JP9955054 Density-Matrix Description of Polarized Atomic Radiative Emission in Electric and Magnetic Fields V. L. Jacobs Institute for Plasma Research, University of Maryland, College Park, MD 20742-3511 and Complex Systems Theory Branch, Code 6693, Condensed Matter and Radiation Sciences Division, Naval Research Laboratory, Washington, D. C. 20375-5345 (Permanent Address) A. B. Filuk (Deceased) Ion Beam Generation Department, Organization 9533, MS 1186, Sandia National Laboratories, P. O. Box 5800, Albuquerque, New Mexico 87185-1186 (For Submission to the Proceedings of the Japan-U. S. Workshop and International Seminar on Plasma Polarization Spectroscopy, 26-28 January, 1998, Kyoto, Japan) February, 1998 — 187 — ABSTRACT A density-matrix description has been developed for the investigation of the angular distribution and polarization of radiative emission during single-photon atomic transitions in the presence of a general arrangement of static (or quasi-static) electric and magnetic fields. Particular emphasis has been given to the influence of directed collisional excitations, which may be produced by an anisotropic incident-electron velocity distribution. We have allowed for the possibility of the coherent excitation of the nearly degenerate field-dependent atomic substates. Coherent excitations may be produced by non-parallel electric and magnetic fields. Our main result is a general expression for the matrix elements of the photon-polarization density operator. This expression provides a unified framework for the analysis of the total intensity, angular distribution, and polarization of the Stark-Zeeman spectral patterns. For the observation of radiative emission in the direction of the magnetic field, the detection of linearly polarized emissions, in addition to the usual circularly polarized radiations, can reveal the presence of a perpendicular electric field or a coherent excitation mechanism. — 188 — I. INTRODUCTION Polarized radiative emission can occur as a result of a nonuniform (or nonstatistical) distribution of the population densities of the excited atoms (or ions) among the degenerate (or nearly degenerate) angular-momentum magnetic sublevels. A nonuniform distribution of population densities among the magnetic sublevels can be produced by, for example, directed electron or ion beam excitation, laser photon excitation, or the action of perturbing electric or magnetic fields. The measurement and analysis of the polarization of the atomic radiative emission can provide information on the nature of the excitation mechanisms and the strength of the electric or magnetic fields. We have been concerned with applications of the density-matrix description of polarized atomic radiative emission to spectroscopic observations in electric and magnetic fields. Particular interest has been directed at radiative emission in the intense crossed electric and magnetic fields generated by the applied-B ion diodes of the Particle Beam Fusion Accelerators PBFA II and SABRE at Sandia National Laboratories (Bailey et al., 1995; Filuk et al., 1996). Our theoretical investigation has also been motivated by magnetic field measurements in tokamak plasmas, allowing for the Zeeman and the motional-Stark effects (Huang, Wroblewski, Finkenthal, and Moos, 1989; Ida et al., 1998). Electric and magnetic fields may also play an important role in the production of polarized radiative emission by the anisotropic electron velocity distributions in the Electron Beam Ion Trap (EBIT) devices at the Lawrence Livermore National Laboratory (Beiersdorfer et al., 1996) and at the National Institute of Standards and Technology (Takacs et al., 1996). Finally, magnetic fields are now believed to influence the electric-field induced enhancement of — 189 — dielectronic recombination radiation that is observed in electron-ion beam interactions (Savin et al., 1996; Bartsch et al., 1997). In our analysis of polarized atomic radiative emission, we shall allow for a general set of steady-state excitation processes in the presence of an arbitrary arrangement of static (or quasi-static) electric and magnetic fields. The geometry for spectroscopic observations in crossed electric and magnetic fields is illustrated in Fig. 1. We will be concerned with applications for which the total magnetic field acting on the radiating atomic system is the sum of an external (applied) magnetic field and an internal (dynamical) magnetic field. Examples of the dynamical magnetic field include the nearly parallel magnetic field that is due to electron diamagnetic compression of flux in the anode-cathode region of an applied-B ion diode (PBFA II) and the perpendicular poloidal magnetic field in a tokamak plasma. The viewing angle e is taken to be parallel to the applied