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<titleInfo><title>Thermodynamics of diamond formation from hydrocarbon mixtures in planets</title></titleInfo>


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<name type="personal">
  <namePart type="given">Bingqing</namePart>
  <namePart type="family">Cheng</namePart>
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<name type="personal">
  <namePart type="given">Sebastien</namePart>
  <namePart type="family">Hamel</namePart>
  <role><roleTerm type="text">author</roleTerm> </role></name>
<name type="personal">
  <namePart type="given">Mandy</namePart>
  <namePart type="family">Bethkenhagen</namePart>
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  <namePart>NOMIS Fellowship Program</namePart>
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<abstract lang="eng">Hydrocarbon mixtures are extremely abundant in the Universe, and diamond formation from them can play a crucial role in shaping the interior structure and evolution of planets. With first-principles accuracy, we first estimate the melting line of diamond, and then reveal the nature of chemical bonding in hydrocarbons at extreme conditions. We finally establish the pressure-temperature phase boundary where it is thermodynamically possible for diamond to form from hydrocarbon mixtures with different atomic fractions of carbon. Notably, here we show a depletion zone at pressures above 200 GPa and temperatures below 3000 K-3500 K where diamond formation is thermodynamically favorable regardless of the carbon atomic fraction, due to a phase separation mechanism. The cooler condition of the interior of Neptune compared to Uranus means that the former is much more likely to contain the depletion zone. Our findings can help explain the dichotomy of the two ice giants manifested by the low luminosity of Uranus, and lead to a better understanding of (exo-)planetary formation and evolution.</abstract>

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<originInfo><publisher>Springer Nature</publisher><dateIssued encoding="w3cdtf">2023</dateIssued>
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<language><languageTerm authority="iso639-2b" type="code">eng</languageTerm>
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<relatedItem type="host"><titleInfo><title>Nature Communications</title></titleInfo>
  <identifier type="eIssn">2041-1723</identifier>
  <identifier type="MEDLINE">36843123</identifier>
  <identifier type="ISI">000939678300002</identifier><identifier type="doi">10.1038/s41467-023-36841-1</identifier>
<part><detail type="volume"><number>14</number></detail>
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<apa>Cheng, B., Hamel, S., &amp;#38; Bethkenhagen, M. (2023). Thermodynamics of diamond formation from hydrocarbon mixtures in planets. &lt;i&gt;Nature Communications&lt;/i&gt;. Springer Nature. &lt;a href=&quot;https://doi.org/10.1038/s41467-023-36841-1&quot;&gt;https://doi.org/10.1038/s41467-023-36841-1&lt;/a&gt;</apa>
<ista>Cheng B, Hamel S, Bethkenhagen M. 2023. Thermodynamics of diamond formation from hydrocarbon mixtures in planets. Nature Communications. 14, 1104.</ista>
<chicago>Cheng, Bingqing, Sebastien Hamel, and Mandy Bethkenhagen. “Thermodynamics of Diamond Formation from Hydrocarbon Mixtures in Planets.” &lt;i&gt;Nature Communications&lt;/i&gt;. Springer Nature, 2023. &lt;a href=&quot;https://doi.org/10.1038/s41467-023-36841-1&quot;&gt;https://doi.org/10.1038/s41467-023-36841-1&lt;/a&gt;.</chicago>
<mla>Cheng, Bingqing, et al. “Thermodynamics of Diamond Formation from Hydrocarbon Mixtures in Planets.” &lt;i&gt;Nature Communications&lt;/i&gt;, vol. 14, 1104, Springer Nature, 2023, doi:&lt;a href=&quot;https://doi.org/10.1038/s41467-023-36841-1&quot;&gt;10.1038/s41467-023-36841-1&lt;/a&gt;.</mla>
<ama>Cheng B, Hamel S, Bethkenhagen M. Thermodynamics of diamond formation from hydrocarbon mixtures in planets. &lt;i&gt;Nature Communications&lt;/i&gt;. 2023;14. doi:&lt;a href=&quot;https://doi.org/10.1038/s41467-023-36841-1&quot;&gt;10.1038/s41467-023-36841-1&lt;/a&gt;</ama>
<short>B. Cheng, S. Hamel, M. Bethkenhagen, Nature Communications 14 (2023).</short>
<ieee>B. Cheng, S. Hamel, and M. Bethkenhagen, “Thermodynamics of diamond formation from hydrocarbon mixtures in planets,” &lt;i&gt;Nature Communications&lt;/i&gt;, vol. 14. Springer Nature, 2023.</ieee>
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