<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article  PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd"><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article"><front><journal-meta><journal-id journal-id-type="publisher-id">EPE</journal-id><journal-title-group><journal-title>Energy and Power Engineering</journal-title></journal-title-group><issn pub-type="epub">1949-243X</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/epe.2023.1511021</article-id><article-id pub-id-type="publisher-id">EPE-129095</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Engineering</subject></subj-group></article-categories><title-group><article-title>
 
 
  XPS Study of Electroless Deposited Sb&lt;sub&gt;2&lt;/sub&gt;Se&lt;sub&gt;3&lt;/sub&gt; Thin Films for Solar Cell Absorber Material
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Towhid</surname><given-names>Adnan Chowdhury</given-names></name><xref ref-type="aff" rid="aff1"><sub>1</sub></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib></contrib-group><aff id="aff1"><label>1</label><addr-line>Department of Electrical &amp;amp; Electronic Engineering, Ahsanullah University of Science &amp;amp; Technology, Dhaka, Bangladesh</addr-line></aff><pub-date pub-type="epub"><day>03</day><month>11</month><year>2023</year></pub-date><volume>15</volume><issue>11</issue><fpage>363</fpage><lpage>371</lpage><history><date date-type="received"><day>17,</day>	<month>October</month>	<year>2023</year></date><date date-type="rev-recd"><day>14,</day>	<month>November</month>	<year>2023</year>	</date><date date-type="accepted"><day>17,</day>	<month>November</month>	<year>2023</year></date></history><permissions><copyright-statement>&#169; Copyright  2014 by authors and Scientific Research Publishing Inc. </copyright-statement><copyright-year>2014</copyright-year><license><license-p>This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/</license-p></license></permissions><abstract><p>
 
 
  As a thin film solar cell absorber material, antimony selenide (Sb
  <sub>2</sub>Se
  <sub>3</sub>) has become a potential candidate recently because of its unique optical and electrical properties and easy fabrication method. X-ray photoelectron spectroscopy (XPS) was used to determine the stoichiometry and composition of electroless Sb
  <sub>2</sub>Se
  <sub>3</sub> thin films using depth profile studies. The surface layers were analyzed nearly stoichiometric. But the abundant amount of antimony makes the inner layer electrically more conductive.
 
</p></abstract><kwd-group><kwd>Sb&lt;sub&gt;2&lt;/sub&gt;Se&lt;sub&gt;3&lt;/sub&gt;</kwd><kwd> Electroless</kwd><kwd> Depth Profiling</kwd><kwd> Thin Film</kwd><kwd> X-Ray Photoelectron Spectroscopy</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Innovative photovoltaic (PV) technologies with excellent power conversion efficiency (PCE) and inexpensive mass production costs are required to expand solar energy utilization [<xref ref-type="bibr" rid="scirp.129095-ref1">1</xref>] . Huge research interest is developed in thin-film photovoltaic (TFPV) technologies due to the advantages of scalable flexibility, lesser material usage and greater power generation [<xref ref-type="bibr" rid="scirp.129095-ref2">2</xref>] [<xref ref-type="bibr" rid="scirp.129095-ref3">3</xref>] [<xref ref-type="bibr" rid="scirp.129095-ref4">4</xref>] . Important successes have been achieved in the representative cadmium telluride (CdTe) [<xref ref-type="bibr" rid="scirp.129095-ref5">5</xref>] , copper indium gallium selenide (CIGS) [<xref ref-type="bibr" rid="scirp.129095-ref5">5</xref>] [<xref ref-type="bibr" rid="scirp.129095-ref6">6</xref>] , cadmium