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<front>
<journal-meta>
<journal-id journal-id-type="publisher-id">Front. Phys.</journal-id>
<journal-title>Frontiers in Physics</journal-title>
<abbrev-journal-title abbrev-type="pubmed">Front. Phys.</abbrev-journal-title>
<issn pub-type="epub">2296-424X</issn>
<publisher>
<publisher-name>Frontiers Media S.A.</publisher-name>
</publisher>
</journal-meta>
<article-meta>
<article-id pub-id-type="publisher-id">1240731</article-id>
<article-id pub-id-type="doi">10.3389/fphy.2023.1240731</article-id>
<article-categories>
<subj-group subj-group-type="heading">
<subject>Physics</subject>
<subj-group>
<subject>Original Research</subject>
</subj-group>
</subj-group>
</article-categories>
<title-group>
<article-title>From a Co-Mo precursor to 1H and 1T Co-promoted MoS<sub>2</sub>: exploring the effects of gas pressure</article-title>
<alt-title alt-title-type="left-running-head">Prabhu and Groot</alt-title>
<alt-title alt-title-type="right-running-head">
<ext-link ext-link-type="uri" xlink:href="https://doi.org/10.3389/fphy.2023.1240731">10.3389/fphy.2023.1240731</ext-link>
</alt-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name>
<surname>Prabhu</surname>
<given-names>M. K.</given-names>
</name>
</contrib>
<contrib contrib-type="author" corresp="yes">
<name>
<surname>Groot</surname>
<given-names>I. M. N.</given-names>
</name>
<xref ref-type="corresp" rid="c001">&#x2a;</xref>
<uri xlink:href="https://loop.frontiersin.org/people/2347409/overview"/>
</contrib>
</contrib-group>
<aff>
<institution>Leiden Institute of Chemistry</institution>, <institution>Leiden University</institution>, <addr-line>Leiden</addr-line>, <country>Netherlands</country>
</aff>
<author-notes>
<fn fn-type="edited-by">
<p>
<bold>Edited by:</bold> <ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/2041289/overview">Marco Sacchi</ext-link>, University of Surrey, United Kingdom</p>
</fn>
<fn fn-type="edited-by">
<p>
<bold>Reviewed by:</bold> <ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/2356861/overview">Yukun Lu</ext-link>, China University of Petroleum, China</p>
<p>
<ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/1261768/overview">Jatis Kumar Dash</ext-link>, SRM University, India</p>
</fn>
<corresp id="c001">&#x2a;Correspondence: I. M. N. Groot, <email>i.m.n.groot@lic.leidenuniv.nl</email>
</corresp>
</author-notes>
<pub-date pub-type="epub">
<day>14</day>
<month>09</month>
<year>2023</year>
</pub-date>
<pub-date pub-type="collection">
<year>2023</year>
</pub-date>
<volume>11</volume>
<elocation-id>1240731</elocation-id>
<history>
<date date-type="received">
<day>15</day>
<month>06</month>
<year>2023</year>
</date>
<date date-type="accepted">
<day>04</day>
<month>09</month>
<year>2023</year>
</date>
</history>
<permissions>
<copyright-statement>Copyright &#xa9; 2023 Prabhu and Groot.</copyright-statement>
<copyright-year>2023</copyright-year>
<copyright-holder>Prabhu and Groot</copyright-holder>
<license xlink:href="http://creativecommons.org/licenses/by/4.0/">
<p>This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY). The use, distribution or reproduction in other forums is permitted, provided the original author(s) and the copyright owner(s) are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. No use, distribution or reproduction is permitted which does not comply with these terms.</p>
</license>
</permissions>
<abstract>
<p>The work presented in this paper makes use of the high-pressure <italic>in situ</italic> imaging capabilities of the ReactorSTM to demonstrate that single layer 1T Co-promoted MoS<sub>2</sub> can be directly synthesized without the use of any intercalating agents by applying highly reducing conditions during the growth. In this work, we have sulfided a CoMo nanoparticle precursor supported on Au(111) using a H<sub>2</sub>:CH<sub>3</sub>SH gas mixture at 1&#xa0;bar and imaged the crystallization process <italic>in situ</italic> using the ReactorSTM. We have observed that at low temperatures (&#x223c;500&#xa0;K), an intermediate disordered CoMoS<sub>x</sub> phase is formed which crystallizes into metallic single-layer 1T Co-promoted MoS<sub>2</sub> slabs at temperatures close to 600&#xa0;K. We also show that semiconducting 1H Co-promoted MoS<sub>2</sub> slabs synthesized under sulfur-rich conditions using a vacuum physical vapor deposition process, do not transform into their metallic 1T counterparts when exposed to the same reducing gas pressures and temperatures, thus, demonstrating the importance of the highly reducing conditions during the crystallization process for inducing the formation of the metastable 1T phase. XPS spectra of the 1T Co-promoted MoS<sub>2</sub> slabs indicate a sulfur deficiency of up to 11% in the top layer S, suggesting the likely role of sulfur vacancies in the formation of the 1T phase.</p>
</abstract>
<kwd-group>
<kwd>1T Co-promoted MoS<sub>2</sub>
</kwd>
<kwd>scanning tunneling microscopy</kwd>
<kwd>atmospheric-pressure studies</kwd>
<kwd>
<italic>in situ</italic>
</kwd>
<kwd>X-ray photoelectron spectroscopy</kwd>
</kwd-group>
<custom-meta-wrap>
<custom-meta>
<meta-name>section-at-acceptance</meta-name>
<meta-value>Chemical Physics and Physical Chemistry</meta-value>
</custom-meta>
</custom-meta-wrap>
</article-meta>
</front>
<body>
<sec sec-type="intro" id="s1">
<title>1 Introduction</title>
