A view of OPMD

OPMD

The Oxford Physics Microstructure Detector (OPMD) laboratory is equipped with state-of-the-art instrumentation to evaluate sensors in the laboratory before and after irradiation as well as to build detector assemblies.
Experimental team at the commissioning experiment of the HED station of the European XFEL.

Oxford Centre for High Energy Density Science (OxCHEDS)

The Oxford Centre For High Energy Density Science (OxCHEDS) brings together groups from across Atomic and Laser physics (and beyond) with an interest in the study of matter under extreme conditions.
HFSP meeting in Hokkaido

Oxford Molecular Motors

We are currently working on Rotary Molecular Motors. In particular the Bacterial Flagellar Motor and F1FO ATP-synthase. The aim is to try and understand how these living machines work. We use a range of techniques. Molecular motors are tens of nanometre
Magnetic vortices in Fe2O3

Oxide electronics

We study novel quantum materials with the potential for integration in a new generation of fast, non-volatile memories and other electronic devices. Our current emphasis is on magnetic oxides which can be controlled by electric fields.
A blackboard of work in the Beecroft Building

Particle theory

We develop mathematical theories to describe the fundamental properties of nature and explore their implications
Group photo from Feb 2019

Photovoltaic and optoelectronic device group

The Photovoltaic and Optoelectronic device group is led by Prof Henry Snaith. Our main interest is in metal halide perovskites for photovoltaic and light emitting applications.
ocean eddies

Physical oceanography

Physics of the circulation and structure of the global ocean and its impacts on climate
contera lab

Physics of biological shape: from molecules to organisms and biohybrid structures

Physics and nanomechanics at the interface of biology and nanotechnology, in molecules, cells, tissues (artificial or natural) and whole organisms. Atomic force microscopy. Led by Professor Sonia Contera
Image of Saturn from NASA Cassini

Planetary atmosphere observation analysis

Atmospheric observation data analysis of planets.
Concept map for Planetary Climate Dynamics

Planetary Climate Dynamics

Processes governing planetary climate and its evolution over time
Enceladus' Damascus Sulcus. This image was generated by combining high resolution images of Enceladus acquired in August 2008 at 12 to 30 meters (40 to 100 feet) resolution with a topographic map.

Planetary surfaces

Investigating the surfaces of (primarily airless) bodies in our solar system.