Published October 2011 | Version v1
Journal article

Anomalous evolution of Ar metastable density with electron density in high density Ar discharge

  • 1. Department of Physics, Korea Advanced Institute of Science and Technology, Daejeon 305-701 (Korea, Republic of)
  • 2. Center for Vacuum Technology, Korea Research Institute of Standards and Science, Daejeon, 305-306 (Korea, Republic of)

Description

Recently, an anomalous evolution of argon metastable density with plasma discharge power (electron density) was reported [A. M. Daltrini, S. A. Moshkalev, T. J. Morgan, R. B. Piejak, and W. G. Graham, Appl. Phys. Lett. 92, 061504 (2008)]. Although the importance of the metastable atom and its density has been reported in a lot of literature, however, a basic physics behind the anomalous evolution of metastable density has not been clearly understood yet. In this study, we investigated a simple global model to elucidate the underlying physics of the anomalous evolution of argon metastable density with the electron density. On the basis of the proposed simple model, we reproduced the anomalous evolution of the metastable density and disclosed the detailed physics for the anomalous result. Drastic changes of dominant mechanisms for the population and depopulation processes of Ar metastable atoms with electron density, which take place even in relatively low electron density regime, is the clue to understand the result.

Additional details

Identifiers

Publishing Information

Journal Title
Physics of Plasmas
Journal Volume
18
Journal Issue
10
Journal Page Range
p. 103510-103510.7
ISSN
1070-664X
CODEN
PHPAEN

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
44006468
Subject category
S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
Descriptors DEI
ARGON; ATOMS; ELECTRIC DISCHARGES; ELECTRON DENSITY; IONIZATION; METASTABLE STATES; PLASMA; PLASMA DENSITY
Descriptors DEC
ELEMENTS; ENERGY LEVELS; EXCITED STATES; FLUIDS; GASES; NONMETALS; RARE GASES

Optional Information

Notes
(c) 2011 American Institute of Physics