telluride (CdTe) [<xref ref-type="bibr" rid="scirp.129095-ref7">7</xref>] and perovskites [<xref ref-type="bibr" rid="scirp.129095-ref8">8</xref>] [<xref ref-type="bibr" rid="scirp.129095-ref9">9</xref>] among various types of thin-film solar cells. However, the main disadvantages of these solar cells are the toxicity of cadmium (Cd), the scarcity of tellurium(Te) and indium (In) and the problem of achieving a stoichiometric ratio. As a result, different novel earth-abundant materials, such as CuSbSe<sub>2</sub> [<xref ref-type="bibr" rid="scirp.129095-ref10">10</xref>] , Cu<sub>2</sub>SnS<sub>3</sub> [<xref ref-type="bibr" rid="scirp.129095-ref11">11</xref>] , Cu<sub>2</sub>ZnSnSe<sub>4</sub> [<xref ref-type="bibr" rid="scirp.129095-ref12">12</xref>] , SnSe [<xref ref-type="bibr" rid="scirp.129095-ref13">13</xref>] , CuSbS<sub>2</sub> [<xref ref-type="bibr" rid="scirp.129095-ref14">14</xref>] , Sb<sub>2</sub>S<sub>3</sub> [<xref ref-type="bibr" rid="scirp.129095-ref15">15</xref>] and Sb<sub>2</sub>Se<sub>3</sub> [<xref ref-type="bibr" rid="scirp.129095-ref16">16</xref>] have been suggested as a substitute for the low cost and eco-friendly of thin film solar cells.</p><p>Among those, antimony selenide (Sb<sub>2</sub>Se<sub>3</sub>) has emerged as a promising candidate for next-generation solar absorber material. It is a compound semiconductor belonging to the group V-VI with a suitable band gap of 1.1 - 1.2 eV and finds widespread applications in optoelectronic, thermoelectric photoconducting targets, infrared spectroscopy and television camera [<xref ref-type="bibr" rid="scirp.129095-ref17">17</xref>] [<xref ref-type="bibr" rid="scirp.129095-ref18">18</xref>] . It was used in the 1950s [<xref ref-type="bibr" rid="scirp.129095-ref19">19</xref>] in mineral anti-monselite [<xref ref-type="bibr" rid="scirp.129095-ref20">20</xref>] . It exhibits good photovoltaic and thermoelectric properties which allow possible usage for thermophotovoltaic, thermoelectric [<xref ref-type="bibr" rid="scirp.129095-ref21">21</xref>] [<xref ref-type="bibr" rid="scirp.129095-ref22">22</xref>] [<xref ref-type="bibr" rid="scirp.129095-ref23">23</xref>] [<xref ref-type="bibr" rid="scirp.129095-ref24">24</xref>] and solar cells [<xref ref-type="bibr" rid="scirp.129095-ref25">25</xref>] . Sb<sub>2</sub>Se<sub>3</sub> also finds usage in batteries, photodetectors, and memory gadgets [<xref ref-type="bibr" rid="scirp.129095-ref26">26</xref>] . Tremendous research has been focused on Sb<sub>2</sub>Se<sub>3</sub> for hybrid solar cell fabrication as light absorber materials [<xref ref-type="bibr" rid="scirp.129095-ref21">21</xref>] [<xref ref-type="bibr" rid="scirp.129095-ref27">27</xref>] due to its low cost, narrow band gap, non-toxic and comparatively earth-abundant [<xref ref-type="bibr" rid="scirp.129095-ref28">28</xref>] . In the present work, electroless deposition of Sb<sub>2</sub>Se<sub>3</sub> thin films was done and examination of stoichiometry of Sb<sub>2</sub>Se<sub>3</sub> thin films using X-ray photoelectron spectroscopy (XPS) depth profiling was carried out.</p></sec><sec id="s2"><title>2. Experimental Details</title><p>All the glassware in our experiment has been cleaned by first washing and scrubbing with Alconox, followed by a 20 min. sonication in acetone, and methanol, and then washed with isopropanol and DI water. Afterward, the glassware was dried using N<sub>2</sub> gas. An aqueous solution of 0.227 g Sb<sub>2</sub>Se<sub>3</sub>, 0.259 g Na<sub>2</sub>SeO<sub>3</sub>, 3 ml hydrazine hydrate and 50 ml water have been used for precursor solution electroless deposition. The substrate temperature was controlled by a hot plate with which a thermocouple was attached. The substrate temperature was maintained within &#177;1˚C of 40˚C for 50 min.