Charge-Exchange Factor in EBIT Spectral Analysis

POSTER

Abstract

The intensity analysis of the spectra of highly charged ions in electron beam ion traps (EBIT) requires accurate experimental or theoretical ionization, excitation, and recombination cross sections and device parameters, like electron beam density and energy, and trapped ion temperatures. Because of the generally high charge state of the trapped ions, charge exchange recombination with residual gases requires sophisticated analysis to correctly account for. By introducing the charge exchange factor, the constraint of accurate charge exchange cross section and device conditions are replaced by the determination of a single parameter, which is a combination of all these factors. If accurately determined experimentally, the charge exchange factor allows for accurate prediction of relative spectral line intensity ratios, determination of ionization or recombination cross sections, or device parameters. As an example, X-ray spectra of highly charged ions of Fe produced in the EBIT at National Institute of Standards and Technology with the beam energy varying between 9.21 keV and 18.00keV will be presented. Spectra were recorded by an array of transition-edge sensor (TES) x-ray microcalorimeters. The analysis of the measured spectra was performed via detailed collisional-radiative modeling of the non-Maxwellian plasma. [1] P. Szypryt et al., Rev. Sci. Instrum. 90, 123107 (2019). [2] Yu. Ralchenko and Y. Maron, J. Quant. Spectr. Rad. Transf. 71, 609 (2001).

*NASA Award # 80NSSC18K0234 NSF Award # 1806494 NIST Award # 70NANB19H024

Authors

  • Yang Yang

    • Clemson University
  • Endre Takacs

    • Clemson University
  • Adam Hosier

    • Clemson University
  • Dipti FNU

    • National Institute of Standards and Technology
  • Yuri Ralchenko

    • National Institute of Standards and Technology
  • Paul Szypryt

    • National Institute of Standards and Technology
  • Galen O'Neil

    • National Institute of Standards and Technology
  • Joseph N. Tan

    • National Institute of Standards and Technology
  • Aung S. Naing

    • National Institute of Standards and Technology
  • Amy Gall

    • Harvard-Smithsonian Center for Astrophysics, Cambridge
  • Adam Foster

    • Harvard-Smithsonian Center for Astrophysics, Cambridge
  • Nancy Brickhouse

    • Harvard-Smithsonian Center for Astrophysics, Cambridge
  • Randall Smith

    • Harvard-Smithsonian Center for Astrophysics, Cambridge
  • David Schultz

    • Northern Arizona University, Flagstaff, AZ