magnetic field in PBFA II and perpendicular to the known toroidal magnetic field in the case of a tokamak plasma. Our theoretical description of polarized atomic radiative emission has been developed within the framework of the density-matrix approach. The theory of polarized radiative emission following directed-electron collisional excitation of an atomic system (in the absence of electric and magnetic fields) was first presented by Oppenheimer (1927) and subsequently refined by Percival and Seaton (1958). A density-matrix approach has been presented by Inal and Dubau (1987, 1989). A density-matrix description for dielectronic recombination radiation has been developed by Shlyaptseva, Urnov, and Vinogradov (1981, 1992). We have employed the formalism advanced in our density-matrix description of the angular distribution and polarization in single- and multi-photon ionization processes (Jacobs, 1972; 1973), as well as the formulation presented by Inal and Dubau (1987, 1989). The density-matrix approach can provide a fundamental description of the coherent excitation of the atomic states. — 190 II. DENSITY-MATRIX DESCRIPTION In our description of polarized atomic radiative emission in electric and magnetic fields, we have employed the density matrix formalism. The density-matrix formalism has been discussed by Fano (1957), Jacobs (1972, 1773), Blum (1996), and by Kazantsev and J.-C. Henoux (1995). We have assumed that the total Hamiltonian, describing the many- electron atomic system in the presence of an arbitrary arrangement of static (or quasi-static) electric and magnetic fields, has been diagonalized in a basis set consisting of discrete and continuum field-free eigenstates. The atomic excitation and spontaneous radiative emission processes are treated as independent events. The initial excited state is represented by a density matrix, whose diagonal elements give the familiar population densities and whose non-diagonal elements correspond to the coherences (Blum, 1996). A brief account of our description of polarized radiative emission has been published (Jacobs and Filuk, 1995). The steady-state (frequency-integrated) intensity, angular distribution, and polarization of the radiation that is emitted in the transition yi -> Yf can be determined from the photon-polarization density operator. In the lowest-order of perturbation theory for the electromagnetic interaction V, the matrix elements of the photon-polarization density operator are given by i X\pR\X') = I f, i, i' — 191 — The photon helicity quantum numbers may have the numerical values X, V = ± 1, corresponding the right and left circular polarization along the direction of observation. The sums over f, i, and i' include the quantum numbers specifying degenerate or nearly degenerate sublevels of the field-dependent final and initial states in the radiative transition Yi -* Yf- These restricted sums are indicated by the prime above the summation symbol in Eq. (1). pA is the density operator representing the field-dependent atomic states. In order to determine the precise spectral distribution of the possibly overlapping Stark and Zeeman components, it is necessary to employ our more detailed (higher-order) density-matrix formulation, incorporating the individual line shifts and widths (Jacobs, Cooper, and Haan, 1994). Since polarization is intimately related to angular momentum, it is advantageous to employ the angular-momentum representation for the atomic states and the multipole expansion for the quantized radiation field. We will assume that the field-dependent atomic eigenstates can be expanded in a basis set of field-free bound and continuum eigenstates: (2) Here Ji is the total electronic angular momentum, M\ is the component along a suitably chosen atomic quantization axis, and Aj denotes the set of remaining quantum numbers. Hyperfine structure will be ignored in our analysis. In order to relate the photon polarization, which is defined with respect to the direction of observation, to the atomic quantization axis, it is necessary to expand the radiative-transition matrix elements in terms of the matrix elements of the electric and magnetic multipole operators: — 192 — j m - - (3) x (~rm Here Q(i)m is the irreducible spherical-tensor form of the multipole-moment operator, and D^(k) designates the Wigner rotation-matrix element DV^((j),9,O). The multiplying factor A(j) depends on the particular type of multipole radiation. The matrix elements of the multipole-moment operator can be evaluated in the angular-momentum representation, in terms of Wigner 3-j symbols and reduced matrix elements, using the Wigner-Eckart theorem: In order to take into account both the electric and the magnetic multipole contributions associated with a given value of