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<front>
<journal-meta>
<journal-id journal-id-type="publisher-id">Front. Earth Sci.</journal-id>
<journal-title>Frontiers in Earth Science</journal-title>
<abbrev-journal-title abbrev-type="pubmed">Front. Earth Sci.</abbrev-journal-title>
<issn pub-type="epub">2296-6463</issn>
<publisher>
<publisher-name>Frontiers Media S.A.</publisher-name>
</publisher>
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<article-meta>
<article-id pub-id-type="publisher-id">1399541</article-id>
<article-id pub-id-type="doi">10.3389/feart.2024.1399541</article-id>
<article-categories>
<subj-group subj-group-type="heading">
<subject>Earth Science</subject>
<subj-group>
<subject>Original Research</subject>
</subj-group>
</subj-group>
</article-categories>
<title-group>
<article-title>Characterization of the evolution of thermal maturity and pore structure of continental organic-rich shales</article-title>
<alt-title alt-title-type="left-running-head">Li et al.</alt-title>
<alt-title alt-title-type="right-running-head">
<ext-link ext-link-type="uri" xlink:href="https://doi.org/10.3389/feart.2024.1399541">10.3389/feart.2024.1399541</ext-link>
</alt-title>
</title-group>
<contrib-group>
<contrib contrib-type="author" corresp="yes">
<name>
<surname>Li</surname>
<given-names>Yanju</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
<xref ref-type="corresp" rid="c001">&#x2a;</xref>
<uri xlink:href="https://loop.frontiersin.org/people/2674988/overview"/>
<role content-type="https://credit.niso.org/contributor-roles/conceptualization/"/>
<role content-type="https://credit.niso.org/contributor-roles/Writing - review &#x26; editing/"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Wu</surname>
<given-names>Yuandong</given-names>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
<role content-type="https://credit.niso.org/contributor-roles/methodology/"/>
<role content-type="https://credit.niso.org/contributor-roles/writing-original-draft/"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Zhao</surname>
<given-names>Ruirui</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<role content-type="https://credit.niso.org/contributor-roles/data-curation/"/>
<role content-type="https://credit.niso.org/contributor-roles/investigation/"/>
<role content-type="https://credit.niso.org/contributor-roles/Writing - review &#x26; editing/"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Jiang</surname>
<given-names>Shengling</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<uri xlink:href="https://loop.frontiersin.org/people/2238326/overview"/>
<role content-type="https://credit.niso.org/contributor-roles/methodology/"/>
<role content-type="https://credit.niso.org/contributor-roles/supervision/"/>
<role content-type="https://credit.niso.org/contributor-roles/Writing - review &#x26; editing/"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Du</surname>
<given-names>Xuanhong</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<role content-type="https://credit.niso.org/contributor-roles/validation/"/>
<role content-type="https://credit.niso.org/contributor-roles/Writing - review &#x26; editing/"/>
</contrib>
</contrib-group>
<aff id="aff1">
<sup>1</sup>
<institution>School of New Energy</institution>, <institution>Longdong University</institution>, <addr-line>Qingyang</addr-line>, <country>China</country>
</aff>
<aff id="aff2">
<sup>2</sup>
<institution>College of Geographical Science</institution>, <institution>Qinghai Normal University</institution>, <addr-line>Xining</addr-line>, <country>China</country>
</aff>
<aff id="aff3">
<sup>3</sup>
<institution>PKU-HKUST ShenZhen-HongKong Institution</institution>, <addr-line>Shenzhen</addr-line>, <country>China</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/1046379/overview">Yunyan Ni</ext-link>, China University of Petroleum, China</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/1224050/overview">Qingyong Luo</ext-link>, China University of Petroleum, China</p>
<p>
<ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/1257670/overview">Peng Li</ext-link>, SINOPEC Petroleum Exploration and Production Research Institute, China</p>
</fn>
<corresp id="c001">&#x2a;Correspondence: Yanju Li, <email>lyj890609@email.cugb.edu.cn</email>
</corresp>
</author-notes>
<pub-date pub-type="epub">
<day>16</day>
<month>05</month>
<year>2024</year>
</pub-date>
<pub-date pub-type="collection">
<year>2024</year>
</pub-date>
<volume>12</volume>
<elocation-id>1399541</elocation-id>
<history>
<date date-type="received">
<day>12</day>
<month>03</month>
<year>2024</year>
</date>
<date date-type="accepted">
<day>02</day>
<month>05</month>
<year>2024</year>
</date>
</history>
<permissions>
<copyright-statement>Copyright &#xa9; 2024 Li, Wu, Zhao, Jiang and Du.</copyright-statement>
<copyright-year>2024</copyright-year>
<copyright-holder>Li, Wu, Zhao, Jiang and Du</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>To clarify the evolution of thermal maturity and pore structure in continental organic-rich shales, calcareous shales of the Liaohe Basin (China) were pyrolyzed, and examined using Raman spectroscopy, Fourier transform infrared spectroscopy (FTIR), X-ray diffraction (XRD), X-ray photoelectron spectroscopy (XPS), scanning electron microscopy (SEM), nitrogen sorption isotherms, and nuclear magnetic resonance (NMR) spectroscopy. The increase in Raman G&#x2012;D band separation and decrease in Raman I<sub>D</sub>/I<sub>G</sub> ratio with increasing thermal maturity indicate that these parameters provide superior thermal maturity indicators. This is also confirmed by the good linear correlation of G&#x2012;D band shifts and I<sub>D</sub>/I<sub>G</sub> with vitrinite reflectance (VR) and maximum temperature (T<sub>max</sub>), respectively. The relative detection accuracy (DA), sampling requirements (SR), sample preparation (SP), detection time (DT), and equipment requirement (ER) of VR, G&#x2012;D band shifts, I<sub>D</sub>/I<sub>G</sub>, T<sub>max</sub>, FTIR, and XPS indicate that Raman analysis is a simple, quick, and robust method to evaluate thermal maturity. The moderate SR, complex SP, and long DT suggest that VR and T<sub>max</sub> are less widely applicable for characterizing thermal maturity. The FTIR and XPS techniques provide semi-quantitative maturity indicators with poor DA and high ER. Pores observed within organic matter and minerals under SEM indicate that an increase in thermal maturity not only affects the development of organic pores but is also beneficial for the formation of mineral dissolution pores, such as those formed during the transformation of Na<sub>0.95</sub>Ca<sub>0.16</sub>Al<sub>1.16</sub>Si<sub>2.84</sub>O<sub>8</sub> to Na<sub>0.84</sub>Ca<sub>0.02</sub>Al<sub>1.02</sub>Si<sub>2.98</sub>O<sub>8</sub>, a process confirmed by XRD. The BET and NMR data also indicate that the development of pore structure is closely related to the evolution of thermal maturity in calcareous shale. During the initial stage, primary pores are filled by bitumen generated from kerogen; this leads to a decrease in transition pores, mesopores, and shale porosity, and reduced pore connectivity. Then, secondary nanoscale pores, transition pores, and mesopores increase with increasing thermal maturity. The peak in secondary porosity is consistent with the liquid hydrocarbon production rate peak, a process that increases shale porosity and leads to improved pore connectivity. The dissolution of minerals induced by organic acids may also contribute to this secondary porosity. With a further increase in thermal maturity, secondary porosity at the microscale is further developed, while transition pores and mesopores collapse, resulting in reduced pore connectivity. The poor pore connectivity that occurs at both low and high VR values may be more conducive to the preservation of shale oil and gas. This study is significant for research into the evolution of thermal maturity and pore structure in continental organic-rich shales.</p>
</abstract>
<kwd-group>
<kwd>continental organic-rich shales</kwd>
<kwd>evaluation</kwd>
<kwd>maturity</kwd>
<kwd>pore structures</kwd>
<kwd>SEM</kwd>
<kwd>NMR</kwd>
</kwd-group>
<custom-meta-wrap>
<custom-meta>
<meta-name>section-at-acceptance</meta-name>
<meta-value>Geochemistry</meta-value>
</custom-meta>
</custom-meta-wrap>
</article-meta>
</front>
<body>
<sec id="s1">
<title>1 Introduction</title>
<p>Shale gas is a type of unconventional petroleum, which is generated from, and hosted in, organic-rich shales. There are three states in which shale gas exists: 1) free state, distributed in micro-cracks and macropores; 2) adsorbed state, adhered on the surface of organic matter and clay mineral micropores; and 3) dissolved state, dispersed in water and oil. Among these, free gas and adsorbed gas are the main components of shale gas (<xref ref-type="bibr" rid="B16">Curtis, 2002</xref>; <xref ref-type="bibr" rid="B35">Ji et al., 2017</xref>; <xref ref-type="bibr" rid="B119">Zhu et al., 2021</xref>). Therefore, investigating the pore composition and development characteristics of shale and associated influencing factors is critical for shale oil and gas exploration and development.</p>
<p>According to the relationship between shale pores and mineral particles, shale pores can be divided into mineral pores, organic pores, and micro-fracture pores. In organic-rich shales, organic pores are the most important pore component because they can comprise up to 70% of the total pore volume of the shale, whilst also having good connectivity (<xref ref-type="bibr" rid="B57">L&#xf6;hr et al., 2015</xref>; <xref ref-type="bibr" rid="B35">Ji et al., 2017</xref>; <xref ref-type="bibr" rid="B4">Borjigin et al., 2021</xref>; <xref ref-type="bibr" rid="B113">Zhang et al., 2022</xref>; <xref ref-type="bibr" rid="B115">Zheng et al., 2022</xref>). Investigating pore composition and evolution as organic-rich shales mature has important theoretical and practical significance for predicting shale gas content and evaluating shale gas resources.</p>
