Bulletin of the American Physical Society
60th Annual Meeting of the APS Division of Plasma Physics
Volume 63, Number 11
Monday–Friday, November 5–9, 2018; Portland, Oregon
Session TP11: Poster Session VII: Basic Plasma Physics: Pure Electron Plasma, Strongly Coupled Plasmas, Self-Organization, Elementary Processes, Dusty Plasmas, Sheaths, Shocks, and Sources; Mini-conference on Nonlinear Waves and Processes in Space Plasmas - Posters; MHD and Stability, Transients (2), Runaway Electrons; NSTX-U; Spherical Tokamaks; Analytical and Computational Techniques; Diagnostics (9:30am-12:30pm)
Thursday, November 8, 2018
OCC
Room: Exhibit Hall A1&A
Abstract ID: BAPS.2018.DPP.TP11.40
Abstract: TP11.00040 : Measurement of Correlation-Enhanced Collision Rates in the Mildly Correlated Regime (Γ≈1)*
Presenter:
Francois Anderegg
(Univ of California - San Diego)
Authors:
Francois Anderegg
(Univ of California - San Diego)
Daniel H.E. Dubin
(Univ of California - San Diego)
C. Fred Driscoll
(Univ of California - San Diego)
We have measured correlation-enhanced perpendicular-to-parallel collision rates νperp-par in cryogenic, strongly magnetized mildly correlated ion plasmas. The enhancement of νperp-par is directly analogous [1] to the correlation-enhancement of fusion collisions in hot dense stellar plasma, as first analyzed by Salpeter [2]. The enhancement occurs because plasma screening reduces the repulsive Coulomb potential between charges, allowing closer collisions for a given relative energy.Correlations are parameterized by Γ=e2/aT which is the ratio of the nearest neighbor potential energy to the ion thermal energy. Our prior measurements [3] over the range 0 < Γ < 15 observed enhancement up to 107x, in broad agreement with Salpeter “equilibrium screening” theory. However recent “dynamical screening” theories [4] predict negligible enhancement for Γ≈1.
In our magnesium ion plasmas, we obtain Γ≈1 at densities n=2x107cm-3 and temperatures T≈5x10-5eV. After improving lasers stability, we can rule out dynamical screening theories.
[1] D.H.E. Dubin, Phys. Plas. 15, 055705, (2008); [2] E.E. Salpeter, Austr. J. Phys., 7, 373, (1954); [3] F. Anderegg et.al., PRL, 102, 185001, (2009); [4] W. Däppen and K. Mussack Contr. Plas. Phys. 52, 149, (2012).
*DOE Grants DE-SC0008693, and DE-SC0018236
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.TP11.40
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