Brightening of dark excitons in ${\mathrm{WS}}_{2}$ via tensile strain-induced excitonic valley convergence (2024)

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Brightening of dark excitons in WS2 via tensile strain-induced excitonic valley convergence

Tamaghna Chowdhury, Sagnik Chatterjee, Dibyasankar Das, Ivan Timokhin, Pablo Díaz Núñez, Gokul M. A., Suman Chatterjee, Kausik Majumdar, Prasenjit Ghosh, Artem Mishchenko, and Atikur Rahman
Phys. Rev. B 110, L081405 – Published 12 August 2024
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Brightening of dark excitons in ${\mathrm{WS}}_{2}$ via tensile strain-induced excitonic valley convergence (1)

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    Brightening of dark excitons in ${\mathrm{WS}}_{2}$ via tensile strain-induced excitonic valley convergence (2)

    Abstract

    Transition-metal dichalcogenides (TMDs) host tightly bound electron-hole pairs—excitons—which can be either optically bright or dark based on spin and momentum selection rules. In tungsten-based TMDs, a momentum-forbidden dark exciton is the energy ground state, and therefore, it strongly affects the emission properties. In this work, we brighten the momentum-forbidden dark exciton by placing monolayer tungsten disulfide on top of nanotextured substrates, which imparts tensile strain, modifying its electronic band structure. This enables phonon-assisted exciton scattering between momentum valleys, thereby brightening momentum-forbidden dark excitons. In addition to offering a tuning knob for light-matter interactions in two-dimensional materials, our results pave the way for designing ultrasensitive strain-sensing devices based on TMDs.

    • Brightening of dark excitons in ${\mathrm{WS}}_{2}$ via tensile strain-induced excitonic valley convergence (3)
    • Brightening of dark excitons in ${\mathrm{WS}}_{2}$ via tensile strain-induced excitonic valley convergence (4)
    • Brightening of dark excitons in ${\mathrm{WS}}_{2}$ via tensile strain-induced excitonic valley convergence (5)
    • Brightening of dark excitons in ${\mathrm{WS}}_{2}$ via tensile strain-induced excitonic valley convergence (6)
    • Brightening of dark excitons in ${\mathrm{WS}}_{2}$ via tensile strain-induced excitonic valley convergence (7)
    • Received 8 March 2024
    • Revised 20 June 2024
    • Accepted 25 July 2024

    DOI:https://doi.org/10.1103/PhysRevB.110.L081405

    ©2024 American Physical Society

    Physics Subject Headings (PhySH)

    1. Research Areas

    Excitons

    1. Physical Systems

    Monolayer filmsTransition metal dichalcogenides

    1. Techniques

    Density functional calculationsPhotoluminescenceRaman spectroscopy

    Condensed Matter, Materials & Applied Physics

    Authors & Affiliations

    Tamaghna Chowdhury1,2,*, Sagnik Chatterjee2, Dibyasankar Das3, Ivan Timokhin1,4, Pablo Díaz Núñez1,4, Gokul M. A.2, Suman Chatterjee5, Kausik Majumdar5, Prasenjit Ghosh2,6, Artem Mishchenko1,4,†, and Atikur Rahman2,‡

    • *Contact author: tamaghna.chowdhury@students.iiserpune.ac.in
    • Contact author: artem.mishchenko@gmail.com
    • Contact author: atikur@iiserpune.ac.in

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    Vol. 110, Iss. 8 — 15 August 2024

    Brightening of dark excitons in ${\mathrm{WS}}_{2}$ via tensile strain-induced excitonic valley convergence (8)
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    Brightening of dark excitons in ${\mathrm{WS}}_{2}$ via tensile strain-induced excitonic valley convergence (9)

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    Brightening of dark excitons in ${\mathrm{WS}}_{2}$ via tensile strain-induced excitonic valley convergence (12)

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    • Brightening of dark excitons in ${\mathrm{WS}}_{2}$ via tensile strain-induced excitonic valley convergence (13)

      Figure 1

      (a)Schematic showing various excitonic species near the electronic dispersions in the K and Λ valleys. Arrows indicate the spin orientations. (b)Field emission scanning electron microscope (FESEM) image of the C-99 nanotextured sample (side view). (c)FESEM image of the C-99 substrate as viewed from the top (scale bar is 20nm). The yellow line shows the interpillar separation l. (d)Schematic of the substrate with ML WS2 placed on top.

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    • Brightening of dark excitons in ${\mathrm{WS}}_{2}$ via tensile strain-induced excitonic valley convergence (14)

      Figure 2

      Temperature-dependent PL spectra of ML WS2 placed on top of (a)C-99 (b)C-48, and (c)C-132 substrates. All the spectra are recorded at an excitation power of 100µW. The spectra are shifted along the y axis for clarity. (d)The integrated intensity I of XD as a function of excitation power P fitted with the relation IPα, where α is the exponent. (e) Temperature dependence of the peak position of X0 (black solid circles) and XD(blue solid squares); the temperature dependence of X0 is fitted with Eq.(1) (red line). (f) FWHM of X0 as a function of temperature fitted with Eq.(2) (red line).

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    • Brightening of dark excitons in ${\mathrm{WS}}_{2}$ via tensile strain-induced excitonic valley convergence (15)

      Figure 3

      (a)Raman spectra of ML WS2 placed on top of a C-99 substrate at 77K. Various peaks are labeled according to Ref.[35]. The main vibrational modes E and A1 are shown in the schematic. The blue and yellow balls represent tungsten and sulfur atoms, respectively. Anomalous behavior of the E peak (b)position and (c)width as a function of temperature. Simulated ωph and γph are shown in the insets of (b)(blue curve) and (c)(green curve), respectively. γ(T)=γph+γe-ph (red curve) is simulated in the inset of (c).

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    • Brightening of dark excitons in ${\mathrm{WS}}_{2}$ via tensile strain-induced excitonic valley convergence (16)

      Figure 4

      (a)DFT computed electronic band structure of ML WS2 with different strain values. (b)Schematic showing the E phonon mediated scattering of the bright KK excitons to dark KΛ excitons due to tensile strain. The KΛ excitons then decay to a virtual state (dotted violet line marked as VS) inside the light cone (shaded area) by emitting phonons and finally recombine radiatively from the VS by emitting photons. (c)ΔE as a function of strain on ML WS2. (d)Calculated phonon dispersion (left panel) and phonon density of states (DOS; right panel). ν represents the phonon band index. (e) Mean peak position of X in ML WS2 on top of SiO2/Si (flat) and C-99 extracted from the PL map. (f) Mean peak position of X0 in ML WS2 on top of C-48, C-99, and C-132 extracted from the PL map. The normal distribution and the raw data points are also shown.

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    • Brightening of dark excitons in ${\mathrm{WS}}_{2}$ via tensile strain-induced excitonic valley convergence (17)

      Figure 5

      (a)and (b)Calculated gmnν values for two degenerate E phonon modes with ν=6 and 7, respectively, which are responsible for the scattering of electrons from CBM+1 at K to CBM at the Λ valley. (c)Line cut along k=K from (a)and (b)to show gmnν along the phonon momentum q, in the ΓMKΓ direction. The blue dashed line shows the gmnν of q=KΛ at k=K. (d)TRPL measurement on ML WS2 at 60K to determine the lifetime of XD.

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    Brightening of dark excitons in ${\mathrm{WS}}_{2}$ via tensile strain-induced excitonic valley convergence (2024)
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