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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

Operation of kinetic-inductance travelling wave parametric amplifiers at millimetre wavelengths

Superconductor Science and Technology IOP Publishing 37 (2024) 035006

Authors:

Boon Tan, Nikita Klimovich, Ryan Stephenson, Farzad Faramarzi, Peter Day

Abstract:

It is expected that the operation of microwave Kinetic Inductance Travelling Wave Parametric Amplifiers (KITWPAs) can be extended to the millimetre (mm) and the sub-mm wavelength range as long as the frequency is below the gap frequency of the superconducting film. This paper presents possible mm-wave designs for KITWPAs based on microstrip transmission lines. Our device is designed based on the BCS (Bardeen-Cooper-Schrieffer) model which successfully reproduces the measured transmission profile, gain, bandwidth, and nonlinear response of a fabricated KITWPA operating in the Ka-band, and includes the millimetre-wave dielectric loss determined by fitting the quality factor of a Wband microstrip resonator. We suggest a layout for a KITWPA operating near 220 GHz that can be fabricated using the same superconducting properties as the Ka-band device and can be coupled to a waveguide system. We conclude the paper by extending the 220 GHz design to higher frequency regimes approaching 1 THz.
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Modeling and Testing Superconducting Artificial CPW Lines Suitable for Parametric Amplification

(2023)

Authors:

FP Mena, D Valenzuela, C Espinoza, F Pizarro, B-K Tan, DJ Thoen, JJA Baselmans, R Finger
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Engineering the thin film characteristics for optimal performance of superconducting kinetic inductance amplifiers using a rigorous modelling technique.

Open research Europe Faculty of 1000 2 (2023) 88

Authors:

Boon-Kok Tan, Faouzi Boussaha, Christine Chaumont, Joseph Longden, Javier Navarro Montilla

Abstract:

<b>Background:</b> Kinetic Inductance Travelling Wave Parametric Amplifiers (KITWPAs) are a variant of superconducting amplifier that can potentially achieve high gain with quantum-limited noise performance over broad bandwidth, which is important for many ultra-sensitive experiments. In this paper, we present a novel modelling technique that can better capture the electromagnetic behaviour of a KITWPA without the translation symmetry assumption, allowing us to flexibly explore the use of more complex transmission line structures and better predict their performance. <b>Methods:</b> In order to design a KITWPA with optimal performance, we investigate the use of different superconducting thin film materials, and compare their pros and cons in forming a high-gain low-loss medium feasible for amplification. We establish that if the film thickness can be controlled precisely, the material used has less impact on the performance of the device, as long as it is topologically defect-free and operating within its superconducting regime. With this insight, we propose the use of Titanium Nitride (TiN) film for our KITWPA as its critical temperature can be easily altered to suit our applications. We further investigate the topological effect of different commonly used superconducting transmission line structures with the TiN film, including the effect of various non-conducting materials required to form the amplifier. <b>Results:</b> Both of these comprehensive studies led us to two configurations of the KITWPA: 1) A low-loss 100 nm thick TiN coplanar waveguide amplifier, and 2) A compact 50 nm TiN inverted microstrip amplifier. We utilise the novel modelling technique described in the first part of the paper to explore and investigate the optimal design and operational setup required to achieve high gain with the broadest bandwidth for both KITWPAs, including the effect of loss. <b>Conclusions:</b> Finally, we conclude the paper with the actual layout and the predicted gain-bandwidth product of our KITWPAs.
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Searching for wave-like dark matter with QSHS

SciPost Physics Proceedings SciPost 12 (2023)

Authors:

Ian Bailey, Bhaswati Chakraborty, Gemma Chapman, Edward J Daw, John Gallop, Gianluca Gregori, Edward Hardy, Ling Hao, Edward Laird, Peter Leek, John March-Russell, Phil Meeson, Seaárbhan Ó Peatáin, Yuri Pashkin, Mitchell G Perry, Michele Piscitelli, Edward Romans, Subir Sarkar, Paul J Smith, Ningqiang Song, Mahesh Soni, Boon Kok Tan, Stephen West, Stafford Withington

Abstract:

In 2021 the Quantum Sensors for the Hidden Sector (QSHS) collaboration was founded in the UK and received funding to develop and demonstrate quantum devices with the potential to detect hidden sector particles in the μeV to 100 μeV mass window. The collaboration has been developing a range of devices. It is building a high-field, low-temperature facility at the University of Sheffield to characterise and test the devices in a haloscope geometry. This paper introduces the collaboration's motivation, aims, and progress.
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Analytical expressions for the design of twin junction tuning in SIS mixers

Engineering Research Express IOP Publishing 5:2 (2023) 025071

Authors:

J Wenninger, G Yassin, B-K Tan
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