<p>Highly productive shale gas has been shown to be strongly associated with high-maturity shales (<xref ref-type="bibr" rid="B99">Wu et al., 2019</xref>; <xref ref-type="bibr" rid="B10">Chen et al., 2020</xref>; <xref ref-type="bibr" rid="B82">Song et al., 2021</xref>; <xref ref-type="bibr" rid="B117">Zheng et al., 2021</xref>; <xref ref-type="bibr" rid="B6">Cao et al., 2022</xref>), indicating that highly productive shale gas has inevitably experienced a high evolutionary stage and deep burial. In this long and complicated evolution process, the hydrocarbon generation of organic matter and the transformation of clay minerals in shale may have mutual influence. Such as, the organic acids formed in the process of hydrocarbon generation can accelerate the dissolution of minerals and affect the transformation of clay minerals; clay minerals also have catalytic effect on hydrocarbon generation and liquid hydrocarbon cracking. Previous investigators mainly focus on the change of organic pore structure with maturity, and few studies have investigated the effect of organic-inorganic interaction during shale thermal evolution on the formation and evolution of shale pores. At the same time, there are few experimental studies to discuss the influences of organic-inorganic interaction on mineral and organic pores with thermal maturity.</p>
<p>Generally, vitrinite reflectance (VR) and maximum temperature (T<sub>max</sub>) values provide good thermal maturity indicators for source rocks and organic matter (<xref ref-type="bibr" rid="B121">Hunt, 1996</xref>; <xref ref-type="bibr" rid="B20">Evenick, 2021</xref>; <xref ref-type="bibr" rid="B122">Al-Hajeri et al., 2021</xref>; <xref ref-type="bibr" rid="B57">Lohr et al., 2015</xref>; <xref ref-type="bibr" rid="B127">Waliczek et al., 2021</xref>). However, for some samples, VR and T<sub>max</sub> cannot accurately reflect maturity due to a lack of vitrinite or low S<sub>2</sub> values (<xref ref-type="bibr" rid="B47">Lewan and Kotarba, 2014</xref>; <xref ref-type="bibr" rid="B38">Katz and Lin, 2021</xref>), this is the case for highly mature marine shales in the Sichuan Basin, China, and for limestone source rocks with low organic matter contents. Therefore, additional maturity indicators, which are easy to detect and provide high-performance, need to be developed to cover organic matter from a wide range of source rocks, deposited under different sedimentary settings, or at different stages of thermal evolution.</p>
<p>Owing to the success of marine shale gas exploration in both Permian shales and the Devonian&#x2012;Carboniferous Bakken shale of North America, many investigators have focused on the pore structure and development of marine shales (<xref ref-type="bibr" rid="B32">Hao et al., 2013</xref>; <xref ref-type="bibr" rid="B31">Hao and Zou, 2013</xref>; <xref ref-type="bibr" rid="B107">Yang et al., 2017</xref>; <xref ref-type="bibr" rid="B96">Wu et al., 2018</xref>; <xref ref-type="bibr" rid="B109">Yang et al., 2018</xref>; <xref ref-type="bibr" rid="B79">Shi et al., 2021</xref>; <xref ref-type="bibr" rid="B106">Xu et al., 2021</xref>), while there have been relatively few investigations of the pore evolution of continental organic-rich shales. Continental shale gas has great potential, and accounts for one-third of the total shale gas resources of China (<xref ref-type="bibr" rid="B21">Fan et al., 1980</xref>; <xref ref-type="bibr" rid="B23">Fu et al., 1988</xref>; <xref ref-type="bibr" rid="B28">Grice et al., 1998</xref>). Therefore, understanding the evolution of pore textures in continental organic-rich shales can contribute meaningfully to global shale gas exploration and development, especially in China.</p>
<p>In this study, we investigated the evolution of the thermal maturity and mineral/organic pore structure of continental organic-rich shales under semi-closed hydrous conditions to clarify the evolution of thermal maturity, and mineral/organic pores during shale gas generation. Calcareous shales from the Liaohe Basin (China) were pyrolyzed, and examined using laser Raman spectroscopy, Fourier transform infrared spectroscopy (FTIR), X-ray diffraction (XRD), X-ray photoelectron spectroscopy (XPS), scanning electron microscopy (SEM), nitrogen sorption isotherms (BET), and nuclear magnetic resonance (NMR) spectroscopy. Raman, FTIR, XRD, and XPS were used to detect changes in organic functional groups and mineral composition; SEM, BET, and NMR were used to analyze the evolution of pore texture and formation. This study has substantial implications for understanding the evolution of thermal maturity and pore structure in continental organic-rich shales, and for global shale gas exploration and development.</p>
</sec>
<sec id="s2">
<title>2 Samples and experiments</title>
<sec id="s2-1">
<title>2.1 Samples</title>
<p>Calcareous shales were selected from the Shu 13 drill core from the Liaohe Basin (Shahejie Formation), as shown in <xref ref-type="fig" rid="F1">Figure 1</xref>. <xref ref-type="table" rid="T1">Table 1</xref> presents the geochemical parameters of these shales; details of the geochemical analysis methods were presented in a previous study (<xref ref-type="bibr" rid="B96">Wu et al., 2018</xref>). The geochemical data indicate that the kerogen in the calcareous shales is type-I kerogen and is immature (VR &#x3d; 0.40%R<sub>o</sub>; T<sub>max</sub> &#x3d; 434 &#xb0;C). <xref ref-type="table" rid="T1">Table 1</xref> also shows that the hydrogen index (HI) of the calcareous shales is 792, which further suggests that they are oil-prone source rocks (<xref ref-type="table" rid="T1">Table 1</xref>; <xref ref-type="bibr" rid="B96">Wu et al., 2018</xref>).</p>
<fig id="F1" position="float">
<label>FIGURE 1</label>
<caption>
<p>Location <bold>(A)</bold> and sketch structural <bold>(B)</bold> maps, and schematic geological cross-section <bold>(C)</bold> of Liaohe Basin.</p>
</caption>
<graphic xlink:href="feart-12-1399541-g001.tif"/>
</fig>
<table-wrap id="T1" position="float">
<label>TABLE 1</label>
<caption>
<p>Geochemical parameters of the organic-rich shale study samples (after <xref ref-type="bibr" rid="B96">Wu et al., 2018</xref>).</p>
</caption>
<table>
<thead valign="top">
<tr>
<th align="center">Well</th>
<th align="center">Stratum</th>
<th align="center">Depth (m)</th>
<th align="center">Lithology</th>
<th align="center">TOC (%)</th>
<th align="center">HI (mg/g)</th>
<th align="center">OI (mg/g)</th>
<th align="center">S<sub>1</sub> (mg/g)</th>
<th align="center">S<sub>2</sub> (mg/g)</th>
<th align="center">T<sub>max</sub> (<sup>o</sup>C)</th>
<th align="left">VR (%R<sub>o</sub>)</th>
<th align="center">Type of Kerogen</th>
</tr>
</thead>
<tbody valign="top">
<tr>
<td align="center">Shu13</td>
<td align="center">Es3</td>
<td align="center">1,387-1,390</td>
<td align="center">Calcareous Shale</td>
<td align="center">8.73</td>
<td align="center">792</td>
<td align="center">23</td>
<td align="center">0.42</td>
<td align="center">69.2</td>
<td align="center">434</td>
<td align="center">0.40</td>
<td align="center">I</td>
</tr>
</tbody>
</table>
</table-wrap>
</sec>
<sec id="s2-2">
<title>2.2 Hydrous pyrolysis</title>
<p>A WYMN-3 HTHP instrument was used to simulate the thermal evolution process of continental organic-rich shales under geological conditions. The maximum simulation temperature of the WYMN-3 HTHP is 550&#xb0;C, while the maximum values of water pressure and lithostatic pressure are 2,800 bar and 1,200 bar, respectively. A schematic diagram of the main structure of the instrument can be found in <xref ref-type="bibr" rid="B112">Zhang et al. (2020)</xref> and <xref ref-type="bibr" rid="B97">Wu et al. (2021)</xref>. Hydrous pyrolysis was conducted at 350&#x2013;520&#xb0;C, with 400&#x2013;800 bar water pressure, and 1,000&#x2013;2000 bar lithostatic pressure. To simulate the entire evolution of the thermal maturity and pore structure of continental organic-rich shales, immature calcareous shale was used, and the pyrolysis temperatures were higher than classical hydrous pyrolysis (e.g., <xref ref-type="bibr" rid="B33">Hill et al., 2003</xref>; <xref ref-type="bibr" rid="B102">Xie et al., 2016</xref>). Detailed conditions of the pyrolysis experiments can be found in <xref ref-type="bibr" rid="B96">Wu et al. (2018)</xref>.</p>
</sec>
<sec id="s2-3">
<title>2.3 Scanning electron microscopy (SEM)</title>
<p>The SEM analyses were performed at the South China University of Technology, using a Merlin Compact (Zeiss, Germany) instrument, equipped with an X-ray energy spectrometer (Oxford, England). The resolution of this instrument can reach 1.0 nm at 15 kV accelerating voltage and 2 mm working distance, in high vacuum mode. The accelerating voltage used herein was 20 kV.</p>
</sec>
<sec id="s2-4">
<title>2.4 Raman spectroscopy</title>
<p>The source rocks, before and after pyrolysis, were examined by Raman spectroscopy using an Alpha 300M Raman spectrometer (WITec, Germany). The wavelengths of the laser source were 532 and 732 nm, and the power of the laser source was 5 mW.</p>
<p>Raman spectroscopy can record the entire spectrum of each sample. Generally, a Raman spectrum comprises a peak position, peak intensity, and peak area. To further resolve the sample information contained within a Raman spectrum, curve-fitting is usually performed. In this investigation, Gaussian&#x2012;Lorentzian fitting was applied to the Raman spectra of all examined source rocks, before and after pyrolysis; at least 150 iterations were used until the best fit was achieved. Five peaks or bands, including D, G, D2, D3, and D4, can be fitted for organic matter evaluation in shale, as shown in <xref ref-type="fig" rid="F2">Figure 2</xref> (<xref ref-type="bibr" rid="B40">Khatibi et al., 2018</xref>; <xref ref-type="bibr" rid="B123">Khatibi et al., 2019</xref>; <xref ref-type="bibr" rid="B3">Birdwell et al., 2021</xref>; <xref ref-type="bibr" rid="B15">Craddock and Sauerer, 2022</xref>); all of these were fitted herein. However, only the D and G bands, which were most common and had the highest intensity, were considered further in this study (<xref ref-type="table" rid="T2">Table 2</xref>); the minor bands (D2, D3, and D4) were often unclear in both appearance and significance (cf. <xref ref-type="bibr" rid="B2">Beyssac et al., 2003</xref>).</p>
