Excitonic complexes in -doped WS monolayer
arXiv:2012.11509 · doi:10.1021/acs.nanolett.0c05021
Abstract
We investigate the origin of emission lines apparent in the low-temperature photoluminescence spectra of -doped WS monolayer embedded in hexagonal BN layers using external magnetic fields and first-principles calculations. Apart from the neutral A exciton line, all observed emission lines are related to the negatively charged excitons. Consequently, we identify emissions due to both the bright (singlet and triplet) and dark (spin- and momentum-forbidden) negative trions as well as the phonon replicas of the latter optically-inactive complexes. The semi-dark trions and negative biexcitons are distinguished. Based on their experimentally extracted and theoretically calculated -factors, we identify three distinct families of emissions due to exciton complexes in WS: bright, intravalley and intervalley dark. The -factors of the spin-split subbands in both the conduction and valence bands are also determined.
Manuscript: 7 pages, 5 figures; SI: 5 pages, 3 figures
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