Wire Array Z-Pinch Driven High Energy Density Physics Experiments

Lead Research Organisation: Imperial College London
Department Name: Physics

Abstract

High Energy Density Physics (HEDP) studies the behaviour of matter in extremes of temperature, density and pressure. Often this involves heating material to millions of degrees, or subjecting it to Mega-bars of pressure, increasing its density to many times beyond that normally encountered. HEDP is becoming increasingly important to both science and industry / for instance HEDP describes the behaviour of matter in the sun and planetary cores, whilst applications of HEDP include the manufacture of more refined integrated circuits, helping provide the year on year increase in computing power. Perhaps the greatest application of HEDP is yet to emerge: the creation of controlled nuclear fusion, providing a clean energy source of near unlimited reserves.Experiments continually push the boundaries of HEDP, exploring both the fundamental physics issues at its heart, and science that uses these phenomena as its basis. In order to expand the densities, temperatures and pressures available for HEDP studies some of the worlds largest scientific facilities are under construction, including lasers capable of delivering millions of joules of energy in billionths of a second. Further, in order to understand these experiments the worlds most powerful supercomputers are built.The facilities required to perform HEDP experiments are usually large and expensive to run, limiting access to university researchers. This proposal seeks to develop a new source for HEDP experiments that could examine phenomena complementary to those investigated at large facilities, in a system that can be scaled down to university laboratories. To achieve this large, fast rising currents (millions of amps being generated in fractions of a microsecond) will be applied to cylindrical arrangements of fine metallic wires, producing what is known as a wire array z-pinch. Initially the wires in an array gradually 'boil' into plasma*, whilst the magnetic field created around the wires sweeps the plasma towards the axis of the array. Accumulation of material from each of the wires at the axis results in the formation of a dense, stable 'precursor' plasma column with a temperature of millions of degrees. The wires continue to act as sources of plasma until the majority of their mass has been removed, triggering the start of the arrays 'implosion'. This sweeps up plasma on its way towards the axis, accelerating it to speeds in excess of 200kms-1 - at which point it has the same kinetic energy as a tank shell. Colliding with the precursor the implosion releases terrawatts (1000 000 000 000s of watts) of X-rays in a pulse lasting a fraction of a millionth of a second.This fellowship will focus on ways to use the plasma and X-ray pulse from an array to study HEDP phenomena. Measurements of the material in the precursor plasma column will be used to provide information on energy transport mechanisms in stars. The precursor will also be redirected out of the array into a hypersonic plasma jet, which will be impacted onto target materials, driving them unstable over extremely long times. This data will be compared to fluid models that determine processes including the efficiency of fusion reactions and the formation of nebulae. In a final set of experiments the implosion of an array will be focussed to a tight point rather than a long column, significantly increasing the already huge temperatures available to experimenters. All of this work will be in a basement of a university in South Kensington. * Plasma is the 4th state of matter after solids, liquids and gases. Heating a solid it melts into a liquid, then this boils into a gas. If we continue to heat a gas the electrons will aquire enough energy to leave their orbits around the gas nuclei; hence plasma is often referred to as an ionised gas. Like metals, plasmas can be excellent conductors, and are subject to magnetic and electrical forces.