<fig id="F2" position="float">
<label>FIGURE 2</label>
<caption>
<p>Example of spectral deconvolution and Raman band identification. <bold>(A)</bold> Sample with a VR of 1.76%R<sub>o</sub>. <bold>(B)</bold> Sample with a VR of 2.14%R<sub>o.</sub>
</p>
</caption>
<graphic xlink:href="feart-12-1399541-g002.tif"/>
</fig>
<table-wrap id="T2" position="float">
<label>TABLE 2</label>
<caption>
<p>Major D- and G-band shifts for the residue and original sample.</p>
</caption>
<table>
<thead valign="top">
<tr>
<th align="center">Sample no.</th>
<th align="center">D band</th>
<th align="center">G band</th>
<th align="center">G-D band shifts</th>
<th align="center">VR</th>
<th align="center">T<sub>max</sub>
</th>
</tr>
</thead>
<tbody valign="top">
<tr>
<td align="center">Origin Samples</td>
<td align="center">1,358</td>
<td align="center">1,574</td>
<td align="center">216</td>
<td align="center">0.4</td>
<td align="center">434</td>
</tr>
<tr>
<td align="center">311</td>
<td align="center">1,356</td>
<td align="center">1,576</td>
<td align="center">220</td>
<td align="center">0.77</td>
<td align="center">446</td>
</tr>
<tr>
<td align="center">312</td>
<td align="center">1,348</td>
<td align="center">1,583</td>
<td align="center">235</td>
<td align="center">1.46</td>
<td align="center">455</td>
</tr>
<tr>
<td align="center">313</td>
<td align="center">1,346</td>
<td align="center">1,583</td>
<td align="center">237</td>
<td align="center">1.76</td>
<td align="center">467</td>
</tr>
<tr>
<td align="center">314</td>
<td align="center">1,346</td>
<td align="center">1,586</td>
<td align="center">240</td>
<td align="center">2.14</td>
<td align="center">568</td>
</tr>
<tr>
<td align="center">315</td>
<td align="center">1,341</td>
<td align="center">1,586</td>
<td align="center">245</td>
<td align="center">2.23</td>
<td align="center">605</td>
</tr>
<tr>
<td align="center">321</td>
<td align="center">1,336</td>
<td align="center">1,569</td>
<td align="center">233</td>
<td align="center">0.81</td>
<td align="center">449</td>
</tr>
<tr>
<td align="center">322</td>
<td align="center">1,341</td>
<td align="center">1,576</td>
<td align="center">235</td>
<td align="center">1.50</td>
<td align="center">461</td>
</tr>
<tr>
<td align="center">323</td>
<td align="center">1,348</td>
<td align="center">1,588</td>
<td align="center">240</td>
<td align="center">1.95</td>
<td align="center">474</td>
</tr>
<tr>
<td align="center">324</td>
<td align="center">1,338</td>
<td align="center">1,583</td>
<td align="center">245</td>
<td align="center">2.29</td>
<td align="center">573</td>
</tr>
<tr>
<td align="center">325</td>
<td align="center">1,336</td>
<td align="center">1,583</td>
<td align="center">247</td>
<td align="center">2.44</td>
<td align="center">607</td>
</tr>
</tbody>
</table>
</table-wrap>
</sec>
<sec id="s2-5">
<title>2.5 Infrared spectroscopy (IR)</title>
<p>The infrared spectra of source rocks, before and after pyrolysis, were detected using a Perkin Elmer Spectrum 100. Each spectrum was the result of 32 scans, and the resolution was 4 cm<sup>&#x2212;1</sup> in the frequency range of 4,000&#x2013;650 cm<sup>&#x2212;1</sup>.</p>
</sec>
<sec id="s2-6">
<title>2.6 X-ray diffraction (XRD)</title>
<p>X-ray diffraction patterns of the source rocks, before and after pyrolysis, were obtained using a Rigaku D/Max 2550VB/PC diffractometer equipped with Cu K&#x3b1; radiation (&#x3bb; &#x3d; 1.5406 &#xc5;). Duplicate analyses were performed to ensure reproducibility.</p>
</sec>
<sec id="s2-7">
<title>2.7 X-ray photoelectron spectroscopy (XPS)</title>
<p>Data from the source rocks, before and after pyrolysis, were obtained using a Kratos Axis ULTRA X-ray Photoelectron Spectrometer. Monochromatic Al K&#x3b1; X-rays (1,486.6 eV) at 150 W (15 kV, 10 mA) were used. The C 1s (286.8 eV) peak was used as an internal standard for correction. For full spectrum scanning, the transit energy was 100 eV, and the step size was 1 eV; for narrow spectrum scanning, the passage energy was 30 eV and the step size was 0.1 eV. To obtain good experimental results, powdered samples ground to &#x2264;0.074 mm were made into compressed tablets for XPS analysis. In XPS C 1s spectra, the ordinate is electron counts, and the abscissa is electron binding energy (B.E.). Based on the different binding energies of carbon elements in different valence states, the XPS C 1s spectra of samples obtained from our experiments were fitted using Casa XPS software. The Shirley model was adopted for back-bottom deduction, and 70% Gaussian and 30% Lorentz hybrid lines were adopted. In the process of peak fitting, the peak position and half-width of all fitted peaks were fixed, and the half-width was 1.5 (&#xb1;0.1) eV.</p>
</sec>
<sec id="s2-8">
<title>2.8 Low-temperature N<sub>2</sub> adsorption</title>
<p>An ASAP 2020 Plus HD88 SA analyzer (Micromeritics Instruments Corporation, USA) was used to measure the surface area (SA) and pore volume (PV) of the source rocks, before and after pyrolysis. All samples were crushed to 80 mesh and extracted with chloroform for 72 h, then degassed at 150 &#xb0;C for 6 h under vacuum before low-temperature N<sub>2</sub> adsorption analysis. The N<sub>2</sub> adsorption&#x2013;desorption isotherm measurements were conducted at the temperature of liquid nitrogen (77.3 K) with a relative pressure P/P0 range of 0.01&#x2013;0.998.</p>
</sec>
<sec id="s2-9">
<title>2.9 Nuclear magnetic resonance (NMR) spectroscopy</title>
<p>The MicroMR series NMR analyzer used in this study was produced by Suzhou Newmag analytical instrument corporation. The NMR core analyzer can be used as free-induction decay (FID) and Carr-Purcell-Meiboom-Gill pulse sequence (CPMG). sequence. To obtain a more complete NMR response signal and improve the signal-to-noise ratio and resolution, CPMG&#x2012;T<sub>2</sub> measurements were used. The pyrolyzed samples were dried under vacuum, then the dry columnar samples were saturated with deionized water. NMR T<sub>2</sub> distributions were measured using 0.3 ms echo spacing, 3,000 ms waiting time, 10,000 echo numbers, and 64 scan times (<xref ref-type="bibr" rid="B116">Zheng et al., 2019</xref>).</p>
</sec>
</sec>
<sec sec-type="results|discussion" id="s3">
<title>3 Results and discussion</title>
<sec id="s3-1">
<title>3.1 The characterization of Raman spectroscopy, FTIR, XRD and XPS before and after pyrolysis of samples</title>
<p>Generally, VR and T<sub>max</sub> represent good thermal maturity indicators of source rocks and organic matter (<xref ref-type="bibr" rid="B121">Hunt, 1996</xref>; <xref ref-type="bibr" rid="B20">Evenick, 2021</xref>; <xref ref-type="bibr" rid="B122">Al-Hajeri et al., 2021</xref>; <xref ref-type="bibr" rid="B57">Lohr et al., 2015</xref>; <xref ref-type="bibr" rid="B127">Waliczek et al., 2021</xref>).</p>
<sec id="s3-1-1">
<title>3.1.1 Raman spectroscopy</title>
<p>Previous investigations have shown that with increasing kerogen maturity, aromaticity increases and there is a concurrent decrease in H, O, N, and S content (<xref ref-type="bibr" rid="B121">Hunt, 1996</xref>; <xref ref-type="bibr" rid="B45">Lewan, 1997</xref>; <xref ref-type="bibr" rid="B86">Sun et al., 2021</xref>). These changes may be reflected in the Raman spectra of kerogen at the molecular scale (<xref ref-type="bibr" rid="B123">Khatibi et al., 2019</xref>). Hence, Raman spectroscopy can be used to investigate the nature and degree of graphitization of kerogenous carbon (<xref ref-type="bibr" rid="B8">Charisiou et al., 2018</xref>). The Raman analysis results of pyrolyzed samples are presented in <xref ref-type="fig" rid="F3">Figure 3</xref>. Both samples show Raman bands in the 800&#x2013;2000 cm<sup>&#x2212;1</sup> region of the spectrum; these are the carbon G- and D-bands, which appear between 1,500 and 1,600 cm<sup>&#x2212;1</sup>, and between 1,300 and 1,400 cm<sup>&#x2212;1</sup>, respectively. The former is induced by the presence of crystalline graphitic/sp<sup>2</sup> carbon atoms and involves out-of-phase intra-layer displacement in the graphene structure; the latter originates from sp<sup>3</sup> hybridization and relates to polycrystalline imperfect graphite (<xref ref-type="bibr" rid="B48">Li et al., 2017</xref>; <xref ref-type="bibr" rid="B8">Charisiou et al., 2018</xref>; <xref ref-type="bibr" rid="B25">Ghaffar et al., 2018</xref>). The degree of crystallinity of the carbon formed during the thermal evolution of organic matter can also be reflected by the intensity ratio of the D- and G-bands (I<sub>D</sub>/I<sub>G</sub>), where lower I<sub>D</sub>/I<sub>G</sub> values suggest higher crystallinity, because a higher quantity of graphitized carbon is generated during organic matter evolution (<xref ref-type="bibr" rid="B34">Hou et al., 2019</xref>). In this investigation, the I<sub>D</sub>/I<sub>G</sub> values for the pyrolyzed samples follow the order 0.89 &#x3e; 0.65 &#x3e;0.63 &#x3e; 0.51 &#x3e; 0.40 &#x3e; 0.38 corresponding to VRs of 0.77%R<sub>0</sub> &#x3c;1.46%R<sub>o</sub> &#x3c; 1.76%R<sub>o</sub> &#x3c; 1.95%R<sub>o</sub> &#x3c; 2.14%R<sub>o</sub> &#x3c; 2.44%R<sub>o</sub>. A lower I<sub>D</sub>/I<sub>G</sub> ratio may illustrate higher thermal maturity (<xref ref-type="bibr" rid="B124">Muirhead et al., 2021</xref>; <xref ref-type="bibr" rid="B114">Zhang et al., 2021</xref>), the deduction of which matches the report of <xref ref-type="bibr" rid="B125">Sauerer et al. (2017)</xref>. For the pyrolyzed continental shales in this investigation, the degree of crystallinity of kerogenous carbon increased with an increase in VR, and this trend was more pronounced for continental shales with VR &#x3e; 1.46%R<sub>o</sub> (<xref ref-type="fig" rid="F3">Figure 3</xref>); this is also consistent with previously noted increases in the aromaticity of kerogen (<xref ref-type="bibr" rid="B1">Beyssac et al., 2002</xref>; <xref ref-type="bibr" rid="B58">L&#xfc;nsdorf, 2016</xref>). A decrease in the I<sub>D</sub>/I<sub>G</sub> ratio may indicate an increase in larger aromatic clusters and improved ordering of the existing organic compounds within the kerogen.</p>
