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91探花
Black Hole

Lensing of space time around a black hole. At 91探花 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

An initial concept of a resonance phase matched junction-loaded travelling wave parametric tripler

ISSTT 2024 Proceedings National Radio Astronomy Observatory (2025)

Abstract:

In this paper, we investigate the possibility of utilising a tunnel-junction loaded transmission line as high efficiency parametric frequency multiplier. Through the interaction between the injected primary tone and the nonlinear medium, higher harmonic tones can be generated through wave-mixing process. Here, we aim to maximise the third harmonic wave generation. We first establish a theoretical framework outlining the mechanism for generating the third harmonic component from a single pump wave propagating in a nonlinear transmission line. We begin by demonstrating that strong third harmonic generation is possible with the resonance phase matching technique, albeit with an extremely narrow operational bandwidth. To broaden the bandwidth, we modify the dispersion engineering element of our circuit and show that broadband operation is achievable, while preventing unwanted harmonic tone growth. We extend this calculation from the microwave to the millimetre and sub-millimetre regimes and demonstrate that by adjusting the parameters of the junctions and the dispersion engineering circuits, we can achieve high conversion efficiency close to 1 THz.

Heterodyne Spectroscopy Instrument (HSI) for Far-IR Spectroscopy Space Telescope (FIRSST)

National Radio Astronomy Observatory (2025)

Authors:

Martina C Wiedner, Paul Grimes, Boon Tan, Andrey Baryshev

Abstract:

The Heterdyne Spectrometer Instrument (HSI) is one of two instruments on the Far-IR Spectroscopy Space Telescope (FIRSST) proposal to NASA. It would be the first heterodyne array receiver in space and has 3 frequency bands, each containing two 5-pixel arrays, one per polarizations. HSI uses high TRL (>6) components and is an innovative, but low-risk instrument.

Preliminary characterisation of titanium nitride kinetic inductance travelling-wave parametric amplifiers

Open Research Europe F1000Research 5 (2025) 109

Authors:

Joseph Longden, Christine Chaumont, Nikita Klimovich, Samuel Wood, Faouzi Boussaha, Boon-Kok Tan

QSHS: An Axion Dark Matter Resonant Search Apparatus

(2025)

Authors:

A Alsulami, I Bailey, G Carosi, G Chapman, B Chakraborty, EJ Daw, N Du, S Durham, J Esmenda, J Gallop, T Gamble, T Godfrey, G Gregori, J Halliday, L Hao, E Hardy, EA Laird, P Leek, J March-Russell, PJ Meeson, CF Mostyn, Yu A Pashkin, SO Peatain, M Perry, M Piscitelli, M Reig, EJ Romans, S Sarkar, PJ Smith, A Sokolov, N Song, A Sundararajan, B-K Tan, SM West, S Withington

Automated characterisation and operational insights of superconducting travelling wave parametric amplifiers: unveiling novel behaviours and enhancing tunability

Journal of Instrumentation IOP Publishing 19:08 (2024) P08024

Authors:

S Wood, N Klimovich, Boon Tan

Abstract:

Superconducting travelling wave parametric amplifiers (TWPAs) exhibit great promise across various applications, owing to their broadband nature, quantum-limited noise performance, and high-gain operation. Whilst their construction is relatively simple, particularly for thin-film-based TWPAs, challenges such as the requirement for an extremely long transmission line, current fabrication limitations, and their sensitivity to fabrication tolerances, mean that their optimal operating conditions often differ from those anticipated during the design stage. As a result, manual fine-tuning of numerous operational parameters becomes necessary to recover optimal performance; a process that is both labour-intensive and time-consuming. This paper introduces an automated methodology designed to significantly accelerate the characterisation of a TWPA by several orders of magnitude without requiring human intervention. Additionally, we have developed metrics to condense the multitude of measured frequency responses of the TWPA, obtained in data cube form, into an easily-understandable format for further scientific interpretation. To demonstrate the efficacy and speed of our methodology, we utilise an existing NbTiN (niobium titanium nitride) TWPA as an example. This showcases the capability of our approach to unveil both broad- and fine-scale behaviours of the device, highlighting the importance of an automated experimental setup for the in-depth investigation of TWPAs for future developments.

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