6533b823fe1ef96bd127ec89

RESEARCH PRODUCT

Exciton-Phonon Coupling in the Ultraviolet Absorption and Emission Spectra of Bulk Hexagonal Boron Nitride

Henrique Pereira Coutada MirandaHenrique Pereira Coutada MirandaLudger WirtzAlejandro Molina-sanchezFulvio Paleari

subject

Materials sciencePhononExciton: Physics [G04] [Physical chemical mathematical & earth Sciences]Ab initioFOS: Physical sciencesGeneral Physics and Astronomy01 natural sciencesMolecular physicsCondensed Matter::Materials Sciencephonon-assisted luminescenceMesoscale and Nanoscale Physics (cond-mat.mes-hall)0103 physical sciencesEmission spectrum010306 general physicsAbsorption (electromagnetic radiation)Condensed Matter - Materials ScienceCondensed Matter - Mesoscale and Nanoscale PhysicsMaterials Science (cond-mat.mtrl-sci)Condensed Matter::Mesoscopic Systems and Quantum Hall EffectCoupling (probability): Physique [G04] [Physique chimie mathématiques & sciences de la terre]indirect absorptionDirect and indirect band gapsLuminescenceexciton-phonon coupling

description

We present an \textit{ab initio} method to calculate phonon-assisted absorption and emission spectra in the presence of strong excitonic effects. We apply the method to bulk hexagonal BN which has an indirect band gap and is known for its strong luminescence in the UV range. We first analyse the excitons at the wave vector $\overline{q}$ of the indirect gap. The coupling of these excitons with the various phonon modes at $\overline{q}$ is expressed in terms of a product of the mean square displacement of the atoms and the second derivative of the optical response function with respect to atomic displacement along the phonon eigenvectors. The derivatives are calculated numerically with a finite difference scheme in a supercell commensurate with $\overline{q}$. We use detailed balance arguments to obtain the intensity ratio between emission and absorption processes. Our results explain recent luminescence experiments and reveal the exciton-phonon coupling channels responsible for the emission lines.

https://doi.org/10.1103/physrevlett.122.187401