<p>Single-layer transition metal dichalcogenides (TMDCs) based on MoS<sub>2</sub> have garnered a lot of attention in both fundamental and applied research over the last several decades. A classic example of such an MoS<sub>2</sub>-based TMDC is Co-promoted MoS<sub>2</sub> which is very important for many globally-relevant applications involving optoelectronics, heterogeneous catalysis, and electrocatalysis. For instance, catalysts based on Co-promoted MoS<sub>2</sub>, a transition metal dichalcogenide formed by sulfiding mixed Co-Mo nanoparticles, are used for reducing global SO<sub>x</sub> emissions via hydroprocessing in petroleum refineries [<xref ref-type="bibr" rid="B1">1</xref>], mixed alcohol synthesis [<xref ref-type="bibr" rid="B2">2</xref>], selective olefin hydrogenation [<xref ref-type="bibr" rid="B3">3</xref>], and selective mercaptan synthesis [<xref ref-type="bibr" rid="B4">4</xref>, <xref ref-type="bibr" rid="B5">5</xref>]. Co-promoted MoS<sub>2</sub> is also widely used as a noble-metal-free electrocatalyst for the hydrogen evolution reaction (HER) [<xref ref-type="bibr" rid="B6">6</xref>] and Li-ion battery electrodes [<xref ref-type="bibr" rid="B7">7</xref>]. Particularly, its 1T metastable counterpart, has been of great relevance to van der Waals heterostructure-based optoelectronic devices due to its room temperature ferromagnetism [<xref ref-type="bibr" rid="B8">8</xref>&#x2013;<xref ref-type="bibr" rid="B11">11</xref>].</p>
<p>In the laboratory, the 1T and 1T&#x2019; analogues of pristine and promoted MoS<sub>2</sub> can be synthesized by various strategies. One of the techniques involves using alkali metals like Li, Na, or K during the MoS<sub>2</sub> synthesis. The alkali metals intercalate in the MoS<sub>2</sub> van der Waals gap and stabilize the 1T and 1T&#x2019; phases, thus lowering the bandgap for the metastable phase formation with Mo in an octahedral coordination environment [<xref ref-type="bibr" rid="B12">12</xref>&#x2013;<xref ref-type="bibr" rid="B17">17</xref>]. This technique has been used to synthesize and explore applications of Na- and K-doped single-layer MoS<sub>2</sub> and Co-promoted MoS<sub>2</sub> for gas-phase and HER catalysis [<xref ref-type="bibr" rid="B5">5</xref>, <xref ref-type="bibr" rid="B18">18</xref>]. Intercalation with electron-donating aromatic amines has also proven to be successful in inducing the phase transformation from 1H to 1T [<xref ref-type="bibr" rid="B19">19</xref>]. An alternative synthesis strategy for the 1T or 1T&#x2019; MoS<sub>2</sub> phase involves using a sulfur-deficient environment during the synthesis by lowering the chemical potential of sulfur [<xref ref-type="bibr" rid="B15">15</xref>, <xref ref-type="bibr" rid="B20">20</xref>]. Additionally, using argon ion bombardment of 2H MoS<sub>2</sub> has been shown to generate local 1T mosaic structures [<xref ref-type="bibr" rid="B21">21</xref>]. The sulfur vacancy may also be generated by doping with a foreign metal atom of a different formal charge, for instance, Ru or substitutionally co-doping Ni and Co, to generate the 1T phase from the 2H phase [<xref ref-type="bibr" rid="B22">22</xref>, <xref ref-type="bibr" rid="B23">23</xref>]. Similarly, oxygen doping has also been used as a technique to generate sulfur vacancies, and thereby, induce the formation of the 1T phase [<xref ref-type="bibr" rid="B24">24</xref>]. Electrochemical incorporation of S vacancies to induce a 2H&#x2013;1T phase transition has also been reported [<xref ref-type="bibr" rid="B25">25</xref>]. Chalcogen vacancies in other Mo TMDCs have also been shown to induce a phase transition to the 1T and 1T&#x2019; counterpart [<xref ref-type="bibr" rid="B26">26</xref>]. These experiments have generated a lot of excitement in the scientific community, because 1T polymorphs of MoS<sub>2</sub> have been shown to have high hydrogen evolution activity due to its metallic nature, unlike the 1H counterpart, and have been explored for applications in energy production and storage devices, in addition to applications in spintronics due to room temperature ferromagnetism [<xref ref-type="bibr" rid="B27">27</xref>&#x2013;<xref ref-type="bibr" rid="B30">30</xref>]. Especially, many metastable 1T and 1T&#x2019; phases of Co-doped MoS<sub>2</sub> have been demonstrated to be very competitive noble metal-free alternatives for green hydrogen production via water splitting, which has generated a lot of interest in the synthesis of 1T and 1T&#x2019; counterparts of Co-promoted MoS<sub>2</sub> [<xref ref-type="bibr" rid="B6">6</xref>, <xref ref-type="bibr" rid="B31">31</xref>, <xref ref-type="bibr" rid="B32">32</xref>].</p>
<p>Based on these experimental findings, we hypothesize that it should be possible to directly synthesize 1T Co-promoted MoS<sub>2</sub> slabs from metallic Co and Mo nanoparticles by maintaining highly reducing environments during the synthesis, e.g., through a combination of hydrogen gas and the sulfiding agent. Use of hydrogen during the crystallization is expected to generate S-vacanies on the edges and the basal plane. According to the recent work of Jin et. al. [<xref ref-type="bibr" rid="B20">20</xref>], formation of edge S defects and edge sulfur saturations of less than 50% can kinetically favor the formation of the 1T phase by layer sliding. Additionally, the ease of hydrogen dissociation on under-coordinated and metallic Mo [<xref ref-type="bibr" rid="B33">33</xref>, <xref ref-type="bibr" rid="B34">34</xref>] during the synthesis may even allow for some stabilization of the Co-promoted MoS<sub>2</sub> slabs through hydride intercalation. Based on the works of Mom et. al. and Gr&#xf8;nborg et. al. [<xref ref-type="bibr" rid="B33">33</xref>, <xref ref-type="bibr" rid="B34">34</xref>], such reducing conditions can be achieved by using background pressures of hydrogen approaching several bars, typically not possible in an ultra-high vacuum (UHV) setup. Furthermore, using a lower temperature for sulfidation may arrest the transition to the 2H phase. For instance, heating K-promoted MoS<sub>2</sub> to 650&#xa0;K and above, under high gas pressures has been observed to induce irreversible transition to the 1H phase [<xref ref-type="bibr" rid="B5">5</xref>]. Burkhanov et. al. have shown that hydrogen intercalation achieved using H plasma under vacuum environments leads to lattice expansion of MoS<sub>2</sub> similar to that from the 1H to 1T phase transition [<xref ref-type="bibr" rid="B35">35</xref>].</p>
