Broad band acoustic detectors J.P. Zendri* on behalf of the AURIGA - - PowerPoint PPT Presentation

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Broad band acoustic detectors J.P. Zendri* on behalf of the AURIGA - - PowerPoint PPT Presentation

Broad band acoustic detectors J.P. Zendri* on behalf of the AURIGA collaboration www.auriga.lnl.infn.it 5 th International LISA Symposium 12-15 July 2004 Acoustic detector noise budget:one dimensional lumped model Quantum mechanics constrain T


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SLIDE 1

J.P. Zendri*

  • n behalf of the AURIGA collaboration

www.auriga.lnl.infn.it

Broad band acoustic detectors

5th International LISA Symposium 12-15 July 2004

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SLIDE 2

5th International LISA Symposium 12-15 July 2004

Acoustic detector noise budget:one dimensional lumped model

2 2 2 2

( ) ( ) 4

B n FF XX

k T S S ω ω ω ≡ ⋅ ≥ h ( )/ ( )

n FF XX

K S S ω ω =

Quantum mechanics constrain Tn The noise stiffness Kn is unconstrained

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SLIDE 3

5th International LISA Symposium 12-15 July 2004 ( ) ( ) ( ) ( )

FF X V X n V II

T S S S S ω ω ω ω ∝ ⋅ ⋅ ฀

2

( )/ ( ) ( )/ ( )

n VV II II FF

S S K S S ω ω α ω ω = ฀ I X Transducer Efficency α ≡ =

2 2

( ) ( ) ( ) ( )

FF VV XX II

S S S S ω ω ω α α ω

= × ≈ ×

General result:

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SLIDE 4

5th International LISA Symposium 12-15 July 2004

Practical limits to the Kn Passive transducers Active transducers

2 2

( )/ ( ) 10 / 10

n bias VV II

K E S S MV m Breakdown ω ω

↓ ∝ Ω ↓ ฀

For instance capacitive For instance optical

5 6

10 10

n

K Finesse LaserPower Watt ∝ × ≥ ↓ ÷ ↓

Kn OK but problems for cryogenics

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SLIDE 5

5th International LISA Symposium 12-15 July 2004

Methods to increase the efficiency: resonant transducers

Mechanical signal amplified before the transduction One mode transducer Two mode transducer Velocity transformer

bar Tr

ω ω = /

BAR TR

M M = /

bar TR BAR

M M ν = Required Increment of a around resonance Bandwidth upper limit

bar First Last

ω ω ω = = /

BAR LAST

M M = /

bar First BAR

M M ν = Required Increment of a around resonance Bandwidth upper limit Broad Band amplification but still a complete thermal noise analysis is missing

J.P. Richard, Phys. Rev. Let. 52, 165 (1984) H.J. Paik, Jour. Appl. Phys. 47, 1168 (1976)

  • D. Blair et al, Appl. Phys. 20, 162 (1987)
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SLIDE 6

5th International LISA Symposium 12-15 July 2004

Auriga method: Resonating matching line

( ) ( ) ( )

2 2

I 1 x ( ) /

Bias s in eff el el el

i ME L L L i Q ω ω α ω ω ω ω ωω = = + − +

2

1 ( ) 1

eff P P in S el eff el eff el

M L L L L L L C L Q R ω ω   ≡ −   +   ≡ ≡

Enhancement of the transducer efficiency around the mechanical modes

el mech

ω ω ⇒

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SLIDE 7

5th International LISA Symposium 12-15 July 2004

This because the equivalent electric mode mass is light Auriga operate with a Q factor of ~ 500.000

2 2

20 .

Tr Bias el el

C E M gr ω = ฀

Tuning the electrical mode to the mechanical modes require a very high electrical Q quality factor

Tr

C = Transducer capacitance

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SLIDE 8

800 850 900 950 1000 1050 1100 1E-6 1E-5 1E-4 1E-3 Wide Band Noise Level Spurious HV Plate Resonances 3 Main Modes

Auriga Output PSD at 4.5 K

SΦΦ

1/2 [Φ0/Hz 1/2]

Frequency [Hz]

5th International LISA Symposium 12-15 July 2004

Around the sensitivity bandwidth Auriga noise is dominated by LC thermal noise

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SLIDE 9

5th International LISA Symposium 12-15 July 2004

Auriga readout

1.5 2.0 2.5 3.0 3.5 4.0 4.5

0.4 0.6 0.8 1.0 1.2 1.4 1.6 1.8

N

Double SQUID white band noise

PSD [µΦo

2/Hz]

Temperature [K]

150 200 250 300 350 400 450

5000

Auriga Old

N

=

h B n

k T N ω =

h

h

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SLIDE 10

5th International LISA Symposium 12-15 July 2004

AURIGA present Sensitivity

800 820 840 860 880 900 920 940 960 980 1000 1E-21 1E-20 1E-19

Noise curve prediction at 4.5K Auriga Now T=4.5 K Auriga Old T=0.1 K

Shh

1/2 [Hz

  • 1/2]

