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Black Hole

Lensing of space time around a black hole. At Oxford we study black holes observationally and theoretically on all size and time scales - it is some of our core work.

Credit: ALAIN RIAZUELO, IAP/UPMC/CNRS. CLICK HERE TO VIEW MORE IMAGES.

Dr. Boon Kok Tan

Senior Researcher

Research theme

  • Astronomy and astrophysics
  • Instrumentation

Sub department

  • Astrophysics

Research groups

  • Superconducting quantum detectors
boonkok.tan@physics.ox.ac.uk
Telephone: 01865 (2)73352
Denys Wilkinson Building, room 756
  • About
  • Publications

Preliminary characterisation of titanium nitride thin film at 300 mK for the development of kinetic inductance travelling wave parametric amplifiers

Proceedings of the SPIE Photonex + Vacuum Technologies Society of Photo-optical Instrumentation Engineers 11881

Authors:

Joseph Longden, Faouzi Boussaha, Christine Chaumont, Kitti Ratter, Boon Tan

Abstract:

Travelling wave parametric amplifiers (TWPAs) made from highly nonlinear reactive superconducting thin films have been demonstrated to be a viable technology for various quantum applications, including fundamental physics experiments such as astronomy and axion dark matter searches, as well as commercial applications like quantum computational and communication systems. In this paper, we present the design of a kinetic inductance TWPA comprising a patterned titanium nitride film that can operate at 0.3 K to demonstrate the feasibility of operation closer to 1 K temperature, paving the way to achieve even higher bath temperature operation. We discuss in detail the design of our TWPA, along with the predicted gain-bandwidth product and other characteristics. We perform the preliminary experimental investigation of the thin film properties and compare that with the simulated results. We found that there are several discrepancies between the measured and the predicted behaviour of the thin film. We attribute these differences to the fact that the fabricated thin film has a different gap voltage, resistivity and thickness to what we expected. With a new set of estimated parameters, we successfully reproduce the measured transmission profile. We further show that by utilising bridges to ensure equipotential grounds for the CPW lines, we managed to reduce the rippling effect and achieve higher gain with broader bandwidth. We expect that our TWPA can achieve higher than 20 dB gain from approximately 0–8 GHz.
Details from ORA
More details from the publisher

Quantum Detection for Millimetre and Sub-Millimetre Astronomy

Abstract:

Oxford Physics Colloquium

Quantum Sensors for the Hidden Sector (QSHS) - A Summary of Our First Year!

Authors:

Ian Bailey, Bhaswati Chakraborty, Gemma Chapman, Ed Daw, Ling Hao, Edward Hardy, Edward Laird, Peter Leek, John Gallop, Gianluca Gregori, John March-Russell, Phil Meeson, Clem Mostyn, Yuri Pashkin, Searbhan O Peatain, Mitch Perry, Michele Piscitelli, Edward Romans, Subir Sarkar, Ningqiang Song, Mahesh Soni, Paul Smith, Boon-Kok Tan, Stephen West, Stafford Withington
More details from the publisher

Signal coupler

Travelling wave parametric up-converter

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