<p>In order to test our hypothesis, we have sulfided a precursor containing mixed Co-Mo nanoparticles supported on Au(111) under high-pressure sulfo-reductive conditions and observed <italic>in situ</italic> the crystallization process using the ReactorSTM setup. At temperatures of up to &#x223c;500&#xa0;K, a disordered CoMoS<sub>x</sub> phase is observed to form which then crystallizes into single-layer 1T Co-promoted MoS<sub>2</sub> when the temperature is raised to 600&#xa0;K. Sulfiding an identical CoMo precursor using H<sub>2</sub>S under vacuum results in the formation of 1H Co-promoted MoS<sub>2</sub> slabs which do not transform into the 1T counterpart when exposed to the same sulfo-reductive conditions, suggesting that reducing conditions are necessary during the crystallization step to form the 1T phase. XPS spectra acquired post synthesis show that the 1T Co-promoted MoS<sub>2</sub> slabs are largely sulfur-deficient, suggesting the role of sulfur vacancies in metastable phase formation. Thus, we demonstrate that the 1T Co-promoted MoS<sub>2</sub> can be readily synthesized and stabilized by using a lower sulfidation temperature and sufficiently sulfo-reductive conditions, without the need for any additional intercalating agents. Furthermore, the ability to observe the formation of a metastable 1T Co-MoS<sub>2</sub> phase <italic>in situ</italic> (i.e., <italic>while it happens</italic>) with atomic resolution under 1&#xa0;bar of gas pressure, elevated temperature, and aggressive chemical conditions, is the main novelty of this work, as it has remained an experimental challenge to do so for several decades. Additionally, the experimental observation that elevating the gas pressure to attain sufficiently reducing conditions to favor the formation of 1T Co-MoS<sub>2</sub> without the need of an intercalating agent is a very important finding that provides us a fundamental understanding of the 1T phase formation process and is also an additional novelty. To the best of our knowledge, the experimental work presented in this paper has not been carried out elsewhere in the past.</p>
</sec>
<sec sec-type="materials|methods" id="s2">
<title>2 Materials and Methods</title>
<sec id="s2-1">
<title>2.1 Sample cleaning</title>
<p>All the experiments were carried out in the ReactorSTM setup [<xref ref-type="bibr" rid="B36">36</xref>]. The sample cleaning procedure reported in our previous works has been used [<xref ref-type="bibr" rid="B37">37</xref>]. Briefly, a polished Au(111) crystal was cleaned by a cyclic sputtering and annealing procedure until XPS could no longer detect any impurities (&#x3c;0.001 monolayers (ML)). 1.5&#xa0;keV Ar<sup>&#x2b;</sup> ions were used for the sputtering and annealing at 873&#xa0;K was performed using radiative heating from a thoriated-tungsten filament at the back of the sample.</p>
</sec>
<sec id="s2-2">
<title>2.2 Physical vapor deposition (PVD)</title>
<p>To grow Mo and Co nanoparticles, Mo and Co rods of 99.99% purity purchased from Goodfellow were used. The evaporation of the respective metals was carried out using an EGCO4 e-beam evaporator. During the evaporation, the clean Au(111) sample was held at room temperature until the coverage of the respective metal was measured to be &#x223c;0.2 monolayers (ML). The coverage was measured by analyzing the XPS spectra of Co and Mo with respect to Au(111) surface layers. Identical samples were prepared for the low-pressure and high-pressure sulfidation.</p>
</sec>
<sec id="s2-3">
<title>2.3 Low-pressure sulfidation</title>
<p>The mixed Co-Mo nanoparticles supported on Au(111) were sulfided at 650&#xa0;K in a 2 &#xd7; 10<sup>&#x2212;6</sup>&#xa0;mbar H<sub>2</sub>S atmosphere. The heating from room temperature to 650&#xa0;K was carried out in the same H<sub>2</sub>S background at a rate of 4&#xa0;K/s and held at 650&#xa0;K for 20&#xa0;min. The sample was then cooled in the H<sub>2</sub>S background to 450&#xa0;K over 15&#xa0;min and thereafter, to room temperature in UHV over 150&#xa0;min.</p>
</sec>
<sec id="s2-4">
<title>2.4 High-pressure sulfidation</title>
<p>The high-pressure sulfidation of the mixed Co-Mo precursor was carried out in the ReactorSTM. For this purpose, a sulfo-reductive gas mixture containing 9 H<sub>2</sub>: 1 CH<sub>3</sub>SH at a total pressure of 1&#xa0;bar was chosen as the sulfiding agent. A temperature of 603&#xa0;K was used for sulfidation as this is the highest temperature attainable in the ReactorSTM [<xref ref-type="bibr" rid="B38">38</xref>, <xref ref-type="bibr" rid="B39">39</xref>]. A temperature of 520&#xa0;K was also selected as an intermediate temperature to observe the effect of temperature.</p>
<p>After loading the sample for sulfidation into the reactor, the STM was first pressurized to 0.1&#xa0;bar with the sulfo-reductive mixture and thereafter, the temperature was raised to 520&#xa0;K with a heating rate of 2&#xa0;K/min. A slow heating rate was chosen because rapid heating would cause rupturing of the fluor-elastomer seals used for isolating the ReactorSTM from the rest of the UHV. After this step, the total pressure was raised to 1&#xa0;bar at a rate of 0.1&#xa0;bar/min. The system was allowed to reach thermal steady-state for 90&#xa0;min in order to minimize the thermal drift. The STM tip was brought into tunneling contact thereafter and the scanning was commenced. After scanning for &#x223c;70&#xa0;min, the tip was retracted, the sample temperature was raised to 603&#xa0;K at 3&#xa0;K/min, and the system was allowed to thermally stabilize for 30&#xa0;min before continuing the STM scanning.</p>
