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9 Luglio, 2003 LTD 10 – Genova, Italia 1
Parameter Comparison for Low-NoiseMo/Au TES Bolometers
Dominic BenfordHarvey MoseleyJohannes StaguhnChristine Allen
NASA / Goddard Space Flight Center
Jay ChervenakThomas StevensonWen-Ting Hsieh
LTD 10 – Genova, Italia 29 Luglio, 2003
Context
! Developing bolometers for far-IR astronomy! Building arrays of SQUID-multiplexed bolometers for
SOFIA/SAFIRE, ASTRO/SPIFI, GBT/3mmCam! Related presentations:
" Staguhn et al. Detector noise analysis talk R05" Chervenak et al. Detector fabrication description Y18" Allen et al. Detector fabrication description Y24" Dicker et al. GBT/3mmCam instrument talk W03" Moseley et al. 2D (semiconducting) array talk Y06
LTD 10 – Genova, Italia 39 Luglio, 2003
Bolometer Requirements
! Parameters:" Tbath ~ 300mK (±20%)" Power ~ 1pW (±3x)" NEP ~ 10-17 W/√Hz" τ ≤ 10ms" Absorbs at ~100µm-1mm
" TC ~ 450mK (±10%)" RN ~ 400mΩ (±20%)" G(TC) ~ few x 10-11 W/K (±3x)
TC
Tbath
G
C
(Absorber)
τ = C/G
Optical Power
LTD 10 – Genova, Italia 49 Luglio, 2003
Mechanical Implementation
! 1x8 linear arrays of Pop-Up Bolometers
! Folding allows arrays to be close-packed
! Thermal isolation high, since flexure hinges are thin
! SHARC-II (12x32=384 pixel)semiconducting Pop-Up array (Moseley et al.)
LTD 10 – Genova, Italia 59 Luglio, 2003
History of our TES bilayers
! Both Mo/Au and Mo/Cu fabricated
! Good performance demonstrated, but not sufficiently repeatable
! Always some excess noise, often out-of-band, sometimes 5x-10x thermal noise limit
LTD 10 – Genova, Italia 69 Luglio, 2003
Approach: Boundary Conditions
! Current flowing in TES can take many possible paths
! Initial trials indicated that normal metal bars on sides could help constrain possible paths, leading to more orderly current flow
! Other constraints may be more likely to prevent moving “chunks” of superconducting regions
Lindeman et al. model
Superconducting
Normal
LTD 10 – Genova, Italia 79 Luglio, 2003
Trial #1: Longitudinal Bars
! In order to better understand the effect of boundary condition geometry on detector performance, we produced several nearly identicalbolometers with different normal metal bars.
! Several designs of longitudinal bars produced
! Some designs are wedged to remove isotropy
#0
#1
#2
#3
#4
LTD 10 – Genova, Italia 89 Luglio, 2003
Trial #2: Transverse Bars
! Several designs of transverse bars produced
! Some designs are interdigitated; others are continuous
#0
#1
#2
#3
LTD 10 – Genova, Italia 99 Luglio, 2003
Transition Measurements
! 4-wire measurements of resistance vs. temperature, with several bias currents to estimate self-heating and critical currents.
! Addition of transverse bars does cause sharpness to degrade, butstill achieve α≈100
0.00
0.05
0.10
0.15
0.20
0.25
0.30
0.35
0.40
0.45
0.50
0.500 0.501 0.502 0.503 0.504 0.505 0.506 0.507 0.508 0.509 0.510Temperature (K)
Ch 0
Ch 1
Ch 2
0.0
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0.425 0.430 0.435 0.440 0.445 0.450 0.455Temperature (K)
Ch2 cut
Ch3 cut
Longitudinal bars Transverse bars
LTD 10 – Genova, Italia 109 Luglio, 2003
Behavior on Bias (I)
! I(V) curves taken on all devices; calibrated to determine resistance and power as a function of base temperature.
! Some calibration uncertainties remain.
0
5
10
15
20
25
30
35
40
0 1 2 3 4 5 6 7 8 9 10TES Bias Voltage (µV)
C0R4
C0R0
C0R2C0R1
C0R3
0
2
4
6
8
10
12
14
16
18
20
0 1 2 3 4 5 6TES Bias Voltage (µV)
C1R2C1R3
C1R0
C1R1
Longitudinal bars Transverse bars
LTD 10 – Genova, Italia 119 Luglio, 2003
Behavior on Bias (II)
! Resistance vs. bias yields close to expected values.! Some calibration uncertainties remain.
