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Interaction of charged impurities and Rydberg excitons in cuprous oxide

Sjard Ole Krüger, Heinrich Stolz, and Stefan Scheel
Phys. Rev. B 101, 235204 – Published 16 June 2020

Abstract

We investigate the influence of a static, uncorrelated distribution of charged impurities on the spectrum of bound excitons in the copper oxide Cu2O. We show that the statistical distribution of Stark shifts and ionization rates leads to the vanishing of Rydberg resonances into an apparent continuum. The appearance of additional absorption lines due to the broken rotational symmetry, together with spatially inhomogeneous Stark shifts, leads to a modification of the observed line shapes that agrees qualitatively with the changes observed in the experiment.

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  • Received 19 March 2020
  • Revised 11 May 2020
  • Accepted 3 June 2020

DOI:https://doi.org/10.1103/PhysRevB.101.235204

©2020 American Physical Society

Physics Subject Headings (PhySH)

Condensed Matter, Materials & Applied Physics

Authors & Affiliations

Sjard Ole Krüger*, Heinrich Stolz, and Stefan Scheel

  • Institut für Physik, Universität Rostock, Albert-Einstein-Straße 23-24, D-18059 Rostock, Germany

  • *sjard.krueger@uni-rostock.de

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Issue

Vol. 101, Iss. 23 — 15 June 2020

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Images

  • Figure 1
    Figure 1

    Comparison of the linewidths derived from spectrum S1 with the theoretically expected scaling (see Sec. 3 for details about the experimental spectra). The deviation can be explained by an additional broadening of 5.55 μeV for all lines.

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  • Figure 2
    Figure 2

    Comparison of experimental spectra (dashed red lines) and numerical spectra (solid blue lines). (a) Comparison of spectrum S1 to the numerical spectrum for ρci=1.2×109cm3. (b) S2 vs numerical spectrum for ρci=1011cm3. The vertical lines represent the (numerical) positions of the unperturbed P excitons.

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  • Figure 3
    Figure 3

    The line parameters of Eq. (9) derived by fits to the numerical and experimental spectra for different impurity densities: (a) the oscillator strength, (b) the FWHM linewidths, and (c) the asymmetry parameter. The error bars denote one standard deviation.

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  • Figure 4
    Figure 4

    The band-gap shift ΔEg(ρci) (red diamonds) with a power-law fit (dashed line) and the maximum observable principal quantum number nmax(ρci) (blue triangles).

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