</sec>
<sec id="s2-5">
<title>2.5 Scanning tunneling microscopy</title>
<p>STM scanning was performed with the ReactorSTM using both the UHV mode and the high-pressure mode. STM tips were prepared by cutting polycrystalline Pt-Ir 90&#x2013;10 wires purchased from Goodfellow without further processing. Constant-current scans were performed using LPM video-rate scanning electronics described in detail elsewhere [<xref ref-type="bibr" rid="B40">40</xref>, <xref ref-type="bibr" rid="B41">41</xref>]. Home-developed Camera software and WSxM were used for STM image processing [<xref ref-type="bibr" rid="B42">42</xref>, <xref ref-type="bibr" rid="B42">42</xref>]. Line-by-line background subtraction was used for the ease of viewing of the STM images. All UHV scans were carried out at room temperature.</p>
<p>For the high-pressure STM imaging, the sample was loaded into the STM assembly and a Kalrez seal was placed between the sample and the reactor. Thereafter, the bellows of the reactor were actuated to close the reactor and establish the closed volume for introducing the reaction gases. Gas bottles of Ar (N5.0), H<sub>2</sub> (N5.0), and CH<sub>3</sub>SH (N2.8) {dimethylsulfide and dimethyldisulfide are the primary impurities} procured from Westfalen AG were used for all the experiments. The gas purity was confirmed using a mass spectrometer before use. The gas lines were flushed with Ar and baked out at 423&#xa0;K for 12&#xa0;h to remove any residual water and volatiles before commencing all experiments presented in this work.</p>
<p>For the post-sulfidation characterization, depressurizing the ReactorSTM to UHV conditions is necessary. For this purpose, the total pressure in the ReactorSTM was reduced to 0.1&#xa0;bar and the model catalyst was allowed to cool down to 373&#xa0;K under the flow of gases over 15&#xa0;min. Thereafter, the gases were pumped away, the ReactorSTM was brought under UHV conditions, and the sample allowed to cool to room temperature over 60&#xa0;min.</p>
</sec>
<sec id="s2-6">
<title>2.6 X-ray photoelectron spectroscopy</title>
<p>A commercial SPECS Phoibos system equipped with an XRM50 X-ray source set to the Al K-alpha line and coupled to a monochromator was used to excite the sample with a 54.6&#xb0; incidence angle and with the X-rays generated using an acceleration voltage of 10&#xa0;kV, 250&#xa0;W. A HSA3500 hemispherical analyzer with a pass energy of 30&#xa0;eV was used to acquire all the XPS spectra reported in this paper. All spectra were calibrated using the peak position of the Au 4f signal (84.0&#xa0;eV) of the Au(111) substrate. For all the acquired data, 30 integrations were performed to have a sufficiently high signal-to-noise ratio. XPSPEAK41 software was used for the peak deconvolution. Relative sensitivity factors for surfaces were obtained from literature [<xref ref-type="bibr" rid="B43">43</xref>]. Shirley background subtraction was performed for all the spectra and a non-linear least squares fit method was used for convergence. The XPS spectra were fit using mixed Gaussian (65%) &#x2013;Lorentzian (35%) (GL) curves. Asymmetric GL curves were used to fit the spectra of Co 2p<sub>3/2</sub>. For the Mo 3d and S 2p, paired GL peaks with a constrained area ratio of 3:2 and 1:2, respectively, were used to account for the spin-orbit splitting. For Co 2p, the fitting is performed for the Co 2p<sub>3/2</sub> component. All the signature peak positions are based on previously reported literature work and are tabulated in <xref ref-type="table" rid="T1">Table 1</xref> along with the references.</p>
<table-wrap id="T1" position="float">
<label>TABLE 1</label>
<caption>
<p>XPS binding energies for various components used for peak fitting.</p>
</caption>
<table>
<thead valign="top">
<tr>
<th align="center">Components</th>
<th align="center">Binding energy (BE) (eV)</th>
<th align="center">&#x394;BE<xref ref-type="table-fn" rid="Tfn1">
<sup>a</sup>
</xref> (eV)</th>
<th align="center">References</th>
</tr>
</thead>
<tbody valign="top">
<tr>
<td align="left">1H MoS<sub>2</sub> Mo 3d<sub>5/2</sub>
</td>
<td align="center">229.2</td>
<td align="center">3.15</td>
<td align="center">[<xref ref-type="bibr" rid="B5">5</xref>, <xref ref-type="bibr" rid="B27">27</xref>, <xref ref-type="bibr" rid="B44">44</xref>, <xref ref-type="bibr" rid="B45">45</xref>]</td>
</tr>
<tr>
<td align="left">1T MoS<sub>2</sub> Mo 3d<sub>5/2</sub>
</td>
<td align="center">228.3</td>
<td align="center">3.15</td>
<td align="center">[<xref ref-type="bibr" rid="B5">5</xref>, <xref ref-type="bibr" rid="B27">27</xref>, <xref ref-type="bibr" rid="B44">44</xref>, <xref ref-type="bibr" rid="B45">45</xref>]</td>
</tr>
<tr>
<td align="left">S 2p<sub>3/2</sub> (1T MoS<sub>2</sub>)</td>
<td align="center">161.8</td>
<td align="center">1.16</td>
<td align="center">[<xref ref-type="bibr" rid="B5">5</xref>, <xref ref-type="bibr" rid="B27">27</xref>, <xref ref-type="bibr" rid="B44">44</xref>, <xref ref-type="bibr" rid="B45">45</xref>]</td>
</tr>
<tr>
<td align="left">S 2p<sub>3/2</sub> (2D CoS<sub>2</sub>, 1H MoS<sub>2</sub>)</td>
<td align="center">162.7</td>
<td align="center">1.16</td>
<td align="center">[<xref ref-type="bibr" rid="B5">5</xref>, <xref ref-type="bibr" rid="B27">27</xref>, <xref ref-type="bibr" rid="B37">37</xref>, <xref ref-type="bibr" rid="B44">44</xref>&#x2013;<xref ref-type="bibr" rid="B46">46</xref>]</td>
</tr>
<tr>
<td align="left">S 2s</td>
<td align="center">226.9</td>
<td align="left"/>
<td align="center">[<xref ref-type="bibr" rid="B5">5</xref>, <xref ref-type="bibr" rid="B27">27</xref>, <xref ref-type="bibr" rid="B37">37</xref>, <xref ref-type="bibr" rid="B44">44</xref>&#x2013;<xref ref-type="bibr" rid="B46">46</xref>]</td>
</tr>