Longitudinal bars Transverse bars
0
100
200
300
400
500
600
0 1 2 3 4 5 6 7 8 9 10TES Bias Voltage (µV)
C0R4C0R0
C0R2
C0R1C0R3
0
50
100
150
200
250
300
350
400
450
500
0 1 2 3 4 5 6TES Bias Voltage (µV)
C1R2
C1R3
C1R0
C1R1
LTD 10 – Genova, Italia 129 Luglio, 2003
Behavior on Bias (III)
! Power vs. bias yields similar value for all pixels (as should be the case).! Power on transition quite constant (as should be the case).! Some calibration uncertainties remain.
Longitudinal bars Transverse bars
0
20
40
60
80
100
120
140
160
180
200
0 1 2 3 4 5 6 7 8 9 10TES Bias Voltage (µV)
C0R4
C0R0
C0R2
C0R1
C0R3
0
10
20
30
40
50
60
70
80
90
100
0 1 2 3 4 5 6TES Bias Voltage (µV)
C1R2C1R3
C1R0C1R1
LTD 10 – Genova, Italia 139 Luglio, 2003
Pixel Thermal Conductance
! Thermal conductance measured by average power on transition for many bath temperatures
! Power law fit:" TC=443mK" G(TC) = 6·10-10 W/K (higher than desired)" Index G=G0TN, N~2 (though not tightly
constrained)" Psat = 84pW (with Tbath=0)." Phonon noise: 6·10-17 W/√Hz
! Next device mask will reduce leg width, to reduce Psat and G(TC) by ~10x.
0
5
10
15
20
25
30
35
40
45
350 360 370 380 390 400 410 420 430 440 450Temperature (mK)
TC
= 443 mKG(T
C) = 0.58 pW/mK
Index ~ 2P
sat = 84 pW
LTD 10 – Genova, Italia 149 Luglio, 2003
Dynamic Measurements
! Measured complex impedance Z(ω) for bolometers, as perLindeman et al.
! Results prove tricky to interpret; devices too fast for reliable high frequency impedance measurements
! Time constants of 1/τe~5kHz.
-90
-80
-70
-60
-50
-40
-30
-20
-10
0
10
-80 -60 -40 -20 0 20 40 60
Imag
inar
y Im
peda
nce
(mž)
Real Impedance (mž)
SuperconductingZ=24.0mžZ=32.0mžZ=40.0mžZ=52.5mž
10 kHz
~100 Hz
5.5 kHz
4.5 kHz
4.0 kHz
4.0 kHz
X
X
X
X
X
XX
XXX
XXXXXXXXXXXXXXX
XXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXXX
-500
-400
-300
-200
-100
0
100
200
300
-400 -300 -200 -100 0 100 200 300 400
0mž
34mž
44mž
55mž
68mž
81mž
96mž
112mž
129mž
147mž
166mž
187mž
208mž
231mž
255mž
281mž
307mž
335mž
363mž
393mž
X 400mž
410mž
421mž
421mž
LTD 10 – Genova, Italia 159 Luglio, 2003
Noise Measurements
! The subject of Johannes Staguhn’s talk; in order not to spoil the surprise:
The geometry of the bars does affect the noise.
0
50
100
150
200
250
300
0 5000 10000 15000 20000 25000Frequency (Hz)
0
50
100
150
200
250
300
0 5000 10000 15000 20000 25000
Cur
rent
Noi
se (p
A/¦H
z)
Frequency (Hz)
LTD 10 – Genova, Italia 169 Luglio, 2003
Optical Measurements
! Bismuth absorbing film deposited on bolometers to impedance math to free space.
! Dark tests after deposition show same result as tests prior to deposition.
! Optically functioning bolometers are demonstrated in the dark; prior tests have verified optical performance.
Optical measurement of a blackbody calibrator from an earlier, similar bolometer.
LTD 10 – Genova, Italia 179 Luglio, 2003
Summary
! Several nearly identical bolometers produced, with different normal metal bars. Bolometers are optically active detectors.
! Tests of quasi-DC parameters (TC, RN, α, Psat, etc.) show good consistency.
! Noise performance can be improved by changing bar geometry.
! Measurements & analysis ongoing to quantify improvements and differences. Time constant (impedance) analysis to be refined.