262 research outputs found
Strong Quasiparticle Trapping In A 6x6 Array Of Vanadium-Aluminum Superconducting Tunnel Junctions
A 6x6 array of symmetrical V/Al/AlOx/Al/V Superconducting Tunnel Junctions
(STJs) was fabricated. The base electrode is a high quality epitaxial film with
a residual resistance ratio (RRR) of ~30. The top film is polycrystalline with
an RRR of ~10. The leakage currents of the 25x25 mm^2 junctions are of the
order of 0.5 pA/mm^2 at a bias voltage of 100 mV, which corresponds to a
dynamical resistance of ~ 3 10^5 ohms. When the array was illuminated by 6 keV
X-ray photons from a 55Fe radioactive source the single photon charge output
was found to be low and strongly dependent on the temperature of the devices.
This temperature dependence at X-ray energies can be explained by the existence
of a very large number of quasiparticle (QP) traps in the Vanadium. QPs are
confined in these traps, having a lower energy gap than the surrounding
material, and are therefore not available for tunneling. The number of traps
can be derived from the energy dependence of the responsivity of the devices
(charge output per electron volt of photon input energy).Comment: 4 pages. presented at Low Temperature Detectors-
Optical photon detection in Al Superconducting Tunnel Junctions
We report on the successful fabrication of low leakage aluminium
superconducting tunnel junctions with very homogeneous and transparent
insulating barriers. The junctions were tested in an adiabatic demagnetisation
refrigerator with a base temperature of 35 mK. The normal resistance of the
junctions is equal to ~7 uohm cm2 with leakage currents in the bias voltage
domain as low as 100 fA/um2. Optical single photon counting experiments show a
very high responsivity with charge amplification factors in excess of 100. The
total resolving power (including electronic noise) for 500 nm photons is equal
to 13 compared to a theoretical tunnel limited value of 34. The current devices
are found to be limited spectroscopically by spatial inhomogeneities in the
detectors responseComment: 3 pages, 5 figure
Modelling the energy gap in transition metal/aluminium bilayers"
We present an application of the generalised proximity effect theory.Comment: 15 pages, 11 figures, presented at workshop on low temperature
superconducting electronics at the University of Twente, The Netherland
Future optical detectors based on Al superconducting tunnel junctions
Superconducting tunnel junctions are being developed for application as
photon detectors in astronomy. We present the latest results on the development
of very high quality, very low critical temperature junctions, fabricated out
of pure Al electrodes. The detectors are operated at 50 mK in an adiabatic
demagnetisation refrigerator. The contacts to the top and base electrodes of
these junctions are fabricated either out of Nb or Ta, which has strong
implications on the loss time of the quasiparticles. The Nb contacted junctions
show quasiparticle loss times varying between 5 and 80 usec, depending on the
device size. The bias range of the Nb-contacted junctions is limited to the
range 0-100 uV, because of the set-in of strong non-equilibrium quasiparticle
multiplication currents at higher bias voltages. The Ta-contacted junctions, on
the other hand, show quasiparticle loss times in excess of 200 usec. These long
loss times lead to very strong quasiparticle multiplication, which prevents the
stable biasing of the junctions even at very low bias voltages. Junction
fabrication and characterisation are described, as well as the response of the
detectors to monochromatic light with wavelengths varying from 250 to 1000 nm.
The energy resolution of the detectors is discussed.Comment: 12 pages, 10 figure
Dynamics of nonequilibrium quasiparticles in a double superconducting tunnel junction detector
We study a class of superconductive radiation detectors in which the
absorption of energy occurs in a long superconductive strip while the redout
stage is provided by superconductive tunnel junctions positioned at the two
ends of the strip. Such a device is capable both of imaging and energy
resolution. In the established current scheme, well studied from the
theoretical and experimental point of view, a fundamental ingredient is
considered the presence of traps, or regions adjacent to the junctions made of
a superconducting material of lower gap. We reconsider the problem by
investigating the dynamics of the radiation induced excess quasiparticles in a
simpler device, i.e. one without traps. The nonequilibrium excess
quasiparticles can be seen to obey a diffusion equation whose coefficients are
discontinuous functions of the position. Based on the analytical solution to
this equation, we follow the dynamics of the quasiparticles in the device,
predict the signal formation of the detector and discuss the potentiality
offered by this configuration.Comment: 16 pages, 5 figures Submitted to Superconducting Science and
Technolog
First results of a cryogenic optical photon counting imaging spectrometer using a DROID array
Context. In this paper we present the first system test in which we
demonstrate the concept of using an array of Distributed Read Out Imaging
Devices (DROIDs) for optical photon detection. Aims. After the successful S-Cam
3 detector the next step in the development of a cryogenic optical photon
counting imaging spectrometer under the S-Cam project is to increase the field
of view using DROIDs. With this modification the field of view of the camera
has been increased by a factor of 5 in area, while keeping the number of
readout channels the same. Methods. The test has been performed using the
flexible S-Cam 3 system and exchanging the 10x12 Superconducting Tunnel
Junction array for a 3x20 DROID array. The extra data reduction needed with
DROIDs is performed offline. Results. We show that, although the responsivity
(number of tunnelled quasiparticles per unit of absorbed photon energy, e- /eV)
of the current array is too low for direct astronomical applications, the
imaging quality is already good enough for pattern detection, and will improve
further with increasing responsivity. Conclusions. The obtained knowledge can
be used to optimise the system for the use of DROIDs.Comment: 7 pages, 9 figures, accepted for publicaiton in A&
Non-Commutative Geometry and Measurements of Polarized Two Photon Coincidence Counts
Employing Maxwell's equations as the field theory of the photon, quantum
mechanical operators for spin, chirality, helicity, velocity, momentum, energy
and position are derived. The photon ``Zitterbewegung'' along helical paths is
explored. The resulting non-commutative geometry of photon position and the
quantum version of the Pythagorean theorem is discussed. The distance between
two photons in a polarized beam of given helicity is shown to have a discrete
spectrum. Such a spectrum should become manifest in measurements of two photon
coincidence counts. The proposed experiment is briefly described.Comment: Latex, 13 pages, 3 figure
Simultaneous Absolute Timing of the Crab Pulsar at Radio and Optical Wavelengths
The Crab pulsar emits across a large part of the electromagnetic spectrum.
Determining the time delay between the emission at different wavelengths will
allow to better constrain the site and mechanism of the emission. We have
simultaneously observed the Crab Pulsar in the optical with S-Cam, an
instrument based on Superconducting Tunneling Junctions (STJs) with s time
resolution and at 2 GHz using the Nan\c{c}ay radio telescope with an instrument
doing coherent dedispersion and able to record giant pulses data. We have
studied the delay between the radio and optical pulse using simultaneously
obtained data therefore reducing possible uncertainties present in previous
observations. We determined the arrival times of the (mean) optical and radio
pulse and compared them using the tempo2 software package. We present the most
accurate value for the optical-radio lag of 255 21 s and suggest the
likelihood of a spectral dependence to the excess optical emission asociated
with giant radio pulses.Comment: 8 pages; accepted for publication in Astronomy and Astrophysic
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