<tr>
<td align="left">CoS<sub>2</sub> main Co 2p<sub>3/2</sub>
</td>
<td align="center">778.1</td>
<td align="left"/>
<td align="center">[<xref ref-type="bibr" rid="B27">27</xref>, <xref ref-type="bibr" rid="B44">44</xref>, <xref ref-type="bibr" rid="B47">47</xref>]</td>
</tr>
<tr>
<td align="left">CoS<sub>2</sub> satellites Co 2p<sub>3/2</sub>
</td>
<td align="center">781.1, 783.1</td>
<td align="left"/>
<td align="center">[<xref ref-type="bibr" rid="B27">27</xref>, <xref ref-type="bibr" rid="B44">44</xref>, <xref ref-type="bibr" rid="B47">47</xref>]</td>
</tr>
<tr>
<td align="left">Co-MoS<sub>2</sub> main Co 2p<sub>3/2</sub>
</td>
<td align="center">778.6</td>
<td align="left"/>
<td align="center">[<xref ref-type="bibr" rid="B27">27</xref>, <xref ref-type="bibr" rid="B44">44</xref>, <xref ref-type="bibr" rid="B47">47</xref>]</td>
</tr>
<tr>
<td align="left">Co-MoS<sub>2</sub> satellite Co 2p<sub>3/2</sub>
</td>
<td align="center">781.6, 783.6</td>
<td align="left"/>
<td align="center">[<xref ref-type="bibr" rid="B27">27</xref>, <xref ref-type="bibr" rid="B44">44</xref>, <xref ref-type="bibr" rid="B47">47</xref>]</td>
</tr>
</tbody>
</table>
<table-wrap-foot>
<fn id="Tfn1">
<label>
<sup>a</sup>
</label>
<p>&#x394;BE, is the energy difference between the spin-orbit splitting components. For example, &#x394;BE(3d) &#x3d; BE, 3d<sub>5/2</sub>&#x2013;BE, 3d<sub>3/2</sub>.</p>
</fn>
</table-wrap-foot>
</table-wrap>
</sec>
</sec>
<sec sec-type="results|discussion" id="s3">
<title>3 Results and discussion</title>
<p>We first prepare identical precursors containing Co-Mo mixed nanoparticles supported on a clean Au(111) substrate by sequential physical vapor deposition (PVD) of 0.2 monolayers (ML) Mo metal, followed by 0.2&#xa0;ML Co metal at room temperature. The exact synthesis procedure is detailed in the Materials and Methods section and in the <xref ref-type="sec" rid="s10">Supplementary Materials</xref>.</p>
<p>First, as a control experiment, one of the identical Co-Mo precursors was sulfided at 650&#xa0;K under 2 &#xd7; 10<sup>&#x2212;6</sup>&#xa0;mbar of H<sub>2</sub>S and cooled to room temperature according to the recipe detailed in the Materials and Methods section, in order to replicate the vacuum synthesis recipe of single layer 1H Co-promoted MoS<sub>2</sub> slabs on Au(111) [<xref ref-type="bibr" rid="B48">48</xref>]. After this step, the sample was loaded into the ReactorSTM operated in the UHV mode. <xref ref-type="fig" rid="F1">Figure 1</xref> shows a large-scale STM image thus obtained. In <xref ref-type="fig" rid="F1">Figure 1</xref>, we observe the formation of atomically-flat hexagonal slabs which are identified as single-layer 1H Co-promoted MoS<sub>2</sub> slabs. Under the sulfur-rich conditions used in this experiment, pristine MoS<sub>2</sub> slabs are known to display only the Mo-terminated edges due to the thermodynamic stability of the Mo-termination and hence, adopt a triangular shape [<xref ref-type="bibr" rid="B49">49</xref>]. The substitution of Mo atoms by Co along the S-terminated edges leads to the thermodynamic stability of the S-termination as well, thus, driving the formation of hexagon-shaped slabs such as those in <xref ref-type="fig" rid="F1">Figure 1</xref> [<xref ref-type="bibr" rid="B33">33</xref>]. The Co-promoted MoS<sub>2</sub> slabs have a bright outline along their periphery while their basal planes are imaged relatively darker. The darker basal plane is attributed to the semi-conducting nature of 1H Co-promoted MoS<sub>2</sub> while the bright edge features are attributed to the 1D metallic edge states called BRIM sites [<xref ref-type="bibr" rid="B33">33</xref>]. Additionally, we also observe the formation of the single-layer 2D CoS<sub>2</sub> phase as a byproduct, with the characteristic hexagonal moir&#xe9; structure which is 7 &#xd7; 7 Au atoms (1.95&#xa0;nm &#xd7; 1.95&#xa0;nm) wide. The 2D CoS<sub>2</sub> phase is also observed to form between the Co-promoted MoS<sub>2</sub> slabs on the Au(111) steps. These observations are in excellent agreement with our recent work on 2D CoS<sub>2</sub> slabs supported on Au(111) [<xref ref-type="bibr" rid="B46">46</xref>]. Furthermore, the observation of the complete conversion of the Co and Mo nanoparticles into the respective TMDC phases after the sulfidation process is in agreement with the prior experimental works on the sulfidation of Co and Mo nanoparticles under controlled vacuum conditions [<xref ref-type="bibr" rid="B33">33</xref>, <xref ref-type="bibr" rid="B49">49</xref>, <xref ref-type="bibr" rid="B50">50</xref>].</p>
<fig id="F1" position="float">
<label>FIGURE 1</label>
<caption>
<p>STM image of single-layer 1H Co-promoted MoS<sub>2</sub> slabs prepared by sulfidation of the Co-Mo precursor with H<sub>2</sub>S (2 &#xd7; 10<sup>&#x2212;6</sup>&#xa0;mbar). The STM image was acquired in UHV with a sample voltage of &#x2212;1&#xa0;V and tunneling current of 100&#xa0;pA.</p>
</caption>
<graphic xlink:href="fphy-11-1240731-g001.tif"/>
</fig>
<p>In order to test our hypothesis on the formation of 1T Co-promoted MoS<sub>2</sub> slabs under highly reducing conditions, a freshly prepared identical Co-Mo precursor was sulfided using high-pressure sulfo-reductive conditions within the ReactorSTM. For this purpose, a sulfo-reductive gas mixture (9:1 H<sub>2</sub>:CH<sub>3</sub>SH) was used to pressurize the ReactorSTM to 1&#xa0;bar. Thereafter, the temperature was raised from room temperature to 520&#xa0;K at a rate of 2&#xa0;K/min. <xref ref-type="fig" rid="F2">Figure 2A</xref> shows a large-scale STM image obtained <italic>in situ</italic> during the sulfidation under the sulfo-reductive gas mixture. We observed the formation of two phases: islands with a somewhat hexagonal shape and disordered arrangement of bright protrusions and large atomically-flat islands with an ordered hexagonal pattern, both of which are seen in <xref ref-type="fig" rid="F2">Figures 2A, B</xref>.</p>