<fig id="F3" position="float">
<label>FIGURE 3</label>
<caption>
<p>Raman spectra of kerogen with different VR.</p>
</caption>
<graphic xlink:href="feart-12-1399541-g003.tif"/>
</fig>
<p>Previous investigations have reported that G- and D-band shifts increase with maturity until the dry gas window is reached (<xref ref-type="bibr" rid="B40">Khatibi et al., 2018</xref>; <xref ref-type="bibr" rid="B17">Delarue et al., 2021</xref>; <xref ref-type="bibr" rid="B30">Hackley et al., 2021</xref>); the D-band shifts towards lower wavenumbers and the G-band shifts towards higher wavenumbers (<xref ref-type="bibr" rid="B39">Kelemen and Fang, 2001</xref>; <xref ref-type="bibr" rid="B40">Khatibi et al., 2018</xref>; <xref ref-type="bibr" rid="B30">Hackley et al., 2021</xref>; <xref ref-type="bibr" rid="B17">Delarue et al., 2021</xref>). These increases in separation between the D- and G-bands may be caused by the increase in number of larger aromatic clusters and improved structural ordering of kerogen as maturity increases (<xref ref-type="bibr" rid="B75">Schito et al., 2017</xref>; <xref ref-type="bibr" rid="B74">2021</xref>). Further investigations have speculated that these shifts may be attributed to the wavelength dependence of the D-band position and the independence of the excitation energy of the G-band position in the Raman spectra of carbonaceous materials (<xref ref-type="bibr" rid="B62">Marshall et al., 2010</xref>; <xref ref-type="bibr" rid="B58">L&#xfc;nsdorf, 2016</xref>; <xref ref-type="bibr" rid="B75">Schito et al., 2017</xref>; <xref ref-type="bibr" rid="B74">Schito et al., 2021</xref>). The VR, T<sub>max</sub>, and D- and G-band shifts of the original and pyrolyzed samples are listed in <xref ref-type="table" rid="T3">Table 3</xref>. <xref ref-type="fig" rid="F4">Figure 4</xref> shows a strong positive relationship between VR and D&#x2012;G separation; statistical analysis shows that this is a linear relationship with R<sub>2</sub> &#x3d; 0.8901.</p>
<table-wrap id="T3" position="float">
<label>TABLE 3</label>
<caption>
<p>Results of pore size distribution in NMR analyses.</p>
</caption>
<table>
<thead valign="top">
<tr>
<th rowspan="2" align="center">Sample no.</th>
<th colspan="3" align="center">NMR pore size distribution frequency/%</th>
<th rowspan="2" align="center">VR</th>
<th rowspan="2" align="center">T<sub>max</sub>
</th>
</tr>
<tr>
<th align="center">&#x3c;10 nm</th>
<th align="center">10&#x2013;100 nm</th>
<th align="center">&#x3e;100 nm</th>
</tr>
</thead>
<tbody valign="top">
<tr>
<td align="center">Origin Samples</td>
<td align="center">62.2</td>
<td align="center">26.7</td>
<td align="center">11.1</td>
<td align="center">0.4</td>
<td align="center">434</td>
</tr>
<tr>
<td align="center">311</td>
<td align="center">66.7</td>
<td align="center">20.5</td>
<td align="center">12.8</td>
<td align="center">0.77</td>
<td align="center">446</td>
</tr>
<tr>
<td align="center">312</td>
<td align="center">63.2</td>
<td align="center">34.2</td>
<td align="center">2.6</td>
<td align="center">1.46</td>
<td align="center">455</td>
</tr>
<tr>
<td align="center">313</td>
<td align="center">65.5</td>
<td align="center">29.0</td>
<td align="center">5.5</td>
<td align="center">1.76</td>
<td align="center">467</td>
</tr>
<tr>
<td align="center">315</td>
<td align="center">72.8</td>
<td align="center">18.2</td>
<td align="center">9.0</td>
<td align="center">2.23</td>
<td align="center">605</td>
</tr>
<tr>
<td align="center">323</td>
<td align="center">64.4</td>
<td align="center">25.4</td>
<td align="center">10.2</td>
<td align="center">1.95</td>
<td align="center">474</td>
</tr>
<tr>
<td align="center">325</td>
<td align="center">76.2</td>
<td align="center">15.9</td>
<td align="center">7.9</td>
<td align="center">2.44</td>
<td align="center">607</td>
</tr>
</tbody>
</table>
</table-wrap>
<fig id="F4" position="float">
<label>FIGURE 4</label>
<caption>
<p>Relationships between VR and D&#x2012;G band separation (blue), and T<sub>max</sub> and D&#x2012;G band separation (pink).</p>
</caption>
<graphic xlink:href="feart-12-1399541-g004.tif"/>
</fig>
<p>Generally, the increasing carbon D&#x2012;G band separation as organic matter maturity increases is attributed to the D-band shifting towards lower wavenumbers, while the G-band remains largely unchanged. During the initial stages of maturation, D-band shifting increases before gradually stabilizing at the stage of over-maturity, like the trend of coal. <xref ref-type="bibr" rid="B39">Kelemen and Fang (2001)</xref> found that the metamorphic grade, like maturity, evolves faster at the catagenesis stage than at the metagenesis stage, for both natural and laboratory matured coal. Moreover, some investigators have also indicated that there is good relationship between D&#x2012;G band separation and T<sub>max</sub> values, which represents a good thermal maturity index. However, previous research has suggested that T<sub>max</sub> values may not be an appropriate parameter to quantify the thermal maturity of kerogen with high maturity (&#x2265;2.0%R<sub>o</sub>) and low S<sub>2</sub> values (<xref ref-type="bibr" rid="B47">Lewan and Kotarba, 2014</xref>; <xref ref-type="bibr" rid="B96">Wu et al., 2018</xref>). A cross-plot of T<sub>max</sub> <italic>versus</italic> band separation showed good correlation using data from pyrolyzed samples with T<sub>max</sub> ranging from 434&#xb0;C to 474 &#xb0;C. Statistical analysis also shows that there was a good linear relationship between T<sub>max</sub> and the D&#x2012;G band separation for the pyrolyzed samples with T<sub>max</sub> ranging from 434&#xb0;C to 474 &#xb0;C (<xref ref-type="fig" rid="F4">Figure 4</xref>). The band separation increases with increasing T<sub>max</sub> further indicated that the organic compounds in kerogen evolved to larger aromatic clusters and a better-ordered structure.</p>
</sec>
<sec id="s3-1-2">
<title>3.1.2 FTIR</title>
<p>The FTIR spectra of the organic-rich shales, before and after pyrolysis, had well-resolved peaks and bands, and flat baselines (<xref ref-type="fig" rid="F5">Figure 5</xref>), which indicated that the FTIR spectra were appropriate for further qualitative analysis. Generally, bands at 3,100&#x2013;3,000 cm<sup>&#x2212;1</sup> and 3,000&#x2013;2,800 cm<sup>&#x2212;1</sup> have been assigned to aromatic CH stretching vibrations and aliphatic CH stretching vibrations, respectively (<xref ref-type="bibr" rid="B50">Li et al., 2007</xref>; <xref ref-type="bibr" rid="B67">Okolo et al., 2015</xref>; <xref ref-type="bibr" rid="B11">Chen et al., 2019</xref>; <xref ref-type="bibr" rid="B13">Cincinelli et al., 2021</xref>; <xref ref-type="bibr" rid="B63">Mastalerz et al., 2021</xref>; <xref ref-type="bibr" rid="B68">Phan et al., 2021</xref>). As shown in <xref ref-type="fig" rid="F5">Figure 5</xref>, the bands at 3,100&#x2013;3,000 cm<sup>&#x2212;1</sup> and 3,000&#x2013;2,800 cm<sup>&#x2212;1</sup> were indiscernible in our pyrolyzed samples; this may indicate that these bands are not suitable for identifying the hydrocarbon potential and maturity of kerogen where there is the influence of large quantities of inorganic minerals within the source rocks.</p>
<fig id="F5" position="float">
<label>FIGURE 5</label>
<caption>
<p>FTIR spectra for the pyrolyzed samples.</p>
</caption>
<graphic xlink:href="feart-12-1399541-g005.tif"/>
</fig>
<p>The band at &#x223c;2,361 cm<sup>&#x2212;1</sup> may be assigned to adsorbed CO<sub>2</sub> and this band becomes broader and the center shifts to a lower wavenumber when <sup>18</sup>O is incorporated into CO<sub>2</sub> (<xref ref-type="bibr" rid="B52">Liao et al., 2002</xref>). The broad bands at &#x223c;2,361 and &#x223c;2,347 cm<sup>&#x2212;1</sup> are due to band overlap of adsorbed C<sup>18</sup>O<sub>2</sub>, C<sup>16</sup>O<sup>18</sup>O, and C<sup>16</sup>O<sub>2</sub> (<xref ref-type="bibr" rid="B52">Liao et al., 2002</xref>). The broad bands at &#x223c;2,361 and &#x223c;2,347 cm<sup>&#x2212;1</sup> are due to band overlap of adsorbed C<sup>18</sup>O<sub>2</sub>, C<sup>16</sup>O<sup>18</sup>O, and C<sup>16</sup>O<sub>2</sub>. Those can be confirmed in previous investigation in which &#x3b4;<sup>13</sup>C of CO<sub>2</sub> was &#x2b;0.84 to &#x2b;1.06&#x2030;, suggesting that the adsorbed CO<sub>2</sub> was mainly generated from carbonate minerals (<xref ref-type="bibr" rid="B96">Wu et al., 2018</xref>), and the inorganic CO<sub>2</sub> enrich <sup>18</sup>O, comparing with organic CO<sub>2</sub> under wet climate, low salinity environments, on the basis that the wet climate and the small mineralization of the shells of the lakes are composed of carbon and oxygen isotopes, which are lightly composed, with the climate drying, the salinity of the lake increases, and the shells are enriched with heavy carbon and oxygen isotopes (<xref ref-type="bibr" rid="B69">Ping, 1990</xref>).</p>
