P5. Cold-Electron Bolometer Array (CEB Array) made by E-Beam Lithography and a Shadow Evaporation Technology - PowerPoint PPT Presentation

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P5. Cold-Electron Bolometer Array (CEB Array) made by E-Beam Lithography and a Shadow Evaporation Technology

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JFET _at_ 4K - sensitive current measurements - but high voltage noise - promising with S-I-S -I-S bolometers Chalmers Un., IREE, IZMIRAN, MSU, VTT ... – PowerPoint PPT presentation

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Title: P5. Cold-Electron Bolometer Array (CEB Array) made by E-Beam Lithography and a Shadow Evaporation Technology


1
Bolometer Group
Through the thorns to the stars! Igenom törnen
mot stjärnorna! ????? ?????? ? ???????!
Chalmers University of Technology
  • P5. Cold-Electron Bolometer Array (CEB Array)
    made by E-Beam Lithography and a Shadow
    Evaporation Technology

Leonid Kuzmin and Ian Agulo
FKA190
2
Bolometer Group
Chalmers University of Technology
  • Superconducting Cold-Electron Bolometer with JFET
    readout for OLIMPO balloon telescope

Leonid Kuzmin, Philip Mauskopf , and Dmitry
Golubev Cardiff University, UK Karlsruhe
Forschungszentrum, Germany
EUCAS -2005
3
3-layer technology
JFET Voltage- biased
SCEB
OLIMPO Cardiff
2-layer Al-Ti Direct Write technology
CEB- Series array
JFET Current -biased
2-layer Ti-Al Direct Write technology
CEB
CLOVER others Oxford
SQUID
Shadow Evaporation Technology
CEB- Parallel array
  • CLOVER
  • Phase Switch
  • Oxford,
  • Cardiff

NbN Nanostrip Finline
4
Balloon telescope OLIMPO (follower of BOOMERanG)
  • a multi-wavelength survey of galaxy clusters and
    the cosmic submm/mm background
  • 2.6 meter antenna
  • A few arcmin resolution survey of the sky
  • 150, 220 350, 600 GHz (Background load Po 3 -
    20 pW
  • Background limited bolometers (210-17 110-16
    W/Hz1/2),
  • 64 bolom. per channel
  • Bolometers TESSQUID readout
  • SiNJFET readout
  • CEBJFET (or SQUID) readout
  • Rome Un., Cardiff Un., IROE-CNR (Italy), Caltech
    (USA), Santa Barbara Un. , DAFNIA/SPP (France),
    Tel Aviv Un., VTT (finland), Chalmers Univ.

5
Balloon telescope OLIMPO
  • 1. Channel I 2.1 mm (140 GHz)
  • Power load is relatively high P0 2 3 pW
  • Photon noise
  • Total NEP of CEB should be less than photon
    noise NEPtot lt NEPphot.
  • Single CEB doesnt give proper results.
  • Only SCEB could give the proper NEP.

6
Cold-Electron Bolometer (CEB) with Capacitive
Coupling to the Antenna Kuzmin ISSTT-98
7
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8
Readout Systems for CEB current measurements
SQUID with a bulk input transformer - most sensitive - very complicated Chalmers Un., IREE, IZMIRAN, MSU, VTT (Finland)
JFET _at_ 4K - sensitive current measurements - but high voltage noise - promising with S-I-S-I-S bolometers Chalmers Un., Cardiff Un, IREE, Rome Un.
HEMT _at_ 4K with resonance circuits - good for multiplexing - need modulation technique IPHT (Jena), Chalmers Un., CESR (Toulouse)

9
CEB with JFET
10
Cold-Electron Bolometer Noise
11
JFET amplifier noise
We need matching with
12
Capacitively Coupled Superconducting
Cold-Electron Bolometer (SCEB)
L. Kuzmin, Microelectronic Engineering, 69 (2003)
13
SCEB with JFET
Total NEP is less than NEPphot for SCEB, total
iJFET10 fA/Hz1/2, R0.5 kOhm and 0.1 kOhm (one
junction), Vol0.05um3, power load 2 pW.
IV curves are shown for estimation of high
dynamic resistance of the junctions.
14
Series Array of CEBs with JFET readout
Circle waveguide is coupled to 4 coplanar
lines Each Coplanar line is coupled to 2 CEBs
15
CEB, Current-biased, Array - 10 junctions
Total NEP is less than NEPphot vJFET2nV/Hz1/2
R0.5 kOhm (one junction), Vol0.02um3, power
load2 pW The power is split between bolometers
and responsivity is considerably improved.
16
Total NEP of CEB and NEPphot for series array
CEBs in dependence on number of CEBs
a) 600 GHz, power load P0 20 pW, vJFET3
nV/Hz1/2 R0.5 kOhm Vol0.05um3 Optimal number of
CEBs 20-50. b) 140 GHz, power load P0 2 pW,
vJFET2 nV/Hz1/2 R0.5 kOhm Vol0.02um3. Optimal
number of CEBs 5-10.
17
JFET in current-biased mode. Variants
  • Series array of CEBs
  • Array of SINIS structures without biasing
  • Array of SN NS Andreev contacts thermo-voltage
    without biasing
  • Array of thermocouples (thermo-pile)
  • Combination of thermocouples and superconducting
    islands (SN Andreev contacts)
  • Array of CEBs series for DC
  • - parallel for HF

18
Series Array of CEBs with JFET readout
Parallel for HF
HF
19
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20
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21
Conclusions
New generation of detectors is needed to measure
Cosmic Microwave Background (OLIMPO project)
Cold-Electron Bolometer (CEB) with JFET readout
very attractive option! Single CEB with JFET
no chance! Array of CEBs with JFET the most
attractive opportunity SCEB (Superconducting
Cold-Electron Bolometer) with JFET realistic
and effective decision
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