50th Annual Meeting of the Division of Plasma Physics
Volume 53, Number 14
Monday–Friday, November 17–21, 2008;
Dallas, Texas
Session XR0: Celebration of Plasma Physics Plenary Presentations IV
8:00 AM–9:12 AM,
Friday, November 21, 2008
Room: Landmark A/B
Chair: Ian Hutchinson, Massachusetts Institute of Technology
Abstract ID: BAPS.2008.DPP.XR0.2
Abstract: XR0.00002 : Perspectives on High-Energy-Density Physics*
8:36 AM–9:12 AM
Preview Abstract
Abstract
Author:
R. Paul Drake
(University of Michigan)
Much of 21st century plasma physics will involve work to produce,
understand, control, and exploit very non-traditional plasmas.
High-energy density (HED) plasmas are often examples, variously
involving strong Coulomb interactions and few particles per
Debeye sphere, dominant radiation effects, strongly relativistic
effects, or strongly quantum-mechanical
behavior. Indeed, these and other modern plasma systems often
fall outside the early standard theoretical definitions of
``plasma''. This presentation will focus on two types of HED
plasmas that exhibit non-traditional behavior.
Our first example will be the plasmas produced by extremely
strong shock waves. Shock waves are present across the entire
realm of plasma densities, often in space or astrophysical
contexts. HED shock waves (at pressures $>$ 1 Mbar) enable
studies in many areas, from equations of state to hydrodynamics
to radiation hydrodynamics. We will specifically consider
strongly radiative shocks, in which the radiative energy fluxes
are comparable to the mechanical energy fluxes that drive the
shocks. Modern HED facilities can produce such shocks, which are
also present in dense, energetic, astrophysical systems such as
supernovae. These shocks are also excellent targets for advanced
simulations due to their range of spatial scales and complex
radiation transport.
Our second example will be relativistic plasmas. In general,
these vary from plasmas containing relativistic particle beams,
produced for some decades in the laboratory, to the relativistic
thermal plasmas present for example in pulsar winds. Laboratory
HED relativistic plasmas to date have been those produced by
laser beams of irradiance $\sim $ 10$^{18}$ to 10$^{22}$
W/cm$^{2}$ or by accelerator-produced HED electron beams. These
have applications ranging from generation of intense x-rays to
production of proton beams for radiation therapy to acceleration
of electrons. Here we will focus on electron acceleration, a
spectacular recent success and a rare example in which simplicity
emerges from the complexity present in the
plasma state.
*Sponsored by DOE/NNSA Predictive and Stewardship Sciences Academic Alliances through DOE Research Grants DE-FC52-08NA28616 and DE-FG52-04NA00064, and by other grants and contracts.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2008.DPP.XR0.2