sas group r&d results

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October 8th 2002 SAS Group R&D results 1 SAS group R&D results Riccardo DeSalvo 8th October 2002 1. TAMA-SAS 2. Active Internal Damping 3. Passive Pre-Isolation 4. Glassy metal developments 5. Nursery

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SAS group R&D results. Riccardo DeSalvo 8th October 2002 TAMA-SAS Active Internal Damping Passive Pre-Isolation Glassy metal developments Nursery. TAMA SAS team. Akiteru Takamori’s PhD thesis. Univ. of Tokyo M. Ando Y. Iida K. Nanjo Y. Nishi K. Numata - PowerPoint PPT Presentation

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Page 1: SAS group R&D results

October 8th 2002 SAS Group R&D results 1

SAS group R&D results

Riccardo DeSalvo8th October 2002

1. TAMA-SAS2. Active Internal Damping3. Passive Pre-Isolation4. Glassy metal developments5. Nursery

Page 2: SAS group R&D results

October 8th 2002 SAS Group R&D results 2

Univ. of Tokyo M. Ando Y. Iida K. Nanjo Y. Nishi K. Numata K. Otsuka K. Somiya A. Takamori K. Tsubono T. Yoda

NAOJ M. Fukushima S. Kawamura R. Takahashi

Caltech R. DeSalvo Sz. Márka V. Sannibale H. Yamamoto C. Wang H. Tariq

INSA de Lyon F. Jacquier N. ViboudUniversita’ di Pisa

A. Bertolini G. Cella Other Institution

G. Losurdo (Virgo) and others

TAMA SAS team

•Akiteru Takamori’s PhD thesis

Page 3: SAS group R&D results

October 8th 2002 SAS Group R&D results 3

1 TAMA-SAS results

• Completed assembly of TAMA-SAS suspended 3 m test F.P. interferometer,

• Characterizing performance (A.T. thesis subject).

• Validating design and performance for production of the main towers for TAMA 300 (production in 2003)

other users (production in 2002/2003) : 3 towers for Naples, 1 tower for Florence

Page 4: SAS group R&D results

October 8th 2002 SAS Group R&D results 4

TAMA SAS 3 m F.P. experiment

10-5

10-4

10-3

10-2

10-1

100

101

102

Magnitude

0.1 1 10Frequency [Hz]

Experiment Noise Simulation SAS noise

Reduction:

One towerMeasuringA Michelson to ground

Page 5: SAS group R&D results

October 8th 2002 SAS Group R&D results 5

TAMA SAS 3 m F.P. experiment

10-12

10-11

10-10

10-9

10-8

10-7

10-6

10-5

10-4

Displacement [m/Hz

1/2

] [m]

0.012 3 4 5 6 7

0.12 3 4 5 6 7

12 3 4 5 6 7

10

Frequency [Hz]

psd rms damping off damping on

Acquired Lock of Cavity−Test Mass Motion of

0.2 nm r.m.s.

4 nm/rtHz @ 1 Hz

Natural Motion of Test MassesAir measurement

Page 6: SAS group R&D results

October 8th 2002 SAS Group R&D results 6

1 TAMA-SASfuture developments/commitments

• Provide technical support for :1. production of TAMA-300 SAS towers (2003-2004)

2. SAS tower development optimized for LCGT and second generation Cryo-Virgo (long term)

3. production of a TAMA-SAS tower for University of Florence accelerometer development facility(2003)

4. production of 3 TAMA-SAS towers for University of Naples test interferometer (2003)

• No construction costs, marginal drafting costs ($5000)

Page 7: SAS group R&D results

October 8th 2002 SAS Group R&D results 7

1 TAMA-SASpossible future developments

• Small incremental improvements of SAS passive attenuation chain concept

• Study of use of glassy metal GAS springs for mirror suspensions

• Timescale– Low priority operation

• Costs– Marginal drafting and hardware costs

Page 8: SAS group R&D results

October 8th 2002 SAS Group R&D results 8

2 Active Internal Damping• Developed in vacuum damping scheme to limit the

excitation of the present LIGO stacks,– LIGO- T020038-01-R

• Made complete construction design and started construction of parts for installation in LASTI– LIGO -D020212-00-R

Page 9: SAS group R&D results

October 8th 2002 SAS Group R&D results 9

2 Active Internal Damping• Developed in vacuum damping scheme to limit the excitation of the present

LIGO stacks,– LIGO- T020038-01-R

• Made complete construction design and started construction of parts for installation in LASTI

– LIGO -D020212-00-R

• Built functional 1-to-1 prototype with spare LIGO springs, an optical table and cannibalized SAS sensors and actuators – LIGO- G020169-00

• Tested successfully the 6 degree of freedom damping scheme– LIGO- G020212-00

Page 10: SAS group R&D results

October 8th 2002 SAS Group R&D results 10

• Damping OFF

• Damping ON

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Step response

Page 11: SAS group R&D results

October 8th 2002 SAS Group R&D results 11

2 Active Internal Damping

• Aborted production• Mothballed in April 2002

– deemed superfluous because of active pre-isolator expected performance

(HEPI/MEPI).

Page 12: SAS group R&D results

12 SAS Group R&D results October 8th 2002

3 Passive Pre-Isolation

• Developed passive pre-isolator alternative to HEPI/MEPI. – Negative stiffness springs, derived from SAS would mount on

each pier and both support the LIGO platform weights and neutralize the bellow springness.

