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Effect of spin-orbit interaction on the optical spectra of single-layer, double-layer, and bulk MoS2
A. Molina-Sanchez, D. Sangalli, K. Hummer, A. Marini, L. Wirtz

Effect of spin-orbit interaction on the optical spectra of single-layer, double-layer, and bulk MoS2

Science & Mathematics Published 2013 Verification Pending

Overview & Synopsis

We present converged ab initio calculations of the optical absorption spectra of single-layer, double-layer, and bulk MoS2. Both the quasiparticle-energy calculations (on the level of the GW approximation ) and the calculation of the absorption spectra (on the level of the Bethe-Salpeter equation) explicitly include spin-orbit coupling, using the full spinorial Kohn-Sham wave functions as input. Without excitonic effects, the absorption spectra would have the form of a step function, corresponding to the joint density of states of a parabolic band dispersion in two dimensions. This profile is deformed by a pronounced bound excitonic peak below the continuum onset. The peak is split by spin-orbit interaction in the case of single-layer and (mostly) by interlayer interaction in the case of double-layer and bulk MoS2. The resulting absorption spectra are thus very similar in the three cases, but the interpretation of the spectra is different. Differences in the spectra can be seen in the shape of the absorption spectra at 3 eV where the spectra of the single and double layers are dominated by a strongly bound exciton.

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Document Information

Document Title Effect of spin-orbit interaction on the optical spectra of single-layer, double-layer, and bulk MoS2
Author / Organization A. Molina-Sanchez, D. Sangalli, K. Hummer, A. Marini, L. Wirtz
Subject & Discipline Multidisciplinary Academic Open Research
Categories Science & Mathematics
Publication Year 2013
License / Rights Open Access / Creative Commons
Resource Verification Listed PDF (Verification Pending)
Original Host Website HAL Open Science (hal.science)
File Format application/pdf (Portable Document Format)
Language EN
Catalog ID DOC-43129
Original Source Link Visit Source Page on hal.science »