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.

Ghassan Yassin

Emeriti

Sub department

  • Astrophysics

Research groups

  • Superconducting quantum detectors
ghassan.yassin@physics.ox.ac.uk
Telephone: 01865 (2)73440
Denys Wilkinson Building, room 750
  • About
  • Publications

Microwave transmission through high-temperature superconducting waveguides

PHYSICA C 372 (2002) 523-525

Authors:

G Yassin, I Barboy, V Dikovsky, M Kambara, DA Cardwell, S Withignton, G Jung

Abstract:

Microwave transmission through HTSC circular waveguides close to the cutoff conditions has been investigated. Applicative consequences of a sharp decrease in the transmitted power observed in the vicinity of the superconducting transition are discussed. (C) 2002 Elsevier Science B.V. All rights reserved.
More details from the publisher

Far-infrared optics design & verification

International Journal of Infrared and Millimeter Waves 23:7 (2002) 1029-1045

Authors:

C O'Sullivan, E Atad-Ettedgui, W Duncan, D Henry, W Jellema, JA Murphy, N Trappe, H Van De Stadt, S Withington, G Yassin

Abstract:

Compact quasi-optics are difficult to design with any confidence using techniques developed for visible wavelengths. In this paper we investigate the performance of existing software design tools (ASAP, CODE V, GLAD) as well as a Gaussian beam mode analysis technique not yet available as commercial software. We have devised a set of test cases and used these to study the underlying methodologies and physics of these packages and we probe their suitability for the analysis of submillimetre-wave systems and components. We have used the physical optics package GRASP as our benchmark software.
More details from the publisher
More details

Analyzing the power coupled between partially coherent waveguide fields in different states of coherence.

J Opt Soc Am A Opt Image Sci Vis 19:7 (2002) 1376-1382

Authors:

Stafford Withington, Ghassan Yassin

Abstract:

A procedure is described for calculating the power coupled between partially coherent waveguide fields that are in different states of coherence. The method becomes important when it is necessary to calculate the power transferred from a distributed source S to a distributed load L through a length of multimode metallic, or dielectric, waveguide. It is shown that if the correlations between the transverse components of the electric and magnetic fields of S and L are described by coherence matrices M and M', respectively, then the normalized average power coupled between them is (eta) = Tr[MM']/Tr[M]Tr[M'], where Tr denotes the trace. When the modal impedances are equal, this expression for the coupled power reduces to an equation derived in a previous paper [J. Opt. Soc. Am. A 18, 3061 (2001)], by use of thermodynamic arguments, for the power coupled between partially coherent free-space beams.
More details from the publisher
More details

Microwave transmission through high-temperature superconducting waveguides

Physica C: Superconductivity and Applications 372-376 (2002) 532-525

Authors:

G Yassin, G. Dikovsky, V. Barboy, I. Kambara
More details from the publisher

Non-linear two-frequency analysis of SIS mixers through harmonic balance

J PHYS IV 12:PR3 (2002) 165-168

Authors:

S Withington, P Kittara, G Yassin

Abstract:

We present a numerical procedure for simulating the non-linear behaviour of Superconductor-Insulator-Superconductor (SIS) tunnel-junction mixers. Mixers of this kind are used extensively in high-performance submillimetre-wave astronomical receivers. The procedure is complete in that both the signal and local-oscillator voltages can be at high levels, with significant amounts of harmonic content; also, the full quantum mechanical behaviour of the tunnel junction is taken into account. The initial simulations show that multi-tone analysis can be carried out in a numerically efficient manner, and that saturation, and the attendant generation of IF harmonics, can be modelled rigorously. This work constitutes the first full non-linear model of an SIS mixer, arid the theoretical and numerical procedures described, will be of great importance when designing the next generation of heterodyne astronomical receivers.
More details from the publisher
More details

Pagination

  • First page First
  • Previous page Prev
  • …
  • Page 11
  • Page 12
  • Page 13
  • Page 14
  • Current page 15
  • Page 16
  • Page 17
  • Page 18
  • Page 19
  • …
  • 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