STREGA - WP2-Task C: Design of advanced cryogenic suspensions

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articipants: C-1:Cryogenic last-stage suspensions (interferometers) (F.Ricci-G.Frossati) Objectives: -Design new suspension elements for the last stage of interferometers. -Achieve a low noise remote control of the mirror position using cryogenic sensors -Assemble and test of a full-scale prototype of cryogenic final stage C-2:Cryogenics suspensions for advanced interferometers (G.Frossati-M.Bassan)- Objectives: -Two 1.2 ton spheres with their suspension assembled and measurements of Q and thermal noise at low temperature performed. C-3: Cryogenics suspension system for interferometers (S.Braccini-M.Bassan) Objectives:

description

STREGA - WP2-Task C: Design of advanced cryogenic suspensions. Year 1 - 2004. C-1:Cryogenic last-stage suspensions (interferometers) (F.Ricci-G.Frossati) Objectives: -Design new suspension elements for the last stage of interferometers. - PowerPoint PPT Presentation

Transcript of STREGA - WP2-Task C: Design of advanced cryogenic suspensions

Page 1: STREGA - WP2-Task C: Design of advanced cryogenic suspensions

Participants:

C-1:Cryogenic last-stage suspensions (interferometers) (F.Ricci-G.Frossati)Objectives: -Design new suspension elements for the last stage of interferometers.-Achieve a low noise remote control of the mirror position using cryogenic sensors-Assemble and test of a full-scale prototype of cryogenic final stage C-2:Cryogenics suspensions for advanced interferometers (G.Frossati-M.Bassan)-Objectives:-Two 1.2 ton spheres with their suspension assembled and measurementsof Q and thermal noise at low temperature performed.C-3: Cryogenics suspension system for interferometers (S.Braccini-M.Bassan)Objectives:-The entire apparatus be located in a cryogenic environment; the extra noise coming from the cryogenic system be studied and made negligible.-Full cryogenic suspension be assembled and tested

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Participants:Participants: INFN ROG

Leiden University

Tasks: - Cool down of Minigrail to 50 mK- Investigation of heat transfer from the mixing chamber to the sphere

Deliverables: - Report on mechanical transfer function

measurements of cryogenic suspension

Cryogenic suspension system for advanced resonant detectors

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MiniGRAILCryogenics

cryostat

Liquid N2 77K (-196 ºC)

Liquid He4K (-269 ºC)

Dilution refrigerator(10 mK)

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MiniGRAILCryogenics; The dilution refrigerator

still(700 mK)

50 mKplate

mixingchamber(10 mK)

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To 50 mK shield

To mixing chamber

CryogenicsThermal anchoring suspension

To still shield

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CryogenicsRun 4

Minimum temperatures:Tsphere = 80 mKTmc = 20 mK

Time dependent heat leak from sphere:

45 W after 6 weeks

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Vibration Isolation System

1

2

3

4

5

6

7Attenuation cables

+ absorbers

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Vibration Isolation System

1

2

3

4

5

6

7

Attenuation between mass 1 and 2

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• Larger diameter (68 cm instead of 65 cm) gives lower frequency and higher mass (1300 kg instead of 1150 kg).

• Six holes machined in TIGA positions

The new sphere

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Resonance frequencies of bare sphere at 300 K

Old sphereNew sphere

Frequency of new sphere about 200 Hz lower

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Improvements on the Vibration Isolation System

370

370

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370

370

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370

Material before (mm) fbefore (Hz)

CuAl 1,2 370 3516

CuAl 3,4 370 3516

Cu 5-7 370 3397

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Improvements on the Vibration Isolation System

370

370

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Material before (mm) fbefore (Hz) after (mm) fafter (Hz)

CuAl 1,2 370 3516 370 3516

CuAl 3,4 370 3516 362 3633

Cu 5-7 370 3397 358 3512

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Improvements on the Vibration Isolation System

370

370

362

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358

358

~ 50 dB

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Closed Membrane Capacitive Transducer

Advantages:• Compact design• Easy to make

electrode

membrane

mass (~ 200 g)

spring

CuAl6%

d ~ 30 micro mVBIAS up to 500 V

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Cryogenic run

transformer +2-stage SQUID

calibrator

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3 hour acquisition @ 5K of mode 3 (2943 Hz)

exponential fit

Teff = 70 mK

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MiniGRAIL sensitivity - run 6

1.5 x 10-20

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MiniGRAIL sensitivity - run 6

Run 6

T 5 K

700 ħ

Q 105

M 200 g

C 1.1 nF

Vbias 200 V

Run 7

T 80 mK

100 ħ

Q 106

M 400 g

C 1.5 nF

Vbias 400 V

Teff = 40 K4 x 10-22

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MiniGRAIL sensitivity - comparison

Initial target large interferometers

LIGO S3

GEO

AURIGA

NAUTILUS/EXPLORER

MiniGRAILrun 6

Planned at the end of 2004

MiniGRAILrun 7