Nonparabolic dispersion of charge carriers in CsPbI$_3$ in the orthorhombic phase
O. S. Sultanov (1, 2) D. K. Loginov (1), I. V. Ignatiev (1, 2), D. V. Pankin (3), M. B. Smirnov (2), and M. S. Kuznetsova (1) ((1) Spin Optics Laboratory, St.Petersburg State University, (2) Faculty of Physics, St. Petersburg State University, (3) Center for Optical

TL;DR
This paper investigates the nonparabolic dispersion of charge carriers in orthorhombic CsPbI$_3$ using DFT calculations, proposing a model to accurately describe their energy-momentum relationship at higher energies.
Contribution
It introduces a quadratic model for charge carrier dispersion in CsPbI$_3$ that captures nonparabolicity beyond the parabolic approximation.
Findings
Dispersion curves show strong nonparabolicity above 0.2 eV for electrons and 0.1 eV for holes.
A model accurately approximates dispersion curves in all symmetric directions.
Effective masses depend quadratically on the wave vector at higher energies.
Abstract
The dispersion curves for the electrons and holes in CsPbI in the orthorhombic phase are calculated using the density functional theory (DFT), with the spin-orbit coupling taken into account. The effective masses of the charge carriers are obtained using the parabolic approximation of the dispersion curves in different directions in the -space. It is found that the dispersion curves demonstrate strong nonparabolicity at energies above 0.2 eV for electrons and above 0.1 eV for holes, available for experimental study by the means of optical spectroscopy. We propose a model that describes the dispersion dependences of charge carriers at those energies, where the effective masses of the quasiparticles depend quadratically on the wave vector. An expression is obtained according to the model, which can accurately approximate the dispersion curves for the electron and the hole in all…
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