<p>A band at &#x223c;1,435 cm<sup>&#x2212;1</sup> was observed in the pyrolyzed samples, representing the aliphatic bending vibration due to CH<sub>2</sub> and CH<sub>3</sub>. This band exhibited more obvious absorbance in the FTIR spectra of the pyrolyzed samples with VR<sub>s</sub> lower than 1.95%R<sub>o</sub>. A shoulder was observed on the left-hand side of the 1,435 cm<sup>&#x2212;1</sup> band, at around 1,460 cm<sup>&#x2212;1</sup>. This is generally attributed to the aromatic C&#x3d;C stretching vibration (<xref ref-type="bibr" rid="B14">Coates, 2000</xref>; <xref ref-type="bibr" rid="B89">Van Niekerk et al., 2008</xref>; <xref ref-type="bibr" rid="B18">Ding et al., 2021</xref>; <xref ref-type="bibr" rid="B91">Wang et al., 2022</xref>). The intensity of this shoulder was found to be stronger for pyrolyzed samples with increased VR<sub>s</sub> from 0.77%R<sub>o</sub> to 2.44%R<sub>o</sub> and was almost higher than the 1,435 cm<sup>&#x2212;1</sup> peak for pyrolyzed samples with VR<sub>s</sub> higher than 1.95%R<sub>o</sub> (<xref ref-type="fig" rid="F5">Figure 5</xref>). The 1,435 cm<sup>&#x2212;1</sup> peak decreased with increasing maturity for VR<sub>s</sub> ranging from 0.77%R<sub>o</sub> to 2.44%R<sub>o</sub> (<xref ref-type="fig" rid="F5">Figure 5</xref>). The &#x223c;1,600 cm<sup>&#x2212;1</sup> band, assigned to stretching vibrations of aromatic rings (<xref ref-type="bibr" rid="B67">Okolo et al., 2015</xref>; <xref ref-type="bibr" rid="B68">Phan et al., 2021</xref>), became more obvious with increasing maturity for VR<sub>s</sub> ranging from 0.77%R<sub>o</sub> to 2.44%R<sub>o</sub> (<xref ref-type="fig" rid="F5">Figure 5</xref>), which was consistent with the behavior of the 1,460 cm<sup>&#x2212;1</sup> peak.</p>
<p>Spectral bands at 1,280&#x2013;1,000 cm<sup>&#x2212;1</sup> can be assigned to saturated aliphatic skeletal C&#x2012;C vibrations, C&#x2012;O stretching vibrations of ether groups, and O&#x2012;H bending vibrations in phenolic, phenoxy, and hydroxybenzene structures. These bands were also observed in the FTIR spectra of coals (<xref ref-type="bibr" rid="B14">Coates, 2000</xref>; <xref ref-type="bibr" rid="B89">Van Niekerk et al., 2008</xref>; <xref ref-type="bibr" rid="B67">Okolo et al., 2015</xref>; <xref ref-type="bibr" rid="B68">Phan et al., 2021</xref>; <xref ref-type="bibr" rid="B91">Wang et al., 2022</xref>). The band at 1,030 cm<sup>&#x2212;1</sup> observed in <xref ref-type="fig" rid="F5">Figure 5</xref> indicates the intensity of C-C stretching vibrations within an aliphatic skeleton (<xref ref-type="bibr" rid="B67">Okolo et al., 2015</xref>; <xref ref-type="bibr" rid="B36">Jing et al., 2019</xref>; <xref ref-type="bibr" rid="B71">Razavian and Fatemi, 2021</xref>; <xref ref-type="bibr" rid="B77">Shang et al., 2021</xref>). The 1,280&#x2013;1,000 cm<sup>&#x2212;1</sup> peak heights of all pyrolyzed samples showed a steady increase with increasing VR, and the narrowing peak width as VR increased indicated that some organic functional groups (such as C&#x2012;O and O&#x2012;H) were rapidly pyrolyzed and hence sharply decreased; the remaining functional groups (such as C&#x2012;C) were slowly pyrolyzed and hence showed less of a decrease.</p>
<p>The out-of-plane aromatic C&#x2012;H bending vibrations indicated the presence of substituted aromatic species in aromatic rings; and trans- and cis-CH<sub>2</sub> in long, saturated aromatic CH&#x2012;CH chains were observed in the 900&#x2013;700 cm<sup>&#x2212;1</sup> region of the spectra in the entirely pyrolyzed samples (<xref ref-type="bibr" rid="B14">Coates, 2000</xref>; <xref ref-type="bibr" rid="B89">Van Niekerk et al., 2008</xref>; <xref ref-type="bibr" rid="B61">Malumbazo et al., 2011</xref>; <xref ref-type="bibr" rid="B67">Okolo et al., 2015</xref>; <xref ref-type="bibr" rid="B36">Jing et al., 2019</xref>; <xref ref-type="bibr" rid="B77">Shang et al., 2021</xref>; <xref ref-type="bibr" rid="B93">Wang et al., 2022</xref>). The peaks in the 900&#x2013;700 cm<sup>&#x2212;1</sup> region of the spectra became more obvious with increasing VR (<xref ref-type="fig" rid="F5">Figure 5</xref>), indicating an increase in aromatic groups.</p>
</sec>
<sec id="s3-1-3">
<title>3.1.3 XRD with VR</title>
<p>In general, the brittleness and adsorption capacity of shale can be affected by its mineralogy. Hence, it is critical for shale evaluation to obtain accurate analysis of the mineral composition of the rocks. Therefore, XRD analysis was performed on the pyrolyzed samples. As can be seen in <xref ref-type="fig" rid="F6">Figure 6</xref>, calcite, albite, and quartz were identified as the main mineral components of the pyrolyzed shale. According to the standard powder diffraction cards of quartz (PDF&#x23;85-0795), calcite (PDF&#x23;72-1937), albite: Na<sub>0.98</sub>Ca<sub>0.16</sub>Al<sub>1.16</sub>Si<sub>2.84</sub>O<sub>8</sub> (PDF&#x23;70-3,752), and albite: Na<sub>0.84</sub>Ca<sub>0.02</sub>Al<sub>1.02</sub>Si<sub>2.98</sub>O<sub>8</sub> (PDF&#x23;76-0927), the peaks at 20.8&#xb0;, 26.7&#xb0;, 36.6&#xb0;, and 39.5&#xb0; were assigned to quartz; peaks at 29.5&#xb0; and 35.3&#xb0; were assigned to calcite and Na<sub>0.84</sub>Ca<sub>0.02</sub>Al<sub>1.02</sub>Si<sub>2.98</sub>O<sub>8</sub>, respectively; and peaks at 27.9&#xb0; and 30.5&#xb0; were assigned to Na<sub>0.95</sub>Ca<sub>0.16</sub>Al<sub>1.16</sub>Si<sub>2.84</sub>O<sub>8</sub> and Na<sub>0.84</sub>Ca<sub>0.02</sub> Al<sub>1.02</sub>Si<sub>2.98</sub>O<sub>8</sub>, respectively.</p>
<fig id="F6" position="float">
<label>FIGURE 6</label>
<caption>
<p>Identification of various mineral phases in pyrolyzed samples. The standard powder diffraction cards of quartz (PDF&#x23;85-0795), albite (PDF&#x23;70-3,752): Na<sub>0.98</sub>Ca<sub>0.16</sub>Al<sub>1.16</sub>Si<sub>2.84</sub>O<sub>8</sub>, albite (PDF&#x23;76-0927): Na<sub>0.84</sub>Ca<sub>0.02</sub>Al<sub>1.02</sub>Si<sub>2.98</sub>O<sub>8</sub>, and cal. (PDF&#x23;72-1937) are also presented.</p>
</caption>
<graphic xlink:href="feart-12-1399541-g006.tif"/>
</fig>
<p>Calcite is a carbonate mineral, and its peak (29.5&#xb0;) intensity dramatically decreased with increasing maturity (<xref ref-type="fig" rid="F6">Figure 6</xref>); this could be ascribed to the thermal decomposition of carbonate under hydrous pyrolysis. It is notable that the quartz peak (26.7&#xb0;) intensity decreased with increasing VR (<xref ref-type="fig" rid="F6">Figure 6</xref>), while the albite peak (27.9&#xb0;) intensity increased with increasing VR. This appears to indicate that feldspathization was enhanced with an increase in maturity. In addition, the elemental composition of albite changed with increasing VR; the 35.3&#xb0; peak assigned to Na<sub>0.84</sub>Ca<sub>0.02</sub> Al<sub>1.02</sub>Si<sub>2.98</sub>O<sub>8</sub> increased with increasing VR, indicating that Na<sub>0.95</sub>Ca<sub>0.16</sub>Al<sub>1.16</sub>Si<sub>2.84</sub>O<sub>8</sub> converted to Na<sub>0.84</sub>Ca<sub>0.02</sub> Al<sub>1.02</sub>Si<sub>2.98</sub>O<sub>8</sub> with increasing VR (<xref ref-type="fig" rid="F6">Figure 6</xref>). Thus, the XRD results suggest that carbonates were broken down, and quartz and albite (Na<sub>0.98</sub>Ca<sub>0.16</sub>Al<sub>1.16</sub>Si<sub>2.84</sub>O<sub>8</sub>) were converted to Na<sub>0.84</sub>Ca<sub>0.02</sub> Al<sub>1.02</sub>Si<sub>2.98</sub>O<sub>8</sub> as kerogen became more thermally mature. Such inorganic mineral reactions may affect the brittleness and adsorption capacity of the shales.</p>
</sec>
<sec id="s3-1-4">
<title>3.1.4 XPS</title>
<p>To quantify the binding forms of oxygen, carbon, nitrogen, aluminum, and silicon during organic matter evolution, high resolution XPS spectra of O 1s, C 1s, N 1s, Al 2p, and Si 2p were de-convoluted using Gaussian&#x2012;Lorentzian peaks (<xref ref-type="bibr" rid="B90">Wang et al., 2013</xref>; <xref ref-type="bibr" rid="B36">Jing et al., 2019</xref>; <xref ref-type="bibr" rid="B55">Liu et al., 2021</xref>; <xref ref-type="bibr" rid="B100">Wu and Xu, 2022</xref>). The XPS wide energy spectra of the original kerogen sample and the pyrolyzed samples are illustrated in <xref ref-type="fig" rid="F7">Figure 7</xref>. The original sample was found to have low oxygen (12.12%) and high carbon (82.38%) contents. After pyrolysis, the oxygen content increased to 40.15% at VR &#x3d; 1.46%R<sub>o</sub>, 52.01% at VR &#x3d; 1.95%R<sub>o</sub>, and 52.18% at VR &#x3d; 2.44%R<sub>o</sub>, accompanied by a decreasing trend in carbon content (<xref ref-type="fig" rid="F7">Figure 7A, D, G, J</xref>). The trend of a decrease in C 1s suggests that the kerogen gradually broke down and hydrocarbons were generated as VR increased. The increase in O 1s may be attributed to the oxidation of organic carbon or reactions between inorganic minerals during hydrous pyrolysis.</p>
<fig id="F7" position="float">
<label>FIGURE 7</label>
<caption>
<p>XPS wide scan data from the original kerogen <bold>(A&#x2013;C)</bold> and pyrolyzed samples <bold>(D&#x2013;L)</bold>.</p>
</caption>
<graphic xlink:href="feart-12-1399541-g007.tif"/>
</fig>
<p>The evolution of carbon content agree with that was found in the ultimate analysis, while evolution of oxygen content showed contrary tendency with that was found in the ultimate analysis of kerogen (<xref ref-type="bibr" rid="B96">Wu et al., 2018</xref>). This may indicate that the increase in oxygen content was mainly contained within inorganic material (e.g., albite and quartz) rather than organic matter (e.g., kerogen and retained petroleum). The data shown in <xref ref-type="fig" rid="F7">Figure 7</xref> directly confirmed the increase in silicon content within feldspar that occurred during feldspathization and organic matter evolution. The decrease in the 533.0 eV binding energy peak corresponding to Si&#x2012;O in quartz, and the slight decrease in the 531.5 eV binding energy peak corresponding to Al&#x2012;O in albite further confirmed the conversion of Na<sub>0.95</sub>Ca<sub>0.16</sub>Al<sub>1.16</sub>Si<sub>2.84</sub>O<sub>8</sub> to Na<sub>0.84</sub>Ca<sub>0.02</sub> Al<sub>1.02</sub>Si<sub>2.98</sub>O<sub>8</sub> (<xref ref-type="fig" rid="F6">Figure 6C,F, I, L</xref>).</p>
<p>
