The invention of the laser in the early 1960s led to experiments where high power (> million Watts) infra-red and visible pulsed lasers were focused onto solid targets in order to produce hot (> 0.5 million degrees Kelvin) plasmas. In almost 50 years of study, the physics of the laser interaction, the physics of the expanding plume and many important applications have been elucidated in some detail. When focussed onto solid targets, visible/infra-red lasers do not penetrate to the solid for most of the pulse duration, but are absorbed in the expanding plasma plume at densities 100- 1000 times smaller than the solid density. Dropping the laser wavelength into the extreme ultra-violet (EUV), however, enables the laser to penetrate into the solid and to create plasma directly at the solid density. Initial modelling studies that have been undertaken by the PI show that the interaction of EUV laser radiation with most solid targets will cause a rapid drop in opacity (so that the target 'bleaches'). Initially an attenuation length for the EUV photon energy is bleached and then another attenuation length, so that a 'bleaching wave' propagates through the solid target on a sub-nanosecond timescale. A much more massive amount of target material is effectively ablated than can occur with infra-red or visible radiation of the same pulse energy and focal spot diameter. Little modelling work has been undertaken to elucidate understanding of EUV laser-produced plasmas because of the lack of sufficiently energetic (> 10 microJoules) laboratory EUV lasers for experiments. However, reliable capillary discharge lasers operating at wavelength 46.9 nm (photon energy 26.4 eV) producing up to 1 milliJoule/pulse and peak powers of a million Watts have been developed at the Colorado State University (CSU). We propose to develop simulation models to interpret emission spectra and mass spectrometer results from EUV laser produced plasmas. We will test spectrometer diagnostics using the University of York high power infra-red laser and in collaboration with CSU make spectral and mass spectrometer measurements for comparison to the simulation models. A new class of laser-produced plasma will be studied with potential impact in the study of warm dense matter, laser cutting and ablation and solid material lithography with relevance to the $70B p.a. revenue industry associated with the manufacture of microelectromechanical systems (MEMS).

Our research with the particle physics rolling grant at Sheffield attempts to progress understanding of some of the most important questions concerning the origins and make-up of the Universe. One of these big questions is to understand what gives fundamental particles their mass. Part of our work on the huge ATLAS experiment at the Large Hadron Collider (LHC) at CERN in Geneva is aimed at this question, in particular to see if the famous Higgs Boson particle exists. The best theories we have to explain particle mass predict that it should be there. We will play a key role in analysing the vast amount of data soon expected to make this exciting discovery. Another search at ATLAS will be to determine if the so-called supersymmetry (SUSY) theory is correct. This is our best prospect for understanding how particles interact at high energy and itself predicts a new class of particles. The concept states that for every known fundamental particle there exists a super-partner particle. We worked for many years developing the key silicon technology now installed in ATLAS to search for these particles. Now we are ready with our software to play a key role in analysing the data that will hopefully discover that they exist. One of the implications of SUSY theory is the likelihood that the most stable new particle, the so-called lightest supersymmetric particle (LSP), probably is very abundant throughout the Universe, making up about 25% of its mass. This would easily explain one of the big mysteries in physics, the so-called Dark Matter seen by astronomers from its gravitational effects on stars and galaxies. Our group has pioneered techniques to search directly for dark matter particles in the laboratory and is participating in a new multi-national venture, EURECA. This will build a tonne-sized device using low temperature superconductors to perform a new search. We will contribute to the key aspect of how to shield the experiment from natural background particles, like muons. Another mystery in the Universe are the strange properties of its most abundant particle, the neutrino. This has only recently been found to have a small mass and to readily change form between three different 'flavours' while propagating through space. Details of this are not fully understood but it is known that if properly unravelled it might answer another big question, why there is so little anti-matter in the Universe. We are working on these questions through participation in the big international T2K neutrino beam experiments in Japan. We are building a key component of the detectors and will, within two years, start to analyse the data to unravel these issues. T2K probably will not do a full job, so we have instigated in the UK work on a new neutrino detector concept, based on liquid argon, contributing to the FJNE programme. We plan to build test devices to enable the next generation of neutrino experiments to follow T2K. This is linked also to our work on accelerator technology, MICE, where we are building test beam targets. This is a vital step towards the ultimate facility, a neutrino factory. We are working on key technology for this within the UKNF project. Finally, much of the hardware and computer code developed for these fundamental studies have great relevance well outside our main research. There are many examples, involving projects with a dozen UK companies. For instance, our work with Corus Ltd. on new techniques for neutron detection, has allowed development of new monitors to detect illicit transport of nuclear materials at ports. This will continue now and broaden into medical applications. Our dark matter work has produced a new national facility for underground science, the Boulby laboratory. Here we have started a new project on climate change, SKY, to explore the effect of comic rays on cloud formation.