<fig id="F2" position="float">
<label>FIGURE 2</label>
<caption>
<p>
<bold>(A&#x2013;D)</bold> STM images of the Co-Mo precursor acquired <italic>in situ</italic> during the sulfidation by a sulfo-reductive gas mixture (1&#xa0;bar, 9H<sub>2</sub>: 1CH<sub>3</sub>SH) at 520&#xa0;K. The MoS<sub>x</sub> and 2D CoS<sub>2</sub> phases are identified. The STM images were aquired at &#x2212;0.3&#xa0;V sample voltage and 500&#xa0;pA tunneling current. The &#x201c;t&#x201d; indicated in the label bars at the top of each STM image indicates the time stamp of acquisition from the commencing of the scanning.</p>
</caption>
<graphic xlink:href="fphy-11-1240731-g002.tif"/>
</fig>
<p>The somewhat hexagon-shaped islands are identified as those of poorly crystalline molybdenum sulfide (MoS<sub>x</sub>). Due to the presence of a sufficient number of diffusing cobalt atoms, we expect that any MoS<sub>x</sub> phase formed will likely be doped with Co atoms, and hence, we denote this phase as CoMoS<sub>x</sub>. The CoMoS<sub>x</sub> islands are measured to be 2.8&#xa0;&#xc5; high (see heightline, <xref ref-type="fig" rid="F2">Figure 2B</xref>), matching closely with the measured height of single-layer Co-promoted MoS<sub>2</sub> from previous experimental reports [<xref ref-type="bibr" rid="B33">33</xref>]. The CoMoS<sub>x</sub> islands are likely an intermediate phase towards the formation of crystalline Co-promoted MoS<sub>2</sub>. No further changes are observed in this disordered CoMoS<sub>x</sub> phase up to 67&#xa0;min into the scanning in the sulfo-reductive gas environment at 520&#xa0;K (see <xref ref-type="fig" rid="F2">Figures 2C, D</xref>), suggesting that the temperature is insufficient for any crystallization to occur.</p>
<p>The atomically-flat slabs with a hexagonal moir&#xe9; pattern on their basal plane are identified as 2D CoS<sub>2</sub> islands. These slabs were also observed to form in our control experiment (see <xref ref-type="fig" rid="F1">Figure 1</xref>). The 2D CoS<sub>2</sub> also retains the characteristic hexagonal moir&#xe9; structure indicating that the basal plane of 2D CoS<sub>2</sub> does not undergo significant structural changes under the sulfo-reductive gas mixture used. Additionally, the formation of this moir&#xe9; structure shows that the 2D CoS<sub>2</sub> islands are crystalline in nature and that the sulfidation of Co nanoparticles is already complete during the process of bringing the ReactorSTM to the operating conditions. This rapid spread and reaction of Co is attributed to the cluster diffusion behavior of Co nanoparticles in the presence of S adatoms which leads to rapid growth of 2D CoS<sub>2</sub> [<xref ref-type="bibr" rid="B50">50</xref>].</p>
<p>To speed up the process of CoMoS<sub>x</sub> crystallization, we further increased the temperature to 603&#xa0;K at the rate of 2&#xa0;K/min while maintaining the sulfo-reductive reaction gases and thermally stabilize the STM before commencing the scanning <italic>in situ</italic>. <xref ref-type="fig" rid="F3">Figure 3A</xref> shows a large-scale STM image obtained <italic>in situ</italic> at 603&#xa0;K at t &#x3d; 121&#xa0;min. Ten minutesafter attaining 603K, the edges of the CoMoS<sub>x</sub> islands are observed to appear slightly brighter in the STM images, as can be seen in <xref ref-type="fig" rid="F3">Figure 3B</xref>. Over the next 35&#xa0;min, the CoMoS<sub>x</sub> slabs are observed to crystallize from the step edges towards the interior (see <xref ref-type="fig" rid="F3">Figures 3B&#x2013;F</xref>). The crystallization is evident from the formation of an ordered hexagonal lattice. The new crystalline phase has a hexagonal arrangement of bright protrusions which are 0.33 &#xb1; 0.01&#xa0;nm apart (see <xref ref-type="fig" rid="F3">Figure 3F</xref>; height profile in <xref ref-type="fig" rid="F3">Figure 3G</xref>). This matches closely with the basal plane S-S distance of single-layer MoS<sub>2</sub> and Co-promoted MoS<sub>2</sub> [<xref ref-type="bibr" rid="B49">49</xref>]. Furthermore, the basal plane protrusions are imaged bright with respect to gold, unlike the 1H Co-promoted MoS<sub>2</sub> in <xref ref-type="fig" rid="F1">Figure 1</xref>, suggesting that this phase has a metallic nature. The crystalline Co-promoted MoS<sub>2</sub> formed under sulfo-reductive conditions (see <xref ref-type="fig" rid="F3">Figures 3B&#x2013;D</xref>), however, does not have a bright BRIM along the edges, unlike the 1H Co-promoted MoS<sub>2</sub> slabs in the control experiment (see <xref ref-type="fig" rid="F1">Figure 1</xref>). All characteristics of this new crystalline phase formed in the sulfo-reductive environment agree very well with those reported for a metastable 1T-MoS<sub>2</sub> phase in which Mo is in an octahedral coordination environment [<xref ref-type="bibr" rid="B15">15</xref>, <xref ref-type="bibr" rid="B28">28</xref>]. Therefore, we identify this new phase as that of single-layer 1T Co-promoted MoS<sub>2</sub>. <xref ref-type="fig" rid="F3">Figures 3B&#x2013;D</xref> also show that the crystalline phase is not resolved well along one of the crystallographic directions especially along the slow scan direction (top to down), giving the appearance of lines. We attribute this to tip assymetry arising from interaction with the gases, especially CH<sub>3</sub>SH at the elevated temperature and pressure used. Such effects were also observed by Mom et. al. under similar gas conditions when using similar as-cut Pt-Ir tips [<xref ref-type="bibr" rid="B34">34</xref>].</p>
<fig id="F3" position="float">
<label>FIGURE 3</label>
<caption>
<p>