</p><p>The composition of the Sb<sub>2</sub>Se<sub>3</sub> thin film was studied using XPS. The XPS spectra were obtained by using monochromatic Al Kα radiation (1486.6 eV). through a Kratos AXIS Ultra DLD XPS system at a base pressure of 5 &#215; 10<sup>−10</sup> Torr, equipped with an electronic neutralization gun to eliminate the charge effect on the sample surface. The sample was firstly pressed to a 1 &#215; 13 mm disc and fixed to the sample holder, and then it was degassed in the load lock chamber overnight. After that, it was removed to the test chamber for XPS study. All binding energy values were calibrated by using the value of contaminant carbon (C 1s 284.6 eV) as a reference. The sample was then ion sputtered with Ar<sup>+</sup> at 4000 eV and 15 mA for 1 min and 10 min.</p><p>XPSPeak software version 4.1 was used to obtain all the spectra. The spectra were deconvoluted using a mixture of Lorentzian-Gaussian type peaks.</p></sec><sec id="s3"><title>3. Results and Discussion</title><p>The chemical purity and the composition of Sb<sub>2</sub>Se<sub>3</sub> thin films were investigated by XPS analysis. The typical XPS survey spectrum Sb<sub>2</sub>Se<sub>3</sub> is shown in <xref ref-type="fig" rid="fig1">Figure 1</xref>(a). The peaks arising from Sb 3p, 3d, Sb Auger, Na 1s, Na Auger, C 1s, Se 3p and 3d are clearly seen in the spectrum. Carbon contamination is present in almost all the preparations. All other peaks that arise due to energy loss features on the major peaks are weak and broad. The Se 3d intensity is very large compared to the Se 3p intensity, and that is why we have reported just the Se 3d spectra of Se compounds. High-resolution spectra of the Sb 3d core level and Se 3d core level are shown in <xref ref-type="fig" rid="fig1">Figure 1</xref>(b) and <xref ref-type="fig" rid="fig1">Figure 1</xref>(c) respectively. The two peaks at 530.1 eV and 539.4 eV can be assigned to the binding energy of Sb 3d<sub>5/2</sub> and 3d<sub>3/2</sub> respectively. The separation of Sb 3d doublet is by 9.3 eV. These binding energy values of Sb 3d are characteristic of antimony tri-selenide [<xref ref-type="bibr" rid="scirp.129095-ref18">18</xref>] . No oxygen peak was observed in this hydrazine-processed Sb<sub>2</sub>Se<sub>3</sub> thin film in the high-resolution spectra of the Sb 3d core level. The binding energy value of 54.96 eV of Se 3d is characteristic of antimony tri-selenide [<xref ref-type="bibr" rid="scirp.129095-ref18">18</xref>] .</p><p>The XPS survey spectrum of Sb<sub>2</sub>Se<sub>3</sub> thin film after 1 min. Ar<sup>+</sup> ion sputtering is shown in <xref ref-type="fig" rid="fig2">Figure 2</xref>(a). The peaks arising from Sb 3p, 3d, Sb Auger, Na 1s, Na Auger, C 1s, Se 3p and 3d are clearly seen in the spectrum. Carbon contaminations on the surface were reduced significantly after 1 min. Ar<sup>+</sup> ion sputtering. High resolution spectra of Sb 3d core level and Se 3d core level are shown in the</p><p><xref ref-type="fig" rid="fig2">Figure 2</xref>(b) and <xref ref-type="fig" rid="fig2">Figure 2</xref>(c) respectively. The two peaks at 530.1 eV and 539.4 eV can be assigned to the binding energy of Sb 3d<sub>5/2</sub> and 3d<sub>3/2</sub> respectively. The separation of Sb 3d double is by 9.3 eV. These binding energy values of Sb 3d are characteristic of antimony tri-selenide [<xref ref-type="bibr" rid="scirp.129095-ref18">18</xref>] . No oxygen peak was observed in this hydrazine-processed Sb<sub>2</sub>Se<sub>3</sub> thin film in the high-resolution spectra of the Sb 3d core level. The binding energy value of 54.96 eV of Se 3d is characteristic of antimony tri-selenide [<xref ref-type="bibr" rid="scirp.129095-ref18">18</xref>] . No chemical shift was observed in Sb 3d and Se 3d core levels after 1 min. of Ar<sup>+</sup> ion sputtering.