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        <datestamp>2026-09-29T13:25:46Z</datestamp>
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          <dc:title>Helium Trapping in Mg–Silicates at Multi-Megabar Pressures</dc:title>
          <dc:creator>Kang Yang (25137222)</dc:creator>
          <dc:subject>Structural properties of condensed matter</dc:subject>
          <dc:subject>high pressure physics</dc:subject>
          <dc:subject>Helium-bearing Mg-Silicates</dc:subject>
          <dc:subject>Machine learning potential</dc:subject>
          <dc:subject>Structural Properties</dc:subject>
          <dc:description>&lt;p dir="ltr"&gt;Helium retention under extreme compression is widely discussed, yet the microscopic&lt;/p&gt;&lt;p dir="ltr"&gt;host phases and stabilization mechanisms remain unsettled. Mg-Si-O minerals form&lt;/p&gt;&lt;p dir="ltr"&gt;the dominant condensed framework of rocky interiors across broad pressuretemperature&lt;/p&gt;&lt;p dir="ltr"&gt;conditions and throughout planetary evolution, making Mg–silicates the&lt;/p&gt;&lt;p dir="ltr"&gt;most relevant (and stringent) minerals in which to assess helium incorporation.&lt;/p&gt;&lt;p dir="ltr"&gt;Meanwhile rare study focuses on the high-pressure behavior between Helium and&lt;/p&gt;&lt;p dir="ltr"&gt;Mg-Silicates.&lt;/p&gt;&lt;p dir="ltr"&gt;Here, we explore the ternary MgO-SiO2-He system and identify two&lt;/p&gt;&lt;p dir="ltr"&gt;thermodynamically stable helium-bearing Mg silicates, Mg2SiO4He and Mg2SiO4He2,&lt;/p&gt;&lt;p dir="ltr"&gt;over 250–930 GPa. We reveal a clear microscopic mechanism: pressure-driven&lt;/p&gt;&lt;p dir="ltr"&gt;reorganization of post-perovskite-derived Mg-Si-O frameworks create interstitial&lt;/p&gt;&lt;p dir="ltr"&gt;cavities that confine helium without chemical bonding.&lt;/p&gt;</dc:description>
          <dc:date>2026-09-29T13:25:46Z</dc:date>
          <dc:type>Text</dc:type>
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          <dc:identifier>10.6084/m9.figshare.34023954.v1</dc:identifier>
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          <dc:rights>CC BY 4.0</dc:rights>
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