Spatially isolated neutral excitons via clusters on trilayer MoS 2
Source abstract
Abstract
In spite of having a large exciton binding energy, two-dimensional (2D) transition metal dichalcogenides (TMDs) are limited as light-emitting materials because the spectral weight of neutral excitons decreases exponentially with increasing the excitation density. That is, neutral excitons easily transfer to trions, and exciton-exciton annihilation (EEA) occurs due to the strengthening of exciton kinetic energy in the layered structure. In here, we come up with an isolated neutral exciton system, maintaining its high spectral weight when the carrier density increased, which is achieved via MoS2 clusters on a MoS2 trilayer directly synthesized by metal-organic chemical vapor deposition (MOCVD). While increasing the excitation density, trions are decomposed by spatial confinement at the saturation level of its full width at half maximum (FWHM), and simultaneously the spectral weight of neutral excitons restarts to increase. Furthermore, we reveal the causality relationship between trions and B excitons, providing a keen insight into organic interactions among radiative recombination processes in 2D TMDs.
Source: europepmc · Quality: candidate unverified · Source record ↗
Research context
OpenAlex topics: 2D Materials and Applications · Perovskite Materials and Applications · Quantum Dots Synthesis And Properties
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
School of Electrical Engineering, Graphene/2D Materials Research Center, Center for Advanced Materials Discovery towards 3D Display, KAIST, Daehakro, Yuseong-gu, Daejeon, 34141, Republic of Korea
Department of Physics, Korea Advanced Institute of Science and Technology (KAIST), Daejeon 34141, Republic of Korea
Funding
National Research Foundation of Korea · Samsung
References (29)
Show source-provided references
1. Chernikov · Phys. Rev. Lett. · 2014 · 113 · 07680210.1103/PhysRevLett.113.076802 ↗
2. Komsa · Phys. Rev. B: Condens. Matter Mater. Phys. · 2012 · 86 · 233
3. Wang · Rev. Mod. Phys. · 2018 · 90 · 02100110.1103/RevModPhys.90.021001 ↗
4. Amani · Science · 2015 · 350 · 106510.1126/science.aad2114 ↗
5. Li · J. Mater. Chem. C · 2019 · 7 · 430410.1039/C8TC06343E ↗
6. Mueller · npj 2D Mater. Appl. · 2018 · 2 · 2910.1038/s41699-018-0074-2 ↗
7. Yuan · Nanoscale · 2015 · 7 · 740210.1039/C5NR00383K ↗
8. Chi · ACS Nano · 2018 · 12 · 896110.1021/acsnano.8b02354 ↗
9. Ayari · Nanoscale · 2020 · 12 · 1444810.1039/D0NR03170D ↗
10. Lee · Phys. Rev. B: Condens. Matter Mater. Phys. · 2016 · 93 · 14040910.1103/PhysRevB.93.140409 ↗
11. Astakhov · Phys. Rev. B: Condens. Matter Mater. Phys. · 2000 · 62 · 1034510.1103/PhysRevB.62.10345 ↗
12. He · 2D Mater. · 2019 · 6 · 02503010.1088/2053-1583/ab0760 ↗
13. Li · Sci. Rep. · 2016 · 21171 · 1
14. Spirko · Surf. Sci. · 2003 · 542 · 19210.1016/S0039-6028(03)00957-9 ↗
15. Schmidt · Phys. Rev. B: Condens. Matter · 1992 · 45 · 898910.1103/PhysRevB.45.8989 ↗
16. Boyer · Science · 2002 · 297 · 116010.1126/science.1073765 ↗
17. Wong · Opt. Eng. · 2011 · 50 · 07320110.1117/1.3600422 ↗
18. Shinde · APL Mater. · 2019 · 7 · 08111310.1063/1.5095451 ↗
19. Luckert · J. Appl. Phys. · 2012 · 111 · 09350710.1063/1.4709448 ↗
20. Lee · ACS Photonics · 2018 · 5 · 290410.1021/acsphotonics.8b00249 ↗
21. Hong · Nat. Commun. · 2015 · 6 · 629310.1038/ncomms7293 ↗
22. Zhou · Nano Lett. · 2013 · 13 · 261510.1021/nl4007479 ↗
23. Chernikov · Phys. Rev. Lett. · 2015 · 115 · 12680210.1103/PhysRevLett.115.126802 ↗
24. Christopher · Sci. Rep. · 2017 · 7 · 1406210.1038/s41598-017-14378-w ↗
25. Salehzadeh · Nano Lett. · 2014 · 14 · 412510.1021/nl5017283 ↗
26. Mak · Nat. Mater. · 2013 · 12 · 20710.1038/nmat3505 ↗
27. Zhang · Phys. Rev. B: Condens. Matter · 2014 · 89 · 20543610.1103/PhysRevB.89.205436 ↗
28. Jia · J. Mater. Chem. C · 2016 · 4 · 882210.1039/C6TC02502A ↗
29. Tran · Curr. Appl. Phys. · 2016 · 16.9 · 115910.1016/j.cap.2016.03.023 ↗