<bold>(A&#x2013;F)</bold> STM images of the Co-Mo precursor acquired <italic>in situ</italic> during the sulfidation by a sulfo-reductive gas mixture (1&#xa0;bar, 9H<sub>2</sub>: 1CH<sub>3</sub>SH) at 603&#xa0;K. The MoS<sub>x</sub> and 2D CoS<sub>2</sub> phases are identified. The STM images were aquired at &#x2212;0.3&#xa0;V sample voltage and 500&#xa0;pA tunneling current. The &#x201c;t&#x201d; indicated in the label bars at the top of each STM image indicates the time stamp of acquisition from the commencing of the scanning. <bold>(G)</bold> Height profile along the red line marked A in F. E anf F have additional derivative enhancing in order to bring forward the detail for the ease of viewing.</p>
</caption>
<graphic xlink:href="fphy-11-1240731-g003.tif"/>
</fig>
<p>One may expect that employing a high partial pressure of hydrogen during the cyrstallization favors the formation of a large number of sulfur vacancies along the Co-MoS<sub>2</sub> edges and the basal plane. Recent theoretical work [<xref ref-type="bibr" rid="B20">20</xref>] has shown that increasing the number of sulfur vacancies can make translational layer sliding to form the 1T configuration more kinetically favorable in pristine MoS<sub>2</sub> slabs. While it may also be argued that the electron donation from Co also aids in the formation of 1T Co-promoted MoS<sub>2</sub>, merely having the Co alone does not yield the formation of the 1T phase under the vacuum sulfidation-based control experiment. We also consider the possibility that using a different sulfiding agent may also aid in the formation of the 1T phase as we have used H<sub>2</sub>S for our control experiment and CH<sub>3</sub>SH for the high-pressure sulfidation as the sulfiding agents. Research carried out in the past has shown that the effect of sulfiding agents on the chemical potential of sulfur is minor for small thiol-containing molecules like H<sub>2</sub>S and CH<sub>3</sub>SH, as they all readily disssociate on the gold surface and form adsorbed&#x2013;SH while aromatic (such as thiophenes) and doubly substituted thiols (like dimethyl sulfide) lead to a lower chemical potential of sulfur [<xref ref-type="bibr" rid="B33">33</xref>], [<xref ref-type="bibr" rid="B51">51</xref>&#x2013;<xref ref-type="bibr" rid="B53">53</xref>]. Additionally, previous experiments using a variety of H<sub>2</sub>:H<sub>2</sub>S mixtures under vacuum pressures for MoS<sub>2</sub> synthesis did not lead to the formation of the 1T phase [<xref ref-type="bibr" rid="B49">49</xref>]. Therefore, the elevated H<sub>2</sub> gas pressure used in our experiment to form a sufficient number of sulfur vacancies remains as a major factor that assists in the formation of 1T Co-promoted MoS<sub>2</sub>.</p>
<p>We make use of XPS analysis to determine the number of sulfur vacancies and the amount of Co incorporation into the edges of 1T Co-promoted MoS<sub>2.</sub> As the 1T phase is metallic, BRIM sites are not present on the edges, making the identification of the Co-substituted S edges from the STM images alone difficult. XPS, on the other hand, can detect and resolve Co present in 1T MoS<sub>2</sub> and CoS<sub>2</sub> phases, albeit in a statistically averaged manner [<xref ref-type="bibr" rid="B9">9</xref>, <xref ref-type="bibr" rid="B54">54</xref>]. Typically, the Co present on the S edges of 1H and 1T MoS<sub>2</sub> has a signal resembling metallic Co sulfide but shifted by 0.6&#x2013;0.8&#xa0;eV to higher binding energy depending on the metallicity of the support [<xref ref-type="bibr" rid="B9">9</xref>, <xref ref-type="bibr" rid="B54">54</xref>, <xref ref-type="bibr" rid="B55">55</xref>]. Additionally, the structural relaxation upon the transformation of the 1T phase into the 2H phase results in a downshift in binding energy of the Mo 3days and S 2p spectra of the 1T phase by &#x223c;0.9&#xa0;eV with respect to the 1H phase, thus allowing for the identification of the 1T phase [<xref ref-type="bibr" rid="B56">56</xref>, <xref ref-type="bibr" rid="B57">57</xref>]. Before measuring the XPS spectra, the sample exposed to high pressure was cooled to room temperature in the sulfo-reductive gas environment and then pumped down to UHV. Thereafter, XPS spectra of Mo 3d, S 2p and Co 2p were acquired and analyzed. The Mo 3d spectrum (see <xref ref-type="fig" rid="F4">Figure 4A</xref>) shows the main Mo 3d<sub>5/2</sub> peak at 282.3&#xa0;eV which matches well with the reported XPS spectra of 1T-MoS<sub>2</sub> and 1T-Co-promoted MoS<sub>2</sub> [<xref ref-type="bibr" rid="B54">54</xref>, <xref ref-type="bibr" rid="B57">57</xref>]. The component at 290.2&#xa0;eV is attributed to the unconverted MoS<sub>x</sub> phase as we did not observe any 1H Co-promoted MoS<sub>2</sub> in the STM images. The Co 2p<sub>3/2</sub> spectrum (see <xref ref-type="fig" rid="F4">Figure 4B</xref>) shows the presence of 2 types of cobalt species, namely, the Co in metallic 2D CoS<sub>2</sub> at 778.1&#xa0;eV (55%) and the Co present on the edges of MoS<sub>2</sub> at 778.7&#xa0;eV (45%). The corresponding S 2p spectrum (see <xref ref-type="fig" rid="F4">Figure 4C</xref>) shows an asymmetric peak that consists of contributions from S in 2D CoS<sub>2</sub> and the 1T phase. Furthermore, comparing the overall signals of Co, Mo, and S, the molecuar formula of 1T Co-MoS<sub>2</sub> is determined to be Mo<sub>0.67</sub>Co<sub>0.32</sub>S<sub>1.89</sub>, with 11% sulfur vacancies in the top layer (see <xref ref-type="sec" rid="s10">Supplementary Material S1.2</xref>, <xref ref-type="sec" rid="s10">Supplementary Table S2</xref>). The high number of sulfur vacancies is expected due to the highly reducing environment used during the synthesis in the ReactorSTM. In comparison, the molecular formula of the 1H Co-promoted MoS<sub>2</sub> from the control experiment is determined to be Mo<sub>0.65</sub>Co<sub>0.35</sub>S<sub>2.05</sub>.</p>
