing and control, SPIE conference, June 2004 1 Sensing and control of the Advanced LIGO optical configuration SPIE conference at

Sensing and control, SPIE conference, June 2004 6LIGO- G040310-00-R

Signal extraction for AdvLIGO

Arm cavity signals are extracted from beat between carrier and f1 or f2.

Central part (Michelson, PR, SR) 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

ETMy

ETMx

ITMy

ITMxBSPRM

SRM

Two modulations are used to separate high finesse, 4km long arm cavity signals from Central part (Michelson, PR, SR) signals.

4km

4k

m

Page 7: LIGO- G040310-00-R Sensing and control, SPIE conference, June 2004 1 Sensing and control of the Advanced LIGO optical configuration SPIE conference at

Sensing and control, SPIE conference, June 2004 7LIGO- G040310-00-R

5 DOF for length control

Laser

ETMy

ETMx

ITMy

ITMxBS

PRM

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.

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 cavityMichelsonSignal recycling cavity

Page 8: LIGO- G040310-00-R Sensing and control, SPIE conference, June 2004 1 Sensing and control of the Advanced LIGO optical configuration SPIE conference at

Sensing and control, SPIE conference, June 2004 8LIGO- G040310-00-R

Disturbance by sidebands of sidebands

Sidebands of sidebands are produced by two series EOMs. Beats between carrier and f2 +/-f1 disturb central part.

Original concept Real world

f1-f1 f2-f2

Carrier

f1-f1 f2-f2

Carrier

Port Dem. Freq.

L L l l l s

SP f1 1 -1.4E-8 -1.2E-3 -1.3E-6 -6.2E-6

AP f2 1.2E-7 1 1.4E-5 1.3E-3 6.5E-6

SP f1 f2 7.4 -3.4E-4 1 -3.3E-2 -1.1E-1

AP f1 f2 -5.7E-4 32 7.1E-1 1 7.1E-2

PO f1 f2 3.3 1.7 1.9E-1 -3.5E-2 1

Page 9: LIGO- G040310-00-R Sensing and control, SPIE conference, June 2004 1 Sensing and control of the Advanced LIGO optical configuration SPIE conference at

Sensing and control, SPIE conference, June 2004 9LIGO- G040310-00-R

Mach-Zehnder on 40m PSLto eliminate sidebands of sidebands

Series EOMswith sidebands of sidebands

EOM2EOM1

Mach-Zehnder interferometerno sidebands of sidebands from beginning

PD

EOM1

EOM2

PZT mirrorBS1

BS2

33MHzEOM

166MHzEOM

29MHzEOM

PD

Page 10: LIGO- G040310-00-R Sensing and control, SPIE conference, June 2004 1 Sensing and control of the Advanced LIGO optical configuration SPIE conference at

Sensing and control, SPIE conference, June 2004 10LIGO- G040310-00-R

Lock Acquisition of Detuned RSE

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

ETMy

ETMx

ITMy

ITMxBSPRM

SRM

ITMy

ITMxBSPRM

SRM

Step 2Step 1Step 3

Central part: not disturbed by lock status change of arm cavity

Find primary signal not disturbed by the other two DOFs

Find secondary signal not disturbed by the residual DOF

Arm cavities: not disturbed by locked central part

Lock each arm cavity independently

Switch control servo to common/differential control

Page 11: LIGO- G040310-00-R Sensing and control, SPIE conference, June 2004 1 Sensing and control of the Advanced LIGO optical configuration SPIE conference at

Sensing and control, SPIE conference, June 2004 11LIGO- G040310-00-R

l- signal with double demodulation

Good l- signal when l+ and ls is locked

No good l- signal once l+ and ls start moving

Lock point

Lock point

Page 12: LIGO- G040310-00-R Sensing and control, SPIE conference, June 2004 1 Sensing and control of the Advanced LIGO optical configuration SPIE conference at

Sensing and control, SPIE conference, June 2004 12LIGO- G040310-00-R

l- signal with double demodulation

Good l- signal when l+ and ls is locked

No good l- signal once l+ and ls start moving

Lock point

Lock point

Page 13: LIGO- G040310-00-R Sensing and control, SPIE conference, June 2004 1 Sensing and control of the Advanced LIGO optical configuration SPIE conference at

Sensing and control, SPIE conference, June 2004 13LIGO- G040310-00-R

Looking for good signal for lock acquisition

Unfortunately, no way to lock central part directly using the original double demodulation

Dither locking for l- signal

Divide signal by inside power» Good cancellation of power recycling

2PO

POAPPOAP

PO

AP

-

V

VVVV

V

V

ld

dVl

Laser

ITMy

ITMxBS

PRM

SRM

SPAP

PO

~

1

Vl

LPF LPF LPF LPF

Digital calculation

(VPO)’ (VAP)’VPO VAP

a few kHz

Page 14: LIGO- G040310-00-R Sensing and control, SPIE conference, June 2004 1 Sensing and control of the Advanced LIGO optical configuration SPIE conference at

Sensing and control, SPIE conference, June 2004 14LIGO- G040310-00-R

l- signal with dither

Dither on ITMx, ITMy with 1kHz

Error signal is calculated digitally as follows;

l- signal does not depend on l+ at all

Good l- signal obtained with all ls movement

Lock point

Lock point

2PO

POAPPOAP

PO

AP -

V

VVVV

V

V

ld

dVl

Page 15: LIGO- G040310-00-R Sensing and control, SPIE conference, June 2004 1 Sensing and control of the Advanced LIGO optical configuration SPIE conference at

Sensing and control, SPIE conference, June 2004 15LIGO- G040310-00-R

l+ signal with l- lock

Zero crossing point of l+ corresponds with movement of ls

Distance between PRM and SRM is kept

Good l+ signal obtained with all ls movement

Lock point

Lock point

Page 16: LIGO- G040310-00-R Sensing and control, SPIE conference, June 2004 1 Sensing and control of the Advanced LIGO optical configuration SPIE conference at

Sensing and control, SPIE conference, June 2004 16LIGO- G040310-00-R

ls signal with l- and l+ lock

Good ls signal can be extracted

Page 17: LIGO- G040310-00-R Sensing and control, SPIE conference, June 2004 1 Sensing and control of the Advanced LIGO optical configuration SPIE conference at

Sensing and control, SPIE conference, June 2004 17LIGO- G040310-00-R

Summary

Optical configuration for AdvLIGO being developed at 40m prototype interferometer

Sidebands of sidebands: eliminated by M-Z interferometer

Ready to try lock acquisition Lock acquisition: promising with dither lock

Hope we succeed in locking detuned RSE very soon!