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  <Article>
    <Journal>
      <PublisherName>American Geophysical Union (AGU)</PublisherName>
      <JournalTitle>Acta Medica Okayama</JournalTitle>
      <Issn>0094-8276</Issn>
      <Volume>52</Volume>
      <Issue>14</Issue>
      <PubDate PubStatus="ppublish">
        <Year>2025</Year>
        <Month/>
      </PubDate>
    </Journal>
    <ArticleTitle>Unraveling the Complex Features of the Seismic Scatterers in the Mid‐Lower Mantle Through Phase Transition of (Al, H)‐Bearing Stishovite</ArticleTitle>
    <FirstPage LZero="delete">e2024GL114146</FirstPage>
    <LastPage/>
    <Language>EN</Language>
    <AuthorList>
      <Author>
        <FirstName EmptyYN="N">Yingxin</FirstName>
        <LastName>Yu</LastName>
        <Affiliation>Deep Space Exploration Laboratory, School of Earth and Space Sciences, University of Science and Technology of China</Affiliation>
      </Author>
      <Author>
        <FirstName EmptyYN="N">Youyue</FirstName>
        <LastName>Zhang</LastName>
        <Affiliation>Institute for Planetary Materials, Okayama University</Affiliation>
      </Author>
      <Author>
        <FirstName EmptyYN="N">Luo</FirstName>
        <LastName>Li</LastName>
        <Affiliation>Deep Space Exploration Laboratory, School of Earth and Space Sciences, University of Science and Technology of China</Affiliation>
      </Author>
      <Author>
        <FirstName EmptyYN="N">Xinyue</FirstName>
        <LastName>Zhang</LastName>
        <Affiliation>Deep Space Exploration Laboratory, School of Earth and Space Sciences, University of Science and Technology of China</Affiliation>
      </Author>
      <Author>
        <FirstName EmptyYN="N">Denglei</FirstName>
        <LastName>Wang</LastName>
        <Affiliation>Deep Space Exploration Laboratory, School of Earth and Space Sciences, University of Science and Technology of China</Affiliation>
      </Author>
      <Author>
        <FirstName EmptyYN="N">Zhu</FirstName>
        <LastName>Mao</LastName>
        <Affiliation>Deep Space Exploration Laboratory, School of Earth and Space Sciences, University of Science and Technology of China</Affiliation>
      </Author>
      <Author>
        <FirstName EmptyYN="N">Ningyu</FirstName>
        <LastName>Sun</LastName>
        <Affiliation>Deep Space Exploration Laboratory, School of Earth and Space Sciences, University of Science and Technology of China</Affiliation>
      </Author>
      <Author>
        <FirstName EmptyYN="N">Yanyao</FirstName>
        <LastName>Zhang</LastName>
        <Affiliation>Earth and Planetary Sciences, Stanford University</Affiliation>
      </Author>
      <Author>
        <FirstName EmptyYN="N">Xinyang</FirstName>
        <LastName>Li</LastName>
        <Affiliation>State Key Laboratory of High Pressure and Superhard Materials, College of Physics, Jilin University</Affiliation>
      </Author>
      <Author>
        <FirstName EmptyYN="N">Wancai</FirstName>
        <LastName>Li</LastName>
        <Affiliation>CAS Key Laboratory of Crust‐Mantle Materials and Environments, School of Earth and Space Sciences, University of Science and Technology of China</Affiliation>
      </Author>
      <Author>
        <FirstName EmptyYN="N">Sergio</FirstName>
        <LastName>Speziale</LastName>
        <Affiliation>GFZ German Research Centre for Geosciences</Affiliation>
      </Author>
      <Author>
        <FirstName EmptyYN="N">Dongzhou</FirstName>
        <LastName>Zhang</LastName>
        <Affiliation>GeoSoilEnviroCARS, University of Chicago</Affiliation>
      </Author>
      <Author>
        <FirstName EmptyYN="N">Jung‐Fu</FirstName>
        <LastName>Lin</LastName>
        <Affiliation>Department of Earth and Planetary Sciences, Jackson School of Geosciences, The University of Texas at Austin</Affiliation>
      </Author>
      <Author>
        <FirstName EmptyYN="N">Takashi</FirstName>
        <LastName>Yoshino</LastName>
        <Affiliation>Institute for Planetary Materials, Okayama University</Affiliation>
      </Author>
    </AuthorList>
    <PublicationType/>
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      <ArticleId IdType="doi"/>
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    <Abstract>Small-scale scatterers observed in the mid-lower mantle beneath the subduction zones are thought to result from the phase transition of stishovite within subducted oceanic crusts. Here we investigate the phase transition of (Al, H)-bearing stishovite with four compositions at simultaneously high P-T conditions combining Raman spectroscopy and X-ray diffraction. These experimental results reveal that the incorporation of 0.01 a.p.f.u Al into stishovite with H/Al ratio of ∼1/3 lowers the transition pressure by 6.7(3) GPa. However, the Clapeyron slope of this transition is nearly unaffected by changes in the Al content and has a value of 12.2–12.5(3) MPa/K. According to our results, Al content variation ranging from 0 to 0.07 a.p.f.u in SiO2 can reasonably explain the depth distribution from 800 to 1,900 km of the seismic scatterers observed in the circum-Pacific region. These results deepen our understanding on the complex features of mid-lower mantle seismic scatterers and corresponding dynamic processes.</Abstract>
    <CoiStatement>No potential conflict of interest relevant to this article was reported.</CoiStatement>
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        <Param Name="value">phase transition</Param>
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        <Param Name="value">mid-lower mantle</Param>
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        <Param Name="value">small-scale seismic scatterers</Param>
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  </Article>
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