<fig id="F4" position="float">
<label>FIGURE 4</label>
<caption>
<p>
<bold>(A&#x2013;C)</bold> Mo 3d, Co 2p<sub>3/2</sub>, and S 2p XPS spectra of the Co-Mo precursor supported on Au(111) after sulfidation in the high-pressure sulfo-reductive gases at 603&#xa0;K.</p>
</caption>
<graphic xlink:href="fphy-11-1240731-g004.tif"/>
</fig>
<p>As an additional control experiment, the control sample containing 1H Co-promoted MoS<sub>2</sub> slabs grown using 2 &#xd7; 10<sup>&#x2212;6</sup>&#xa0;mbar H<sub>2</sub>S was loaded into the ReactorSTM and exposed to the high-pressure sulfo-reductive gas mixture (9:1 H<sub>2</sub>:CH<sub>3</sub>SH, 1&#xa0;bar) at 603&#xa0;K for up to 6&#xa0;h. <xref ref-type="fig" rid="F5">Figure 5</xref> shows a large-scale STM image obtained <italic>in situ</italic> after 6&#xa0;h. Comparing <xref ref-type="fig" rid="F1">Figures 1</xref>, <xref ref-type="fig" rid="F5">5</xref>, we observe that the morphology of the Co-promoted MoS<sub>2</sub> slabs is largely preserved. Under these gas conditions, we expect that the edges of the Co-promoted MoS<sub>2</sub> slabs are reduced to the same degree as in our high-pressure sullfidation experiment since the gas conditions are identical. In <xref ref-type="fig" rid="F5">Figure 5</xref>, we clearly observe that all the Co-promoted MoS<sub>2</sub> slabs remain in the 1H state and do not transform into the 1T state, as can also be seen in the atom-resolved inset where 1H Co-promoted MoS<sub>2</sub> slabs with BRIM sites are clearly imaged. This shows that the 1T state is accessible at the gas conditions and temperatures used, if and only if, the thermodynamically stable 1H state has not already been formed. A schematic summarizing all our findings is shown in <xref ref-type="fig" rid="F6">Figure 6</xref>.</p>
<fig id="F5" position="float">
<label>FIGURE 5</label>
<caption>
<p>
<italic>In situ</italic> STM image of vacuum-synthesized Co-promoted MoS<sub>2</sub> slabs after 6&#xa0;h under the sulfo-reductive gas environment (1&#xa0;bar, 9:1 H<sub>2</sub>:CH<sub>3</sub>SH, 603&#xa0;K). The inset shows atom-resolved 1H Co-promoted MoS<sub>2</sub> slabs with BRIM sites. STM image acquired with a sample voltage of &#x2212;0.3&#xa0;V and tunneling current of 500&#xa0;pA.</p>
</caption>
<graphic xlink:href="fphy-11-1240731-g005.tif"/>
</fig>
<fig id="F6" position="float">
<label>FIGURE 6</label>
<caption>
<p>Schematic diagram describing the kinetically favorable and unfavorable routes for the 1T Co-promoted MoS<sub>2</sub> formation.</p>
</caption>
<graphic xlink:href="fphy-11-1240731-g006.tif"/>
</fig>
</sec>
<sec sec-type="conclusion" id="s4">
<title>4 Conclusion</title>
<p>We have demonstrated using the <italic>in situ</italic> STM imaging capabilities of the ReactorSTM, that using sufficiently reducing environments during the crystallization phase can favor the formation of metallic 1T Co-promoted MoS<sub>2</sub>. On the other hand, if 1H Co-promoted MoS<sub>2</sub> is already formed, then there are large kinetic barriers that hinder the formation of a sufficient number of S vacancies to drive the transformation to the 1T phase through atomic S-layer sliding. These observations with the STM are confirmed and supported very well by the corresponding XPS spectra which show that the 1T Co-MoS<sub>2</sub> slabs have a large number of sulfur vacancies in comparison to the 1H Co-MoS<sub>2</sub> slabs. The formation of pure 1T Co-promoted MoS<sub>2</sub> under sulfo-reductive conditions without an alkali metal intercalator is remarkable as it demonstrates the feasibility for directly synthesizing monolayers of pure 1T or 1H Co-promoted MoS<sub>2</sub>. This is of great relevance for fundamental research in optoelectronics, green hydrogen production, and heterogeneous and electro-catalysis.</p>
</sec>
</body>
<back>
<sec sec-type="data-availability" id="s5">
<title>Data availability statement</title>
<p>The original contributions presented in the study are included in the article/<xref ref-type="sec" rid="s10">Supplementary Material</xref>, further inquiries can be directed to the corresponding author.</p>
</sec>
<sec id="s6">
<title>Author contributions</title>
<p>MP performed all experiments and analyzed all data. IG conceived and supervised the project. All authors contributed to the article and approved the submitted version.</p>
</sec>
<sec id="s7">
<title>Funding</title>
<p>This project received funding from the Leiden Institute of Chemistry, Leiden University.</p>
</sec>
<sec sec-type="COI-statement" id="s8">
<title>Conflict of interest</title>
<p>The authors declare that the research was conducted in the absence of any commercial or financial relationships that could be construed as a potential conflict of interest.</p>
</sec>
<sec sec-type="disclaimer" id="s9">
<title>Publisher&#x2019;s note</title>
<p>All claims expressed in this article are solely those of the authors and do not necessarily represent those of their affiliated organizations, or those of the publisher, the editors and the reviewers. Any product that may be evaluated in this article, or claim that may be made by its manufacturer, is not guaranteed or endorsed by the publisher.</p>
</sec>
<sec id="s10">
<title>Supplementary material</title>
<p>The Supplementary Material for this article can be found online at: <ext-link ext-link-type="uri" xlink:href="https://www.frontiersin.org/articles/10.3389/fphy.2023.1240731/full#supplementary-material">https://www.frontiersin.org/articles/10.3389/fphy.2023.1240731/full&#x23;supplementary-material</ext-link>
</p>
<supplementary-material xlink:href="DataSheet1.pdf" id="SM1" mimetype="application/pdf" xmlns:xlink="http://www.w3.org/1999/xlink"/>
</sec>
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