<xref ref-type="fig" rid="F7">Figure 7B, E, H, K</xref> shows the high resolution XPS spectra of C 1s for calcareous shale. The peak at a binding energy of 284.6 eV corresponds to C&#x2012;C or C&#x2012;H groups, while that at 285.7 eV corresponds to a C&#x2012;O group (alcohol, phenol, or ether) (<xref ref-type="bibr" rid="B5">Buckley and Lamb, 1996</xref>; <xref ref-type="bibr" rid="B27">Gong et al., 1998</xref>; <xref ref-type="bibr" rid="B36">Jing et al., 2019</xref>; <xref ref-type="bibr" rid="B56">Liu et al., 2021</xref>; <xref ref-type="bibr" rid="B100">Wu and Xu, 2022</xref>). The 288.9&#x2013;289.5 eV binding energy peaks that appeared at VRs of 1.95%R<sub>o</sub> and 2.44%R<sub>o</sub> correspond to the COOH (carboxyl) group, which may indicate that water has some oxidability to organic carbon at a high stage of thermal evolution. This is also supported by the binding energy peaks at 531.5 eV in the O 1s XPS spectra increasing at VRs of 1.46%R<sub>o</sub>, 1.95%R<sub>o</sub>, and 2.44%R<sub>o</sub> (<xref ref-type="fig" rid="F7">Figures 7I, L</xref>). This increase in O 1s may partly derive from the oxidation of organic carbon during hydrous pyrolysis.</p>
</sec>
</sec>
<sec id="s3-2">
<title>3.2 Evolution of pore structure</title>
<sec id="s3-2-1">
<title>3.2.1 SEM and SEM-EDS mapping</title>
<p>The Raman, XRD, and XPS results suggested changes in inorganic material and organic matter during hydrous pyrolysis. More information was then needed to directly demonstrate the processes of thermal decomposition of carbonates and organic matter, and conversion of Na<sub>0.95</sub>Ca<sub>0.16</sub>Al<sub>1.16</sub>Si<sub>2.84</sub>O<sub>8</sub> to Na<sub>0.84</sub>Ca<sub>0.02</sub>Al<sub>1.02</sub>Si<sub>2.98</sub>O<sub>8</sub>. As shown in <xref ref-type="fig" rid="F8">Figure 8</xref>, the morphology and pore structure of inorganic and organic matter in the original samples and pyrolyzed residues were fully characterized using SEM imaging and SEM-EDS analysis.</p>
<fig id="F8" position="float">
<label>FIGURE 8</label>
<caption>
<p>SEM images and SEM-EDS elemental maps showing the morphology and chemistry of inorganic minerals and organic matter. Organic matter (1, 3) and pyrite (2) in the original sample <bold>(A)</bold>. Elemental maps of C <bold>(B)</bold>, Fe <bold>(C)</bold>, and S <bold>(D)</bold> within the organic matter and pyrite. Feldspar in the original sample <bold>(E)</bold>. Elemental maps of Si <bold>(F)</bold>, O <bold>(G)</bold>, and Al <bold>(H)</bold> within feldspar. Carbonate before <bold>(I)</bold> and after <bold>(J)</bold> pyrolysis at VR&#x3d;1.5. Morphology of pores in feldspar <bold>(K)</bold> and organic matter <bold>(L)</bold> after pyrolysis at VR&#x3d;1.5.</p>
</caption>
<graphic xlink:href="feart-12-1399541-g008.tif"/>
</fig>
<p>In the original samples, organic matter and inorganic minerals were observed in SEM images, and C, Fe, and S were also detected by SEM-EDS (<xref ref-type="fig" rid="F8">Figures 8A&#x2013;D</xref>). The EDS map of carbon distribution (<xref ref-type="fig" rid="F8">Figure 8B</xref>) indicates that the features labeled 1 and 3 in <xref ref-type="fig" rid="F8">Figure 8A</xref> are organic matter. The distributions of Fe and S correspond with each other (<xref ref-type="fig" rid="F8">Figures 8C, D</xref>), which suggests that the feature labeled 2 in <xref ref-type="fig" rid="F8">Figure 8A</xref> is pyrite, a mineral associated with a favorable reduction environment for oil-prone organic matter. The elements Si, O, and Al have distributions that correspond with one another (<xref ref-type="fig" rid="F8">Figures 8F&#x2013;H</xref>), suggesting that the mineral shown in <xref ref-type="fig" rid="F8">Figure 8E</xref> is feldspar. The results of XRD analysis further indicate that this is albite (<xref ref-type="fig" rid="F6">Figure 6</xref>). Carbonate can also be observed in SEM images (<xref ref-type="fig" rid="F8">Figure 8I</xref>).</p>
<p>After hydrous pyrolysis, decomposition of carbonates was observed in SEM images; fractures formed on the surface of the carbonates, some of which broke down into similar layered blocks (<xref ref-type="fig" rid="F8">Figure 8J</xref>). Many pores also formed on the surface of albite, which may have developed during the transformation of Na<sub>0.95</sub>Ca<sub>0.16</sub>Al<sub>1.16</sub>Si<sub>2.84</sub>O<sub>8</sub> to Na<sub>0.84</sub>Ca<sub>0.02</sub>Al<sub>1.02</sub>Si<sub>2.98</sub>O<sub>8</sub> (<xref ref-type="fig" rid="F6">Figure 6</xref>; <xref ref-type="fig" rid="F9">Figure 9K</xref>). Pore sizes ranged from 1.505 to 3.430 &#x3bc;m (<xref ref-type="fig" rid="F8">Figure 8K</xref>). These pores may be the result of the leaching of Ca<sup>2&#x2b;</sup> and Al<sup>3&#x2b;</sup> during the transformation of albite. More pores developed around organic matter, and these had a size range of 8.412&#x2013;13.970 &#x3bc;m (<xref ref-type="fig" rid="F8">Figure 8L</xref>). Similar pores were also observed on the surface of high-rank coals (<xref ref-type="bibr" rid="B116">Zheng et al., 2019</xref>; <xref ref-type="bibr" rid="B110">Zhang et al., 2021</xref>). Organic matter was also decomposed into many porous pieces by pyrolysis (<xref ref-type="fig" rid="F8">Figure 8L</xref>).</p>
<fig id="F9" position="float">
<label>FIGURE 9</label>
<caption>
<p>Nitrogen adsorption isotherms for the unheated sample <bold>(A)</bold> and pyrolyzed samples <bold>(B&#x2013;J)</bold> with different VRs.</p>
</caption>
<graphic xlink:href="feart-12-1399541-g009.tif"/>
</fig>
<p>According to the changes in mineral composition observed using XRD and SEM, the main reason for the change in porosity of inorganic minerals caused by temperature and pressure appears to be the dissolution of soluble minerals, such as plagioclase, and the fragmentation of refractory minerals, such as quartz. Owing to the influence of high temperature, the strength of quartz and other relatively strong particles will be reduced, so that they become more easily broken. With a rise in temperature, cracks gradually increase, and mineral particles gradually become broken. In addition, as temperature increases, feldspar and other easily plastically deformed minerals will not only dissolve, but also be transformed (e.g., into kaolinite). Some investigators have shown that the conversion of feldspar into clay minerals could markedly reduce the volume of feldspar and increase porosity (<xref ref-type="bibr" rid="B94">Worden and Morad, 1999</xref>; <xref ref-type="bibr" rid="B108">Yang et al., 2020</xref>; <xref ref-type="bibr" rid="B83">Sun et al., 2021</xref>). In the process of dissolution and deformation, minerals will be affected by compaction, resulting in closer particle contact and smaller pores. However, the sample pores are filled with high-pressure fluid, which counteracts much of the overlying rock pressure and inhibits compaction, thus protecting the existing and newly generated pores.</p>
</sec>
<sec id="s3-2-2">
<title>3.2.2 BET</title>
<p>SEM images show the micropores that directly reflect the changes in organic matter and inorganic minerals, and store free shale gas (<xref ref-type="bibr" rid="B35">Ji et al., 2017</xref>). However, some investigations have suggested that adsorbed gas, the main gas component of shales, is mostly stored in nano-pores (<xref ref-type="bibr" rid="B35">Ji et al., 2017</xref>; <xref ref-type="bibr" rid="B64">Memon et al., 2021</xref>; <xref ref-type="bibr" rid="B119">Zhu et al., 2021</xref>; <xref ref-type="bibr" rid="B118">Zhou et al., 2022</xref>). To analyze the nanoporous structure and surface chemistry of the origin samples and pyrolyzed residues, the BET isotherm measurements are carried out. The nitrogen isotherms at different VR are presented in <xref ref-type="fig" rid="F9">Figure 9</xref>. The appearance of hysteresis loops appeared for the different capillary condensation and capillary evaporation under the same pressure (<xref ref-type="bibr" rid="B44">Kruk and Jaroniec, 2001</xref>; <xref ref-type="bibr" rid="B84">Sun et al., 2015</xref>; <xref ref-type="bibr" rid="B70">Qiu et al., 2021</xref>). Generally, the greater the separation between the desorption and adsorption isotherms the larger the pore content, under the same pressure (<xref ref-type="bibr" rid="B22">Fan et al., 2002</xref>; <xref ref-type="bibr" rid="B93">Wang et al., 2022</xref>). However, the degree of separation between the desorption and adsorption isotherms showed no obvious change in our pyrolyzed residues with increasing VR (<xref ref-type="fig" rid="F9">Figure 9</xref>). As the VR increased, the quantity of adsorbed nitrogen gradually increased, compared with the unheated sample; the quantities adsorbed were 14.32, 21.70, 23.39, 25.84, 30.42, 30.89, 34.94, 35.47, 38.73, and 43.14 cm<sup>3</sup>/g for the unheated sample and the pyrolyzed samples with VRs of 0.77%R<sub>o</sub>, 0.81%R<sub>o</sub>, 1.16%R<sub>o</sub>, 1.76%R<sub>o</sub>, 1.95%R<sub>o</sub>, 2.14%R<sub>o</sub>, 2.23%R<sub>o</sub>, 2.29%R<sub>o</sub>, and 2.44%R<sub>o</sub>, respectively (<xref ref-type="fig" rid="F8">Figure 8</xref>). There was a good relationship between the nitrogen quantity adsorbed and the VR, with a correlation coefficient (R<sup>2</sup>) of 0.93 (<xref ref-type="fig" rid="F10">Figure 10</xref>). The cumulative BET surface areas also had a good correlation with VR, with an R<sup>2</sup> of 0.86 (<xref ref-type="fig" rid="F10">Figure 10</xref>). This may suggest that the maturation of organic matter plays a positive role in the development of pores in shales. High pore content is helpful to enhance the self-storage capacity of shale gas. This is a possible reason why highly gas-productive shale is generally also highly mature shale.</p>
<fig id="F10" position="float">
<label>FIGURE 10</label>
<caption>
<p>Relationships between VR and nitrogen quantity adsorbed (black), and between VR and BET surface area (red).</p>
</caption>
<graphic xlink:href="feart-12-1399541-g010.tif"/>
</fig>