Frequency [Hz]

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SLIDE 11

5th International LISA Symposium 12-15 July 2004

Solution One: Wrong! Dominated by thermal and BA of the reference mass Solution Two: M2~ M1 but CM2CM1 Solution Three: M2 ~ M1 and same CM Dual Detector

Increase the bandwidth: The Dual detector

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SLIDE 12

5th International LISA Symposium 12-15 July 2004

Considered geometries for Dual

Dual Sphere

M.Cerdonio et. al., Phys. Rev. Let. 87, 031101 (2001)

Dual Torus

M.Bonaldi et. al., Phys Rev. D62, 102004 (2003)

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SLIDE 13

5th International LISA Symposium 12-15 July 2004

Quantum Limited sensitivity curve (dual torus)

8 1 2 int 1 2 1

/ 2 10 0.25 0.26 0.47 2.35 16. 1 4 .0 1 /

n Mo ext

K Q T r m r m N r m h m Tot wei m gth t

− − −

≥ ⋅ = = = = = = ⋅

8 1 2 in 11 t 2

/ 2 10 0.82 0.83 1. 1.8 10 1. / 44 3 6 5

n Si ext C

Q T r m r m r m h m Tot weigt t N m h K

− − −

≥ ⋅ = = = = = = ⋅

In order to get Kn ~1011 N/m a lever geometrical amplification of at least 10 is required

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SLIDE 14

5th International LISA Symposium 12-15 July 2004

Broad band lever amplification Hinges X Y Mirror

Mechanical amplification=Y/X=1/a>>1

H.J. Paik et al, Proc. Of the first Amaldi Meeting, edited by E. Coccia et al, World scientific Singapore, p201 (1995)

Auriga design:

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SLIDE 15

Prototype under test:Amplification

5th International LISA Symposium 12-15 July 2004

Mode Domain Lever Domain

Material Al7075

  • T=300 K
  • Gaussian Beam waste 0.375 mm
  • Mirrors Fused silica

Geometrical gain factor=10

Parameters for simulation

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SLIDE 16

5th International LISA Symposium 12-15 July 2004

Prototype test:assembling procedure

Harmonic oscillator Amplifier

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SLIDE 17

250 500 750 1000 1250 1500 1750 2000 2250 1E-18 1E-17 1E-16 1E-15 S

1/2 xx(f) [m/Hz 1/2]

Frequency[Hz]

5th International LISA Symposium 12-15 July 2004

Prototype thermal noise estimation The amplifier thermal noise contribution is negligable

Resonator Therm Therm xx Amplifier out xx

S Gain S

− − −

≈ ×

Resonator alone

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SLIDE 18

Room Temperature Thermal Noises Measurement: 10 µK Stabilized Thermal Box!

NTC Thermistors Technology ア5μK Active ア1mK Thermal Box 1 μ Yag LASER

5th International LISA Symposium 12-15 July 2004

Prototype thermal noise measurement set-up

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SLIDE 19

5th International LISA Symposium 12-15 July 2004

A possible implementation in Dual-Torus

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SLIDE 20

5th International LISA Symposium 12-15 July 2004

Dual Torus Therm. and BA noise reduction: Wide area sensing

GW sensitive (quadrupolar) mode: Some GW not sensitive mode which provide only noise: High order modes are averaged out

Signal=mean displacement over the readout area=Green surf.+Yellow surf.

Some of the low order modes are averaged out

Unperturbed torus Mode Shape Rejected Not Rejected

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SLIDE 21

5th International LISA Symposium 12-15 July 2004

Dual Torus Therm. and BA noise reduction: Selective readout

Meas-Selective 1 2 3 4

X X X X X = − + −

meas-Standard

X X =

Meas-Selective

Maximized X →

Meas-Selective

X → Quradrupolar mode (Signal) Octupolar (Noise)

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SLIDE 22

5th International LISA Symposium 12-15 July 2004

1 2 int 2

0.25 0.26 0.47

ext

r cm r cm r cm

− −

= = =

Material:Molybdenum: Dimensions: Red:Selective readout

Strain Noise Power spectrum

Blue: Not Selective readout

Example of Thermal and BA noise reduction using selective readout

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SLIDE 23

5th International LISA Symposium 12-15 July 2004

Conclusions

  • Well designed impedance matching lines between the

main resonator and the amplifier has been used to widen the useful band of the Auriga detector more than one order

  • f magnitude
  • Broad band detectors should be obtained using lever
  • transducers. In particular the proposed detector “dual”

promises a sensitivity of the order of 10-23 Hz-1/2 in the frequency range between 1kHz to 5 kHz.