– Performance: >40dB estimated above 1 Hz, – upgradable to >60dB and lower frequency with low power (mW)

active operation LIGO- T020039-01-R

• Full size, partial prototypes of the horizontal and vertical negative stiffness springs built with SAS spare parts,

• Successfully tested performance and validated concept – LIGO- T020055-00-R – LIGO- T020052-00-R

Page 13: SAS group R&D results

October 8th 2002 SAS Group R&D results 13

Mechanicaldesign LIGO- D200001-00-R

LIGOPassive External Pre-isolator

mounted ona pier

Page 14: SAS group R&D results

October 8th 2002 SAS Group R&D results 14

3 Passive Pre-Isolation

• Made complete construction design of Passive Pre-Isolator,

• Built partial prototype according to production design

• ready for production LIGO- D200001-00-R

Page 15: SAS group R&D results

October 8th 2002 SAS Group R&D results 15

3 Passive Pre-Isolation• Made complete construction design of Passive Pre-Isolator, ready

for production – LIGO- D200001-00-R

• Built partial prototype according to production design

• Costed the system at 50,000$/BSC or HAM– plus 40,000$ for active upgrade

• Estimated production time ~ 2 months

• Mothballed in May 2002 counting on success of baseline active system.

Page 16: SAS group R&D results

October 8th 2002 SAS Group R&D results 16

4 Glassy Metal advanced suspension development program

• Developing a low loss mirror suspension scheme, capable of delivering advanced performance at room temperature

• The aim is to find a viable alternative to the fused silica fiber suspensions (more reliable and better performance) for Adv. LIGO

• The idea is to take advanced of the superior useable strength (~5GPa) of glassy metal to manufacture very small section (a few micron thick) flex joints suspensions

• The high fracture toughness of glassy metal insure very high reliability while requiring minimal safety factors

• Simulations using glassy metal properties indicate performance exceeding the fused silica fiber’s

Page 17: SAS group R&D results

October 8th 2002 SAS Group R&D results 17

Glassy Metal simulated performance

Glassy metal Q=104, Fused SiO2 dumb bell shaped fiber Q=8.4*108,10*3000 = 30,000 m2, 357 m diameter, 100,000 m2, 60 Kg mirror, 40 Kg mirror

Page 18: SAS group R&D results

October 8th 2002 SAS Group R&D results 18

•Valerie Cervantes Data Analysis (TP) / H.S. Student Mayfield (Pas.)•Allyson Feeney Hardness / H.S. Student Westridge (Pas.)•Maddalena Mantovani Hardness & Elasticity / Undergraduate Pisa•Stefano Tirelli Stress & Strain / Undergraduate Pisa•Brian Emmerson X-Ray Diffraction / Undergraduate Cambridge•Michael Hall Thermal Properties / Undergraduate Drexel•Rosalia Stellacci Creep Analysis / Undergraduate Pisa•Xavier De Lepine FEA of Flex Joint / Undergraduate INSA Lyon•Eric Kort Sample Uniformity / Undergraduate Pomona C.•Stoyan Nikolov FEA of Flex Joint / Undergraduate INSA Lyon•Charles Bordier material properties / Undergraduate INSA Lyon•Barbara Simoni Phase Transition / Undergraduate Pisa•ChenYang Wang Stress & Strain / Graduate Student Caltech/Stanford•Jan Schroers Post Doctoral Scholar Caltech•Alessandro Bertolini Assistant Professor (University of Pisa) Pisa•Bill Johnson Professor (Materials Science) Caltech•Riccardo DeSalvo Sr. Scientist Caltech•Hareem Tariq Coordinator / Graduate Student Caltech

Glassy metal team

•Hareem Tariq’s PhD thesis

Page 19: SAS group R&D results

October 8th 2002 SAS Group R&D results 19

4 Glassy Metal advanced suspension development program

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0

0.2

0.4

0.6

0.8

1

1.2

20 40 60 80 100 120

J/mm

-2 s-1

2θ/°

• Main focus of the SAS group efforts• Established a GM production line• Testing the material properties• Developing a suspension construction scheme• Developing a suspension test facility

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50 m 10 m 50 m

Page 20: SAS group R&D results

October 8th 2002 SAS Group R&D results 20

4 Glassy Metal advanced suspension development program

• Timescale / Costs / Efforts: • Aim is to validate simulations, that exceed Fused

Silica fiber performances, within 2003• many small expenses (~$100,000) not detaileable

• Will absorb bulk of SAS team attention and efforts– Unless need to resume mothballed projects

• Mainly run by students of various degrees.

Page 21: SAS group R&D results

October 8th 2002 SAS Group R&D results 21

• Trying to draw talented students to Gravitational Wave Interferometers (poaching in HEP and other fields all over the world)

• 2 Grad students

• ~10 undergrad students

• 2 High School students

5 Nursery

Page 22: SAS group R&D results

October 8th 2002 SAS Group R&D results 22

• Akiteru, finishing Tokyo Univ.PhD thesis on TAMA-SAS, moving to Hanford– (will continue support TAMA-SAS installation)

• Hareem, starting Caltech PhD thesis on low thermal noise mirror suspensions

• Chenyang, Caltech, moving to Stanford

• Eric, Pomona College, will return for 6 month stage and make graduation work with us

• Mike, Drexel, will make graduation work with us, will apply for graduate school in Caltech, possibly on Gravitational Waves

5 Nursery effect

Page 23: SAS group R&D results

October 8th 2002 SAS Group R&D results 23

• Barbara, Lia, Maddalena, Stefano, University of Pisa, third year thesis on Glassy Metals, some will return for fifth year thesis (Master thesis), some to finish measurements

• Brian, Cambridge, will apply for graduate school in Caltech, possibly on Gravitational Waves

• The four Pisa students funded through INFN/NSF international student exchange program.

• Three US exchange students worked in Virgo (Fidecaro).• Forthcoming grad student from Pisa to somewhere in LIGO

– Student selection committee in November

5 Nursery effect