The Cranfield IMRC vision is to grow the existing world class research activity through the development and interaction between:Manufacturing Technologies and Product/Service Systems that move UK manufacturing up the value chain to provide high added value manufacturing business opportunities.This research vision builds on the existing strengths and expertise at Cranfield and is complementary to the activities at other IMRCs. It represents a unique combination of manufacturing research skills and resource that will address key aspects of the UK's future manufacturing needs. The research is multi-disciplinary and cross-sectoral and is designed to promote knowledge transfer between sectors. To realise this vision the Cranfield IMRC has two interdependent strategic aims which will be pursued simultaneously:1.To produce world/beating process and product technologies in the areas of precision engineering and materials processing.2.To enable the creation and exploitation of these technologies within the context of service/based competitive strategies.

1. The purpose of the project Development and commercialization of imaging detectors using artificial diamond technology to provide greatly enhanced performance. 2. Introduction The need to detect fast signals is crucial in many disciplines. Very high speed, low amplitude light signals need signal amplification. The photomultiplier tube (PMT) was the first device to use electronic signal amplification in a vacuum tube for optical light and has been a workhorse detector since. Though silicon chips have replaced vacuum tubes as the technology of choice in most imaging applications they have limited high speed and sensitivity performance compared with devices such as the PMT. The aim of this project is to apply detector technology and know-how from the Space Research Centre (SRC), Leicester, developed through space science R & D, together with recent developments in diamond chemistry at the Diamond Group, Bristol, to the commercialization of an imaging PMT with ground-breaking performance for widespread commercial application and specific relevance to the defence sector / fusion plasma diagnostics at the Atomic Weapons Establishment, Aldermaston. 3. Advantages of Diamond as an electron amplification material a) High gain: Diamond is one of a small number of materials which has high electron gain when correctly treated. b) Simplified design: Diamond can have a higher gain per amplification stage, resulting in a lower number of stages being required for a given gain. c) Enhanced timing: The amplification properties of diamond allow improved signal timing and reduced background. d) Lower gain variability: The higher gain of diamond reduces the variability in the gain. e) Low noise: Diamond is less susceptible to thermal noise so it can operate with lower noise levels or at higher temperatures. f) Large area: Synthetic diamond offers low cost, large area coating and is easily grown on shaped surfaces. g) Stability: Synthetic diamond has a stable performance over long periods. Its performance remains high after exposure to air. The electron gain properties of synthetic diamond promises to greatly expand the usage of PMTs in many fields. 4. Application of synthetic Diamond to Detectors We have already measured the performance of synthetic diamond and our measured data supports published results and demonstrates the potential benefits of synthetic diamond as a detector material. This project will transfer the technology from proof-of-concept to prototype, beginning with optimization of manufacturing processes. Firstly we will manufacture two demonstrator detectors to provide data on process optimization. The next stage of the project will be development of a single transmissive gain stage. Transmissive dynodes can operate in two modes: - a) Transmission: input electrons enter through one surface of a thin film of diamond, and output electrons exit through the other. b) Refection: diamond is deposited on an open conductive wire mesh. Input and output electrons enter and exit through the same diamond surface. The transmission technique is superior, providing better detector performance, but is more demanding because of the need to produce very thin films, however we have already demonstrated manufacture. We will investigate both techniques and choose the optimum technology based on performance, manufacturability, developmental and manufacturing costs, and development timescale. We will initially demonstrate a single stage transmissive gain stage to provide comprehensive device diagnostics. The final stage of the project is to design, build and demonstrate a detector using a stack of gain stages with fast response and high gain and incorporating an imaging capability. Performance evaluation will involve testing with AWE collaborators at Aldermaston and field trials in a laser fusion facility at Los Alamos, and in photon counting mode at Photek and SRC.

Understanding how the structure and physical properties of materials change under extremes of pressure and temperature is essential if we are to develop predictive capabilities on how materials work under such conditions, thereby driving innovation in material design and engineering for the improved materials of tomorrow. Much progress has been made in the last 20 years, to the extent that our understanding of how the crystallographic and electronic structure of matter changes when it is compressed to very high pressures has transformed completely in that time. However, the lack of suitable technologies has severely limited our ability to tackle two key "known unknowns": how do pressure-induced structural changes occur in elements, and how are the microstructure and physical properties of more complex materials, such as key binary alloys, affected by extreme pressures and temperatures. We will exploit our team's expertise in experimental high-pressure physics, combined with recent advances in high repetition rate lasers, and the unprecedented brightness and spatial coherence of next generation synchrotron and x-ray free electron laser facilities, to make definitive studies of phase transitions, transition mechanisms, microstructure, and material strength in key elemental and alloy systems using x-ray diffraction and imaging. In collaboration with our Project Partners, we will then use electronic structure calculations to understand the physics behind the observed material response, and thereby develop new understanding and improved predictive capabilities in the behaviour of matter at extreme conditions.