<p>The pore size distributions of unheated and pyrolyzed samples are presented in <xref ref-type="fig" rid="F11">Figure 11</xref>. In these samples, the pore sizes were distributed across two main size intervals of 4&#x2013;30 nm and 30&#x2013;100 nm, which can be generalized as mesopores (pore diameter: 2&#x2013;50 nm) and macropores (pore diameter: &#x3e;50 nm), respectively (<xref ref-type="fig" rid="F11">Figure 11</xref>). The surface area of the unheated sample was relatively low, and the pores were mainly mesopores with 4&#x2013;30 nm diameters (<xref ref-type="fig" rid="F11">Figure 11</xref>). The pore volume of mesopores gradually increased with an increase in VR from 0.77%R<sub>o</sub> to 1.76%R<sub>o</sub> (<xref ref-type="fig" rid="F11">Figure 11</xref>). This increase in mesopores may be a response to peak hydrocarbon generation, which appears at a VR of 1.5%R<sub>o</sub> (<xref ref-type="bibr" rid="B96">Wu et al., 2018a</xref>). At VRs beyond 1.76%R<sub>o</sub>, there was no obvious further increase in the pore volume of mesopores; instead, there were merely small fluctuations (<xref ref-type="fig" rid="F11">Figure 11</xref>). For the macropores, pore volume gradually increased with an increase in VR from 0.77%R<sub>o</sub> to 2.44%R<sub>o</sub> (<xref ref-type="fig" rid="F11">Figure 11</xref>). We suspect that these macropores are related to the decomposition of inorganic minerals during the pyrolysis experiments because they increased with increasing thermal maturity.</p>
<fig id="F11" position="float">
<label>FIGURE 11</label>
<caption>
<p>The distributions of the pore volume at different VR.</p>
</caption>
<graphic xlink:href="feart-12-1399541-g011.tif"/>
</fig>
<p>The changes in pore volume and surface area show that there were two evolutionary stages in the hydrous pyrolysis of the calcareous shale: 1) a rapid increase stage coinciding with the hydrocarbon generation peak; and 2) a relatively stable stage after the hydrocarbon generation peak. The results show that pore structure evolution in the calcareous shale resulted from two different pore type behaviors: the pore volume and surface area of pores over 30 nm increased gradually, while the volume of pores under 30 nm firstly increased and then continuously decreased after the hydrocarbon generation peak.</p>
</sec>
<sec id="s3-2-3">
<title>3.2.3 NMR T<sub>2</sub> distribution</title>
<p>Nuclear magnetic resonance is an effective method to characterize the pore size distribution (PSD) of source rocks in a non-destructive manner (<xref ref-type="bibr" rid="B103">Xin et al., 2019</xref>; <xref ref-type="bibr" rid="B116">Zheng et al., 2019</xref>; <xref ref-type="bibr" rid="B66">Nie et al., 2021</xref>; <xref ref-type="bibr" rid="B60">Ma et al., 2022</xref>). The transverse relaxation time (T<sub>2</sub>) and pore size (r) are related by r &#x3d; C&#x2a;T<sub>2</sub>, in which C is a constant (&#x3bc;m/ms). Therefore, the T<sub>2</sub> measured by NMR can directly reflect the pore size distribution of rock samples, and a higher T<sub>2</sub> value corresponds to a larger pore radius (<xref ref-type="bibr" rid="B104">Xu et al., 2018</xref>; <xref ref-type="bibr" rid="B65">Meng et al., 2021</xref>). In addition, the connectivity among pores can also be obtained using NMR.</p>
<p>
<xref ref-type="fig" rid="F12">Figure 12</xref> presents the NMR analysis results from the calcareous shale, before and after pyrolysis. Overall, NMR peaks occurred at approximately 1, 10&#x2013;100, and 100&#x2013;1,000 ms, which indicated that mesopores and micropores in both the calcareous shale and the pyrolyzed samples were more developed (<xref ref-type="fig" rid="F12">Figure 12</xref>). This result is consistent with previous investigations, such as <xref ref-type="bibr" rid="B116">Zheng et al. (2019)</xref> and <xref ref-type="bibr" rid="B103">Xin et al. (2019)</xref>. The T<sub>2</sub> distribution of the original calcareous shale showed a trimodal distribution, with the left-hand peak being the highest, indicating a high micropore content and low content of medium&#x2012;large pores before the pyrolysis experiment (<xref ref-type="fig" rid="F12">Figure 12</xref>). After pyrolysis, the peak height of the micropores increased, while that of the macropores decreased, and all three peaks gradually shifted to the left, representing an increase in micropores and a decrease in macropores (<xref ref-type="bibr" rid="B103">Xin et al., 2019</xref>). These changes may be due to the disappearance of primary pores and the further development of secondary pores and fractures. In subsequent experiments, with an increase in VR, the shape of the T<sub>2</sub> spectrum did not change, but the peak height of the main peak kept rising, which confirmed the development of secondary pores and fractures.</p>
<fig id="F12" position="float">
<label>FIGURE 12</label>
<caption>
<p>NMR T<sub>2</sub> distributions of calcareous shale and pyrolyzed samples.</p>
</caption>
<graphic xlink:href="feart-12-1399541-g012.tif"/>
</fig>
<p>In addition, the contribution percentages of pore sizes of different scales as VR increased were analyzed and are presented in <xref ref-type="fig" rid="F14">Figure 14</xref>. The peaks at 10&#x2013;100 ms almost vanished, which suggested that transition pores sharply reduced when VR increased from 0.40%R<sub>o</sub> to 0.77%R<sub>o</sub> (<xref ref-type="fig" rid="F13">Figures 13</xref>, <xref ref-type="fig" rid="F14">14</xref>). The highest yields of bitumen (22.6 mg/g TOC; <xref ref-type="bibr" rid="B98">Wu et al., 2018</xref>) occur in this %R<sub>o</sub> range, which may indicate that the formation of a large quantity of bitumen blocked some micropores, and most of the transition pores and mesopores, ultimately resulting in low pore connectivity as VR increased from 0.40%R<sub>o</sub> to 0.77%R<sub>o</sub>. The peaks at 10&#x2013;100 ms reached a maximum at a VR level of 1.46%R<sub>o</sub> (<xref ref-type="fig" rid="F13">Figures 13</xref>, <xref ref-type="fig" rid="F14">14</xref>), indicating that a large quantity of transition pores was generated at this stage. Low bitumen yields (10.0 mg/g TOC) and high oil yields (96.8 mg/g TOC) suggest that bitumen was further pyrolyzed into liquid hydrocarbons with lower molecular weight and viscosity with this increase in maturity (<xref ref-type="bibr" rid="B96">Wu et al., 2018</xref>); here, transition pores and mesopores were flushed by hydrocarbon expulsion, which markedly improved pore connectivity. This process continued until the oil yield peak at a VR of 1.95%R<sub>o</sub> (<xref ref-type="fig" rid="F13">Figures 13</xref>, <xref ref-type="fig" rid="F14">14</xref>). As maturity increased, the oil began to crack, which resulted in an increase in micropores. Higher maturity and deeper burial may result in the collapse of transition pores and mesopores, and reduced pore connectivity (<xref ref-type="bibr" rid="B19">Dong and Harris, 2020</xref>; <xref ref-type="bibr" rid="B111">Zhang et al., 2020</xref>; <xref ref-type="bibr" rid="B55">Liu et al., 2021</xref>). ; pore collapse may also be triggered by tectonic deformation (<xref ref-type="bibr" rid="B54">Liu et al., 2020</xref>). This process may provide a better shale oil and gas preservation condition.</p>
<fig id="F13" position="float">
<label>FIGURE 13</label>
<caption>
<p>Contribution percentages of pore sizes of different scales in relation to increasing VR.</p>
</caption>
<graphic xlink:href="feart-12-1399541-g013.tif"/>
</fig>
<fig id="F14" position="float">
<label>FIGURE 14</label>
<caption>
<p>Maturity, hydrocarbon generation, and pore evolution of calcareous shale during pyrolysis experiments. The evolution of hydrocarbon generation is based on <xref ref-type="bibr" rid="B96">Wu et al. (2018)</xref>.</p>
</caption>
<graphic xlink:href="feart-12-1399541-g014.tif"/>
</fig>
<p>The variation in pore size distribution of rock samples shows that the primary pores of rocks will gradually decrease with an increase in burial depth. On the other hand, owing to hydrocarbon generation and oil cracking, organic matter is pyrolyzed, minerals are corroded by organic acids generated during hydrocarbon generation, and secondary pores are constantly generated. The results of pore evolution characterized by NMR were essentially consistent with the geological conditions.</p>
</sec>
<sec id="s3-2-4">
<title>3.2.4 Evolution of hydrocarbon generation and pore structure</title>
<p>Thermal maturity has a marked impact on hydrocarbon generation (<xref ref-type="bibr" rid="B126">Tissot and Welt, 1984</xref>; <xref ref-type="bibr" rid="B121">Hunt, 1996</xref>; <xref ref-type="bibr" rid="B49">Li et al., 2022</xref>; <xref ref-type="bibr" rid="B78">Shao et al., 2022</xref>) and pore development (<xref ref-type="bibr" rid="B84">Sun et al., 2015</xref>; <xref ref-type="bibr" rid="B85">Sun et al., 2018</xref>; <xref ref-type="bibr" rid="B80">Song et al., 2019</xref>; <xref ref-type="bibr" rid="B24">Gao et al., 2021</xref>; <xref ref-type="bibr" rid="B106">Xu et al., 2021</xref>). Pore connectivity, pore size distribution, and pore volume are important for the methane adsorption performance of shale (<xref ref-type="bibr" rid="B37">Karacan et al., 2007</xref>; <xref ref-type="bibr" rid="B120">Zou et al., 2015</xref>; <xref ref-type="bibr" rid="B104">Xu et al., 2018</xref>; <xref ref-type="bibr" rid="B41">Kong et al., 2021</xref>). Previous investigations have reported that the formation and development of pore structure is closely related to hydrocarbon generation (<xref ref-type="bibr" rid="B84">Sun et al., 2015</xref>; <xref ref-type="bibr" rid="B24">Gao et al., 2021</xref>; <xref ref-type="bibr" rid="B106">Xu et al., 2021</xref>). Hence, the evolution of hydrocarbon generation and pore structure corresponding to different VR levels were analyzed; this is illustrated in <xref ref-type="fig" rid="F14">Figure 14</xref>.</p>
