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Atomic and Laser Physics
Credit: Jack Hobhouse

Professor Steven Rose

Visiting Professor

Research theme

  • Lasers and high energy density science

Sub department

  • Atomic and Laser Physics

Research groups

  • Oxford Centre for High Energy Density Science (OxCHEDS)
Steven.Rose@physics.ox.ac.uk
Imperial College London webpage
  • About
  • Publications

Modelling K shell spectra from short pulse heated buried microdot targets

HIGH ENERGY DENSITY PHYSICS 23 (2017) 178-183

Authors:

DJ Hoarty, N Sircombe, P Beiersdorfer, CRD Brown, MP Hill, LMR Hobbs, SF James, J Morton, E Hill, M Jeffery, JWO Harris, R Shepherd, E Marley, E Magee, J Emig, J Nilsen, HK Chung, RW Lee, SJ Rose
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Measurements of plasma spectra from hot dense elements and mixtures at conditions relevant to the solar radiative zone.

ATOMIC PROCESSES IN PLASMAS (APIP 2016) 1811 (2017)

Authors:

DJ Hoarty, E Hill, P Beiersdorfer, P Allan, CRD Brown, MP Hill, LMR Hobbs, SF James, J Morton, N Sircombe, L Upcraft, JWO Harris, R Shepherd, E Marley, E Magee, J Emig, J Nilsen, SJ Rose
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Particle Interactions in High-Temperature Plasmas Supervisor's Foreword

Chapter in PARTICLE INTERACTIONS IN HIGH-TEMPERATURE PLASMAS, (2017) V-V
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Sherlock et al. Reply

Physical Review Letters American Physical Society 116 (2016) 159502

Authors:

M Sherlock, W Rozmus, EG Hill, Steven J Rose
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Transport coefficients of a relativistic plasma

Physical Review E - Statistical Physics, Plasmas, Fluids, and Related Interdisciplinary Topics American Physical Society 93:5 (2016) 1-16

Authors:

Steven J Rose, Oliver J Pike

Abstract:

In this work, a self-consistent transport theory for a relativistic plasma is developed. Using the notation of Braginskii [S. I. Braginskii, in Reviews of Plasma Physics, ed. M. A. Leontovich (1965), Vol. 1, p.174], we provide semi-analytical forms of the electrical resistivity, thermoelectric and thermal conductivity tensors for a Lorentzian plasma in a magnetic field. This treatment is then generalized to plasmas with arbitrary atomic number by numerically solving the linearized Boltzmann equation. The corresponding transport coefficients are fitted by rational functions in order to make them suitable for use in radiation-hydrodynamic simulations and transport calculations. Within the confines of linear transport theory and on the assumption that the plasma is optically thin, our results are valid for temperatures up to a few MeV. By contrast, classical transport theory begins to incur significant errors above kBT ~ 10 keV, e.g., the parallel thermal conductivity is suppressed by 15% at kBT = 20 keV due to relativistic effects
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