test mass dynamics with optical springs proposed experiments at gingin

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Test mass dynamics with optical springs proposed experiments at Gingin Chunnong Zhao (University of Western Australia) Thanks to ACIGA members Stefan Danilishin and Farid Khalili (Moscow State University) Yanbei Chen (Caltech) 1 GWADW2010, May 19, 2010

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Test mass dynamics with optical springs proposed experiments at Gingin. Chunnong Zhao (University of Western Australia) Thanks to ACIGA members Stefan Danilishin and Farid Khalili (Moscow State University) Yanbei Chen (Caltech). Contents: Gingin high optical power research facility - PowerPoint PPT Presentation

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Test mass dynamics with optical springsproposed experiments at Gingin

Chunnong Zhao(University of Western Australia)

Thanks to ACIGA members

Stefan Danilishin and Farid Khalili(Moscow State University)

Yanbei Chen (Caltech)

GWADW2010, May 19, 2010

2GWADW2010, May 19, 2010

Contents:

• Gingin high optical power research facility

• 3-mode optomechanical transducer

• Test mass dynamics with double optical springs (negative optical inertia)

• Summary

3GWADW2010, May 19, 2010

Gingin high optical power test facility

High optical power is necessary for improving advanced detector sensitivity, but it also introduces thermal lensing and various instabilities.

4GWADW2010, May 19, 2010

Gingin high optical power test facility

On this facility, we have demonstrated:• Thermal lesing and thermal compensation• In-situ real time thermal lensing monitoring using

Hartmann sensor• 3-mode opto-acoustic interactions• Cavity locking using ultra-low frequency vibration

isolators

Current main focus: parametric instability and its control

GWADW2010, May 19, 2010 5

Future 80m interferometer

M1 M2

M3

To Detector Bench

South Fabry-Perot Cavity

East Fabry-Perot Cavity

Mode Cleaner

Nd:YAG laserl = 1064nm

East-end Station

South-end Station

N

Signal Recycling Mirror

Beam SplitterPower Recycling Cavity

6GWADW2010, May 19, 2010

Currently, 2 independent 80m cavities

South arm: Sapphire test masses with LIGO SOS suspension

Finesse, ~1300, 10 W laserTested thermal lensing and thermal compensation;Observed 3-mode opto-acoustic interactions;Study 3-mode optomechanical transducer.

East arm: Fused silica test masses with UWA isolators and suspensions

Nominal cavity finesse, 1500050W laser to be installed in August

Main goals are test the parametric instability and its control.

7GWADW2010, May 19, 2010

3-mode optomechanical transducer

m 10

Test mass internal mode mCavity Fundamental mode (TEM00, frequency o)

Input light frequency o

Scattering into TEMmn,frequency 1

frequency matching and spatial overlap of acoustic and optical modes

8GWADW2010, May 19, 2010

FSR

01

23

45

DTEM

3-mode optomechanical transducer

0 0 +m

DTEM

9GWADW2010, May 19, 2010

CO2 laser thermal tuning the radius of curvature

Sapphire test mass

Hartmannsensor

He-Ne laser

CO2 laser

Probe beam(800nm) Vacuum

tank

Vacuum pipe

Nd:YAGlaser

10GWADW2010, May 19, 2010

CCD

Laser

ITM

CP

ETM

SpectrumAnalyzer

yx

QPD

Fundamental mode

High order mode

3-mode optomechanical transducer

CO2 Laser

11

181.57 181.58 181.59 181.6 181.61 181.62 181.63 181.64 181.65 181.66

10-17

10-16

kHz

m/rtHz

GWADW2010, May 19, 2010

Test mass thermal noise at ~181.6 kHz

3-mode optomechanical transducer

0 50 100 150 200 250 300-0.8

-0.6

-0.4

-0.2

0

0.2

0.4

0.6

12GWADW2010, May 19, 2010

3-mode optomechanical transducerpotential to observe the quantum radiation pressure noise

Laser

1mm x 1mm x 50nm

The vibration of silicon nitride membrane excites high transverse optical mode

QPD

Finesse=10,000Meff=40 ng, T=4 k, m=2p*200 kHzQm=106

Circulating power= 0.5W

Radiation pressure noise ~ thermal noise@ mechanical resonance

13GWADW2010, May 19, 2010

Test mass dynamics with optical springs

Motivation:

The SQL in terms of GW strain sensitivity:

A system with larger mechanical susceptibility (/m) has smaller SQL than the free mass SQL

Y. Chen, et al, LIGO-T1000069-v1

14GWADW2010, May 19, 2010

Test mass dynamics with optical springs

Considering the test mass dynamics with double optical springs (DOS)

F is the force applied on the test mass, x is the displacement ,

,Here, s=-i;

15GWADW2010, May 19, 2010

Test mass dynamics with optical springs

PM: power recycling mirror; PBS: polarization beam splitter; BS: beam splitter; PD: photodetector; ITM: input test mass; ETM: end test mass.

Driving force

This is achievable at Gingin with a 3-mirror cavity:

The same configuration can also be used to demonstrate the local readout (optical bar)

16GWADW2010, May 19, 2010

Test mass, m=0.8 kg, cavity length L=80m, cavity circulating power:I1= 3kW, I2=10kW,

Cavity detuning:1/2p=200 Hz2/2p=-500 Hz

Cavity linewidth:1/2 p=36 Hz;2/2 p=400 Hz;

Test mass dynamics with optical springs

Free mass

With DOS

17GWADW2010, May 19, 2010

Summary

Gingin high optical power research facility consists:• High power lasers• Advanced vibration isolators and test mass suspension• High finesse cavities

In addition to the parametric instability research, we propose to study:• High sensitivity optomechanical transducer (potential for detecting the quantum radiation pressure noise)• Optical negative inertia • Local readout (optical bar)