<p>With an increase in burial depth and thermal maturity, the evolution of hydrocarbon generation from organic matter mainly follows a pathway from bitumen generation to liquid hydrocarbon generation, and then to gaseous hydrocarbon generation, according to the classical theory of hydrocarbon generation from organic matter (<xref ref-type="bibr" rid="B126">Tissot and Welt, 1984</xref>; <xref ref-type="bibr" rid="B121">Hunt, 1996</xref>; <xref ref-type="bibr" rid="B45">Lewan, 1997</xref>; <xref ref-type="bibr" rid="B33">Hill et al., 2003</xref>; <xref ref-type="bibr" rid="B88">Uguna et al., 2016</xref>). The yields of bitumen, oil, and hydrocarbon gas indicated that the calcareous shale experienced the above stages at VRs from 0.40%R<sub>o</sub> to 2.44%R<sub>o</sub>, under hydrous pyrolysis, and the yields of oil and gaseous hydrocarbons showed a good quadratic function relationship with VR values (<xref ref-type="fig" rid="F14">Figure 14</xref>; <xref ref-type="bibr" rid="B96">Wu et al., 2018</xref>). The peak oil yield occurred at a VR of 1.46%R<sub>o</sub> to 1.95%R<sub>o</sub>. Gaseous hydrocarbon generation increased markedly between 0.5%R<sub>o</sub> and 2.0%R<sub>o</sub>, and then stabilized (<xref ref-type="fig" rid="F14">Figure 14</xref>; <xref ref-type="bibr" rid="B96">Wu et al., 2018</xref>).</p>
<p>Because of the pyrolysis reactions that occurred during the generation of hydrocarbons, the products had different chemical compositions and physical properties. The bitumen mainly consisted of macromolecular hydrocarbons and heteroatomic functional groups, and thus had high viscosity; oil had better fluidity due to it containing a high proportion of saturated hydrocarbons; gaseous hydrocarbons had the best diffusion ability and provided the largest contribution to pressure increase during pyrolysis for the gas phase. The transformations of kerogen to bitumen, bitumen to oil, and oil to gaseous hydrocarbons with increasing maturity determined the compositions and properties of the hydrocarbons, and markedly affected the evolution of pore structure. The good linear relationships between the nitrogen quantity adsorbed, BET surface area, and the VR indicated that the surface area and pore volume of shale increased with the prolongation of hydrocarbon generation (<xref ref-type="fig" rid="F10">Figure 10</xref>). However, the distributions of the pore volume in BET and NMR at different VRs further suggested that mesopores, transition pores, and micropores in calcareous shale had different evolutionary trends during prolonged hydrocarbon generation (<xref ref-type="fig" rid="F13">Figures 13</xref>, <xref ref-type="fig" rid="F14">14</xref>).</p>
<p>The highest yields of bitumen corresponded to the lowest mesopore and transition pore volumes, suggesting that some micropores and most of the transition pores and mesopores were plugged by the high-viscosity bitumen, ultimately resulting in poor pore connectivity. Then, mesopores, transition pores, and micropores increased gradually with a decrease in average pore size. This may indicate that the bitumen pyrolyzed into oil that had better fluidity, flushing the mesopores and transition pores; further pyrolysis of organic matter generated more pores and resulted in better pore connectivity. The pores observed on the surface of feldspar and organic matter in SEM images further confirmed the development of pores through organic matter pyrolysis and through the dissolution of feldspar induced by organic acids that formed during the pyrolysis of organic matter (<xref ref-type="fig" rid="F8">Figures 8I, K</xref>). Oil cracking to gaseous hydrocarbons resulted in an increase in micropores, and poor pore connectivity due to the collapse of transition pores and mesopores under prolonged hydrocarbon generation.</p>
</sec>
</sec>
<sec id="s3-3">
<title>3.3 Geological implications</title>
<p>Organic matter and mineral properties are the main factors determining the pore characteristics of shale because the development of secondary porosity corresponds to hydrocarbon generation and the transformation/dissolution of minerals (<xref ref-type="bibr" rid="B35">Ji et al., 2017</xref>; <xref ref-type="bibr" rid="B95">Wu H. et al., 2021</xref>). Generally, the pore structures of shales have been determined by the total organic carbon content (TOC), type of organic matter, mineral composition, and thermal maturity (<xref ref-type="bibr" rid="B35">Ji et al., 2017</xref>; <xref ref-type="bibr" rid="B92">Wang et al., 2021</xref>; <xref ref-type="bibr" rid="B106">Xu et al., 2021</xref>; <xref ref-type="bibr" rid="B29">Guan et al., 2022</xref>). Among them, thermal maturity has been most widely used (<xref ref-type="bibr" rid="B51">Liang et al., 2014</xref>; <xref ref-type="bibr" rid="B84">Sun et al., 2015</xref>; <xref ref-type="bibr" rid="B24">Gao et al., 2021</xref>; <xref ref-type="bibr" rid="B106">Xu et al., 2021</xref>), because pores induced by the generation of hydrocarbons are the main contributors to secondary porosity in shale. Hence, highly productive shale gas has been strongly associated with high-maturity shales (<xref ref-type="bibr" rid="B9">Chatellier et al., 2011</xref>; <xref ref-type="bibr" rid="B31">Hao and Zou, 2013</xref>; <xref ref-type="bibr" rid="B42">Kotarba and Lewan, 2013</xref>; <xref ref-type="bibr" rid="B35">Ji et al., 2017</xref>; <xref ref-type="bibr" rid="B99">Wu et al., 2019</xref>; <xref ref-type="bibr" rid="B10">Chen et al., 2020</xref>; <xref ref-type="bibr" rid="B82">Song et al., 2021</xref>; <xref ref-type="bibr" rid="B117">Zheng et al., 2021</xref>; <xref ref-type="bibr" rid="B6">Cao et al., 2022</xref>). Rapid and effective characterization of maturity is important for shale gas exploration. Vitrinite reflectance is commonly used to characterize the maturity of organic matter. However, owing to differences in origin, some types of organic matter are amorphous and lack vitrinite, for example, the shales of the Wufeng-Longmaxi Formation (<xref ref-type="bibr" rid="B11">Chen et al., 2019</xref>). Such types of organic matter may not be suitable for VR analysis. Whole-rock FTIR, Raman, XRD, XPS, SEM, BET, SEM, and NMR results can provide thermal and pore evolution information, which is useful for understanding the association of pore development with hydrocarbon generation in shale. The evolution of pore structure can be divided into three stages: i) primary pores are filled by high-viscosity bitumen, resulting in poor pore connectivity; ii) development of secondary porosity corresponding to oil generation, with mineral dissolution induced by organic acids also providing some contribution to the generation of secondary pores; iii) further development of secondary porosity at the micropore scale, accompanied by the collapse of transition pores and mesopores, resulting in poor pore connectivity and an improved shale oil and gas preservation condition.</p>
</sec>
</sec>
<sec sec-type="conclusion" id="s4">
<title>4 Conclusion</title>
<p>To interpret the evolution of thermal maturity and pore structure of continental organic-rich shales and understand the interaction between organic matter and minerals during thermal evolution, calcareous shale (before and after pyrolysis) was analyzed using Raman, FTIR, XRD, XPS, SEM, BET, and NMR. The DA, SR, SP, DT, and ER of VR, Raman G&#x2012;D band separation, Raman I<sub>D</sub>/I<sub>G</sub>, T<sub>max</sub>, FTIR, and XPS were also estimated to develop and evaluate a comprehensive new set of maturity indicators. The results indicated that the Raman G&#x2012;D band separation and I<sub>D</sub>/I<sub>G</sub> ratio, with good DA, low SR, low SP, and short DT, correlated well with VR and T<sub>max</sub> in the pyrolyzed samples. This may indicate that Raman analysis provides good thermal maturity indicators. Vitrinite reflectance and T<sub>max</sub> may be less widely applicable given their moderate SR, complex SP, and long DT. The FTIR and XPS techniques also provided semi-quantitative maturity indicators but had poor DA and high ER. Moreover, SEM allowed direct observation of pore formation accompanying the pyrolysis of organic matter, together with changes in minerals, such as the transformation of Na<sub>0.95</sub>Ca<sub>0.16</sub>Al<sub>1.16</sub>Si<sub>2.84</sub>O<sub>8</sub> to Na<sub>0.84</sub>Ca<sub>0.02</sub>Al<sub>1.02</sub>Si<sub>2.98</sub>O<sub>8</sub>, which was confirmed by XRD. The results of BET and NMR further suggested that three stages may exist in the evolution of pore structure, in which secondary porosity developed after primary pores were filled by bitumen generation, then this secondary porosity further developed during oil-cracking. The poor pore connectivity observed at both low and high VR values may be more conducive to the preservation of shale oil and gas. This work is significant for research into the interactions between organic matter and minerals during the thermal evolution of continental shales.</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/supplementary material, further inquiries can be directed to the corresponding author.</p>
</sec>
<sec id="s6">
<title>Author contributions</title>
<p>YL: Conceptualization, Writing&#x2013;review and editing, Project administration. YW: Methodology, Writing&#x2013;original draft. RZ: Data curation, Investigation, Writing&#x2013;review and editing. SJ: Methodology, Supervision, Writing&#x2013;review and editing. XD: Validation, Writing&#x2013;review and editing.</p>
</sec>
<sec sec-type="funding-information" id="s7">
<title>Funding</title>
<p>The author(s) declare that financial support was received for the research, authorship, and/or publication of this article. This research was supported by Shenzhen Science and Technology Program (Grant Number: KCXST20221021111607018) and Science and Technology Innovation for Youth of Longdong University (Grant Number: XYZK2302).</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>
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