A broad band acoustic detector
- f GW: The dual torus
J.P.Zendri* For the Auriga collaboration
* I.N.F.N. Padova Section, Via Marzolo 8, 35010 Padova, Italy, Zendri@lnl.infn.it
A broad band acoustic detector of GW: The dual torus J.P.Zendri* - - PowerPoint PPT Presentation
A broad band acoustic detector of GW: The dual torus J.P.Zendri* For the Auriga collaboration * I.N.F.N. Padova Section, Via Marzolo 8, 35010 Padova, Italy, Zendri@lnl.infn.it Motivations Design of a new detector: Sensitive at high
* I.N.F.N. Padova Section, Via Marzolo 8, 35010 Padova, Italy, Zendri@lnl.infn.it
XXXVIIIth Rencontre de Moriond, 2003, J.-P.Zendri
. . Elast Body Transd
M Mechanical Amplification G M = ≡
.
1
Transd Elast Body
M Fractional bandwidth M G ν ν Λ = = ≡
. .
1
trasd Elast Body
M M G →
XXXVIIIth Rencontre de Moriond, 2003, J.-P.Zendri
M.Cerdonio et. al., Phys Rev. Let. 87, 031101 (2001) M.Bonaldi et. al., arXiv:gr-qc/0302012
m m m
2 2 2
( ) ( ) ( ) (r) w (r)
n n n n
q t q t F t G dV t ρ ρω ∂ + = ⋅ ∂
r r
2 2
(r, ) [ (r, )] ( ) G(r) u t L u t F t t ρ ∂ − = ⋅ ∂ r r r r r r
2w (r)
[w (r)]
n n n
L ρω = r r r r
N
(r) X( ) (r, ) P P t u t dV = ∫ r r r
XXXVIIIth Rencontre de Moriond, 2003, J.-P.Zendri
Motion Equation Mode expansion Spatial solution Time evolution
+ a,n , , a,n , ,
w (r)= cos( ) sin( ) w (r)=- cos( ) sin( )
a n r a n a n r a n
f a i g a i f a i g a i
θ θ
θ θ θ θ
×
+ + r r r r r r r r
a=2 sensitive to GW a=4 a=30 a=3 Output Signal
XXXVIIIth Rencontre de Moriond, 2003, J.-P.Zendri
XXXVIIIth Rencontre de Moriond, 2003, J.-P.Zendri
.
Meas r N
1 2 3 4 meas
X X X X X = − + −
XXXVIIIth Rencontre de Moriond, 2003, J.-P.Zendri
, ,
Meas a a n n a N N
Same for both Mode weight
XXXVIIIth Rencontre de Moriond, 2003, J.-P.Zendri
1 2 int 2
0.25 0.26 0.47
ext
r cm r cm r cm
− −
= = =
Molybdenum:
XXXVIIIth Rencontre de Moriond, 2003, J.-P.Zendri
( ) Transfer Function ( ) ( )
i i Ext
X H F ω ω ω = ≡
Displacement equivalent force PSD Transfer function
1 2
( ) ( ) Dual T.F. ( ) ( )
D Ext
X X H F ω ω ω ω − = ≡
Displacement equivalent input Force PSD
XXXVIIIth Rencontre de Moriond, 2003, J.-P.Zendri
Back Action displacement PSD Equivalent B.A. input force PSD B.A. equivalent input force PSD
XXXVIIIth Rencontre de Moriond, 2003, J.-P.Zendri
Thermal noise displacement PSD Thermal equivalent input force PSD
Ext Ther
XXXVIIIth Rencontre de Moriond, 2003, J.-P.Zendri
XXXVIIIth Rencontre de Moriond, 2003, J.-P.Zendri 2
( ) ( ) 4
FF XX
S S ω ω ⋅ ≥ h
n
K ( )/ ( )
n FF XX
K S S ω ω = Broad Band White band dominated B.A. dominated
9
10
n
K =
11
10
n
K =
10
10
n
K =
XXXVIIIth Rencontre de Moriond, 2003, J.-P.Zendri
sound
4
3
[ / ] Kg m ρ
LowTemp
3200 N.A.
s
v [ / ] m s 10300 2700 11200 5660 5050
8
10 >
7
10
XXXVIIIth Rencontre de Moriond, 2003, J.-P.Zendri
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
− − −
≥ ⋅ = = = = = = ⋅
XXXVIIIth Rencontre de Moriond, 2003, J.-P.Zendri
Present 1. SQUID at 30 ħ (P. Falferi this congress) 2. Electrical bias field 10 MV/m
7 2
3. / 10 N/m
FF XX
S S E C ≈ ∝ ⋅ Required 1. SQUID at 1 ħ 2. Electrical bias field >200 MV/m 3. Carefully designed matching line
To SQUID Amplifier
XXXVIIIth Rencontre de Moriond, 2003, J.-P.Zendri
Required 1. Laser Power 10 W 2. Finesse 106 Items to be addressed Possible Solution 1. Wide sensing area Folded Fabry-Perot 2. Cryogenics Material with higher Q
XXXVIIIth Rencontre de Moriond, 2003, J.-P.Zendri
has been studied.
comparable with the predicted sensitivity of the next IFO generation with the further advantage of the detector compactness.
noise stiffness of the present transducer generation.
starting
sensitivity using different real read-out, cosmic rays effect)