</p><p>The XPS survey spectrum of Sb<sub>2</sub>Se<sub>3</sub> thin film after 10 min. Ar<sup>+</sup> ion sputtering is shown in <xref ref-type="fig" rid="fig3">Figure 3</xref>(a). The peaks arising from Sb 3p, 3d, Sb Auger, Na 1s, C 1s, Se 3p and 3d are clearly seen in the spectrum. Carbon contaminations and the peak corresponding to Na 1s core level were reduced to a low level after 10 min. Ar<sup>+</sup> ion sputtering. High-resolution spectra of the Sb 3d core level and Se 3d core level are shown in <xref ref-type="fig" rid="fig3">Figure 3</xref>(b) and <xref ref-type="fig" rid="fig3">Figure 3</xref>(c) respectively. The two peaks at 530.2 eV and 539.5 eV can be assigned to the binding energy of Sb 3d<sub>5/2</sub> and 3d<sub>3/2</sub> respectively. The separation of Sb 3d double is by 9.3 eV. These binding energy values of Sb 3d are characteristic of antimony tri-selenide [<xref ref-type="bibr" rid="scirp.129095-ref18">18</xref>] . No oxygen peak was observed in this hydrazine-processed Sb<sub>2</sub>Se<sub>3</sub> thin film in the high-resolution spectra of the Sb 3d core level. The binding energy value of 54.96 eV of the Se 3d is characteristic of antimony tri-selenide [<xref ref-type="bibr" rid="scirp.129095-ref18">18</xref>] . The binding energy value of the Sb 3d core level is increased by 0.1 eV and no chemical shift was observed in the Se 3d core level after 10 min. of Ar<sup>+</sup> ion sputtering.</p></sec><sec id="s4"><title>4. Conclusion</title><p>The device performance deteriorates due to the presence of recombination centers created by oxygen impurity [<xref ref-type="bibr" rid="scirp.129095-ref18">18</xref>] . Oxygen can be present in Sb<sub>2</sub>Se<sub>3</sub> thin films as it is air-sensitive. So X-ray photoelectron spectroscopy (XPS) was used to investigate the composition of Sb<sub>2</sub>Se<sub>3</sub> thin film. Almost stoichiometric composition of Sb<sub>2</sub>Se<sub>3</sub> thin films close to the surface is observed using the XPS depth profile result in this work. The peak intensity of C(1s) becomes smaller at the deeper surface as sputter time is increased. No oxygen peak was observed in this hydrazine-processed Sb<sub>2</sub>Se<sub>3</sub> thin film in the high-resolution spectra of the Sb 3d core level which is good for device performance. The peak corresponding to Na 1s core level decreased significantly with Ar<sup>+</sup> ion sputtering time. The Sb 3d core level binding energy is increased by 0.1 eV after 10 min Ar<sup>+</sup> ion sputtering. No chemical shift was observed in the Se 3d core level during Ar<sup>+</sup> ion sputtering.</p></sec><sec id="s5"><title>Acknowledgements</title><p>The work was supported by the Advanced Support Program for Innovative Research Excellence-(ASPIRE-I), grant number 15530-E404 and Support to Promote Advancement of Research and Creativity (SPARC), grant number 15530-E413 of the University of South Carolina, Columbia, USA.</p></sec><sec id="s6"><title>Conflicts of Interest</title><p>The author declares no conflicts of interest regarding the publication of this paper.</p></sec><sec id="s7"><title>Cite this paper</title><p>Chowdhury, T.A. (2023) XPS Study of Electroless Deposited Sb<sub>2</sub>Se<sub>3</sub> Thin Films for Solar Cell Absorber Material. 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