INVESTIGATION OF K-SHELL EMISSION FROM MODERATE-Z, LOW-ETA (-VELOCITY), Z-PINCH IMPLOSIONS

Citation
Jw. Thornhill et al., INVESTIGATION OF K-SHELL EMISSION FROM MODERATE-Z, LOW-ETA (-VELOCITY), Z-PINCH IMPLOSIONS, Journal of applied physics, 80(2), 1996, pp. 710-718
Citations number
22
Categorie Soggetti
Physics, Applied
Journal title
ISSN journal
00218979
Volume
80
Issue
2
Year of publication
1996
Pages
710 - 718
Database
ISI
SICI code
0021-8979(1996)80:2<710:IOKEFM>2.0.ZU;2-6
Abstract
Because of the large amount of kinetic energy and mass needed for effi cient production of K-shell emission from moderate atomic number z-pin ch plasmas (Z>22), moderate Z experiments performed in the near future will likely take place at relatively low implosion velocities or low- eta values, where eta is defined as the ratio of lire maximum kinetic energy per ion generated prior to stagnation to the minimum energy per ion, E(min) needed to instantly heat and to ionize a plasma into the K shell upon stagnation of the pinch. Since there has been no systemat ic theoretical or experimental investigations of K-shell yield scaling with mass and atomic number in the low-eta regime eta similar to 1-3, in anticipation of such future experiments, we report on the results of our theoretical investigation into this regime. in particular alumi num, argon, titanium, and krypton plasmas were studied using a 1D radi ation hydrodynamics model that uses enhanced transport coefficients to phenomenologically attain the stagnation conditions of experimental z -pinches, The results of this study have identified the following impo rtant effects: low-eta plasmas remain in an inefficient mass(2) (or cu rrent(4)) scaling regime at much higher masses than predicted by our e arlier work,(1,2) which was based on eta > 3.7 calculations. Thus, mor e energy than predicted by the earlier scaling laws will apparently be needed to obtain significant amounts of, for example, krypton K-shell emission. In addition; lags in ionization times become important incr easingly with the Z of the plasma and adversely affect K-shell emissio n. The physics responsible for these time dependent effects and how th ey will influence the design of future experiments are discussed.