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page of Luciano Gottardi
Instrument
Scientist
Welcome
to South Holland
Niels
Bohrweg 4 2333 CA Leiden
The
Netherlands
Tel: +31 (0)88 777
5861
Tel. lab:
(5896,5897) Fax: +31 (0)88 777 5601
Research
Interests
Low
Temperature Detectors for Astrophysics and Particle Physics
The
X-IFU is a 2-D imaging camera, which allows the identification and
characterization of the different ionization stages in hot plasmas
thanks to its excellent spectral resolution (2.5 eV at 6 keV).
This enables detailed diagnostics of abundances, temperatures,
densities and bulk or turbulent velocities of hot plasma in
extended objects. It is an integral-field spectrometer operating
in the soft X-ray band. The detector consists of an array of 3840
micro-calorimeters based on Transition
Edge Sensors (TESs). The read-out is performed using Frequency
Domain Multiplexing (FDM) in the 1-5 MHz bandwidth and is
based on low noise Superconducting Quantum Interference Devices
(SQUID) and high-Q superconducting LC resonators.
The MiniGRAIL detector
is a cryogenic 68 cm diameter spherical gravitational wave antenna
made of CuAl(6%) alloy with a mass of 1400 Kg, a resonance
frequency of 2.9 kHz and a bandwidth around 230 Hz. The
quantum-limited strain sensitivity dL/L would be ~4x10-21.
The antenna will operate at a temperature of 20 mK.
Sensitivity
of the spherical gravitational wave detector MiniGRAIL operating
at 5 K. Phys. Rev. D 76, 102005 (2007)
Complete
model of a spherical gravitational wave detector with capacitive
transducers: Calibration and sensitivity optimization. Phys. Rev.
D 75, 022002 (2007)
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