MRS Meetings and Events

 

NM07.11.04 2022 MRS Fall Meeting

Growth of Thin-Film WS2 for Solar Cell and Photodetector Applications

When and Where

Dec 7, 2022
2:15pm - 2:20pm

NM07-virtual

Presenter

Co-Author(s)

Mohd Samim Reza1,Tejveer Anand1,Henam Devi1,Madhusudan Singh1

Indian Institute of Technology Delhi1

Abstract

Mohd Samim Reza1,Tejveer Anand1,Henam Devi1,Madhusudan Singh1

Indian Institute of Technology Delhi1
Tungsten disulfide, a transition metal dichalcogenide (TMDs) semiconductor, has a bulk phase bandgap of 1.35 eV, very close to the Shockley-Queisser limit for two-level systems at AM1.5G solar spectrum, making it a compelling material for solar photovoltaic applications[1]. Its applications in photovoltaics are still in their inception due to the difficulty of obtaining a uniform, pin-hole-free WS2 thin film with good adhesion [2,3]. This work reports on a two-step process involving sulfurization to grow a WS<sub>2</sub> thin film on a SiO<sub>2</sub> substrate (University Wafers) using a custom-built 12-zone horizontal split furnace (Quazar Technologies) for possible solar cell and photodetector applications. A thin film (~10 nm) of tungsten was deposited on a SiO<sub>2</sub> substrate at a rate of ~0.6A using DC sputtering system (Angstrom Engineering). This thin film was subsequently heated to 800-1100°C under 0-300 sccm of Ar flow in the furnace in presence of elemental sulfur for sulfurization. X-ray diffraction (Rigaku Ultima IV, Copper Kα = 1.54Å) scans of the film revealed a sharp and intense peak at 14.12° (2H-WS<sub>2</sub> nanosheet: JCPDS 08-0237), corresponding to (002) growth with a = 3.154 Å and c = 12.362 Å. The other peaks at 28.12° and 43.20° are inferred to correspond to (004) and (006) crystal planes. Further, Raman spectra (Renishaw inVia confocal microscope-based Raman spectrometer) of the sample reveal in-plane (E<sup>1</sup><sub>2g</sub>) and out-of-plane (A<sub>1g</sub>) vibrational modes at wavenumbers 348.25/cm and 412.90/cm, confirming the WS<sub>2</sub> growth. The wavenumber difference and intensity ratio of E<sup>1</sup><sub>2g</sub> and A<sub>1g</sub> vibrational mode peaks are estimated to be 64.65 and 1.03, respectively, confirming the multilayer growth. Raman mapping over an area of 5.1 x5.1 μm with a step size of 300 nm suggests consistent growth free of directional bias in the sulfurization process. The peak differences range from 64.65/cm to 70.72/cm, with an average of 68.34/cm[4], while the intensity ratio ranges from 0.88 to 1.13, with an average of1.03, again confirming the uniform multilayer growth. Field-emission scanning electron microscope (FESEM, JEOL JSM-7800F Prime) scans indicate formation of nanoflakes. Surface photovoltage spectroscopy (KP Technology KP020+SPS040) was used to measure the work function (-4.613 eV). Atomic force microscopy scans (Asylum Research MFP3D-BIO) were used to estimate the surface roughness of the grown WS2 layer to be 62.33 nm, while the underlying tungsten layer had a surface roughness of 72.99 pm. This suggests that the process of bulk incorporation of sulfur leads to significant increase in surface roughness. As we expected to fabricate heterojunctions of WS<sub>2</sub> with a variety of solution-phase p-type materials in ongoing work, the resulting increase in surface contact area of the heterojunction is expected to provide a larger number of exciton dissociation sites expected to increase the short circuit current, and to reduce optical reflection of the device[5,6].<br/><br/>References :<br/>1. Physica status solidi (a) 214, no. 12 (2017): 1700218<br/>2. Scientific reports 10, no. 1 (2020): 1-11<br/>3. Materials Today Advances 8 (2020): 100098<br/>4. Scientific Reports 3 (2013): 1755<br/>5. Micromachines 10, no. 9 (2019): 619<br/>6. Progress in Photovoltaics: Research and Applications 30, no. 6<br/>(2022): 622-631

Keywords

nanostructure | W

Symposium Organizers

Jeehwan Kim, Massachusetts Institute of Technology
Sanghoon Bae, Washington University in Saint Louis
Deep Jariwala, University of Pennsylvania
Kyusang Lee, University of Virginia

Publishing Alliance

MRS publishes with Springer Nature