Publications

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Description The EPSRC fellowship has helped enable the use of cheap, robust, Mega-Ampere pulsed power systems to drive new high energy density physics experiments, attaining conditions that compliment those available at large - national scale - laser laboratories. The energy densities available in experiments with pulsed power sources were significantly increased through use of radial wire array z-pinch loads. During the course of the fellowship a Laboratory Directed Research Development project was launched with Sandia National Laboratories, which saw the technology transferred to experiments on the multi-million dollar Saturn facility, where X-ray emission from the radial wire array was evaluated for energising hohlraums, which could then be used to drive separate HEDP experiments, and as a direct source for radiation effects testing.
In separate experiments at Imperial College, the use of novel z-pinch configurations as extremely fast current switches has been explored. This demonstrated that the rise time of the current pulse could be significantly shortened - enabling the use of very cheap pulsed power generators based on simple capacitor discharge (which would normally be too slow for driving HEDP experiments). Further it was found that the fast switch configuration allowed a controllable current pre-pulse to be injected into attached loads. This altered the subsequent dynamics of the load, enabling the creation of extremely dense plasma implosions, which could form the basis of new methods to compress and heat fusion fuel.
During the fellowship the use of pulsed power to create plasma jets and shocks that can be scaled to those observed astrophysical scenarios has significantly increased. Multi-centimetre scale shocks, travelling at 10s of kms-1 have been launched through a variety of gases to explore shock wave stability and radiative cooling effects. The shocks appear to be magnetically supported, and attempts have been made to shape the resultant shock waves into planar and convergent forms. Dense, high MACH number plasma jets have been interacted with solid targets, resulting in the formation of reverse shocks and a highly radiating 'stationary' shock structure that is consistent with magnetic field, entrained in the flow of plasma, being compressed close to the target. Further, the interaction of 2 jets with each other has been studied, resulting in bow shock structures, with highly unstable - possibly turbulent - working surfaces. Finally, as part of the fellowship, progress has been made with the development of high resolution XUV spectrometry and imaging techniques, enabling the atomic properties of dense, highly radiating plasmas to be studied.
Exploitation Route Many of the techniques developed during the grant have been used by colleagues in the US and UK - in particular the use of the plasma from wire arrays to drive expts in astrophysics.
Colleagues in the US now use X-pinch driven absorption spectrometry. The use of the X-pinch source has also been followed up in experiments with colleagues at the CEA, and will be further explored at ESRF this summer, where we hope to examine the extremely high pressures and densities predicted.
Sectors Aerospace, Defence and Marine,Education,Manufacturing, including Industrial Biotechology

 
Description The idea of using an X-pinch to provide a broadband X-ray backlighter source has been used by collaborators at Cornell University to explore the the absorption properties of dense aluminium plasmas. Now being further developed in experiments at Imperial College, this technique will enable better modelling of atomic processes, which effects out understanding of many astrophysics phenomena - e.g the radiative properties of stellar atmospheres. One part of the fellowship involved the creation of compact X-ray sources to couple to small hohlraums. This was subject to a set of joint experiments with a US National Laboratory; and - along with several other techniques developed by Dr Bland and his colleagues - is being discussed as a subject for joint experiments with researchers at National Laboratories in China. The creation of compact sources, will enable higher temperature radiation drives to be developed at smaller facilities - potentially helping the effort to create controlled nuclear fusion as a power source. Finally, convergent geometry techniques for the creation of materials under extreme conditions - initially considered by Dr Bland and his colleagues during the fellowship - are now being explored. These are enabling/will enable the production of new, exotic forms of materials, which could significantly affect multiple areas of research and industry - from the creation of new lighter, stronger alloys; to high energy density storage systems; to a better understanding of star and planet formation.
Sector Aerospace, Defence and Marine,Energy,Manufacturing, including Industrial Biotechology,Security and Diplomacy,Other
Impact Types Cultural,Economic

 
Description Experimental Platform for Hypersonic Testing Using Pulsed Power Driven Dense Plasma Flows
Amount £285,000 (GBP)
Organisation US Air Force European Office of Air Force Research and Development 
Sector Public
Country United Kingdom
Start 12/2016 
End 12/2019
 
Description NNSA Centre of Excellence, funded by US DoE
Amount £705,000 (GBP)
Funding ID Subcontract for National Nuclear Securities Administration 
Organisation U.S. Department of Energy 
Sector Public
Country United States
Start 10/2012 
End 09/2017
 
Description PMI2 Connect
Amount £30,400 (GBP)
Funding ID
Organisation British Council 
Sector Charity/Non Profit
Country United Kingdom
Start 09/2008 
End 08/2010
 
Description X-ray spectroscopic studies of X-pinch plasmas with 3-5 picosecond resolution: a quest for clear experimental evidence for radiative collapse
Amount £59,000 (GBP)
Organisation U.S. Department of Energy 
Sector Public
Country United States
Start 10/2017 
End 10/2020
 
Company Name Aqua21 
Description Founded by Trevor Costello, Aqua21 is a company dedicated to providing cheap ozone production systems to clean water at all scales, but in particularly at small scales suitable for local cleaning at point of use, and for use in disaster relief. The company approached me in 2010 to help design their ozone generators and sensors, and I used technical knowledge acquired whilst working on several grants to enable this... reducing cost and size of equipment be orders of magnitude. 
Year Established 2010 
Impact Runner up in St Andrews environmental prize in 2012. The technology is presently being tested at Scottish Water.
Website http://www.aqua21.co.uk/?page_id=121