Machine Learning simulations reveal oxygen’s phase diagram and thermal properties at conditions relevant to white dwarfs

Abstract Current studies show that oxygen does not aggregate into a polymeric phase even under pressures up to 10 TPa. To address the critical knowledge gap in understanding dense oxygen, here we show the complete polymerization process of oxygen, by using structure prediction methods. We determine...

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Main Authors: Yunlong Wang, Jiuyang Shi, Zhixin Liang, Tianheng Huang, Junjie Wang, Chi Ding, Chris J. Pickard, Hui-Tian Wang, Dingyu Xing, Dongdong Ni, Jian Sun
Format: Article
Language:English
Published: Nature Portfolio 2025-07-01
Series:Nature Communications
Online Access:https://doi.org/10.1038/s41467-025-61390-0
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author Yunlong Wang
Jiuyang Shi
Zhixin Liang
Tianheng Huang
Junjie Wang
Chi Ding
Chris J. Pickard
Hui-Tian Wang
Dingyu Xing
Dongdong Ni
Jian Sun
author_facet Yunlong Wang
Jiuyang Shi
Zhixin Liang
Tianheng Huang
Junjie Wang
Chi Ding
Chris J. Pickard
Hui-Tian Wang
Dingyu Xing
Dongdong Ni
Jian Sun
author_sort Yunlong Wang
collection DOAJ
description Abstract Current studies show that oxygen does not aggregate into a polymeric phase even under pressures up to 10 TPa. To address the critical knowledge gap in understanding dense oxygen, here we show the complete polymerization process of oxygen, by using structure prediction methods. We determine the crystal structures of oxygen up to 1 PPa (1000 TPa), identifying a novel two-dimensionally bonded body-centered tetragonal (bct) phase and a fully polymerized hexagonal close-packed (hcp) phase. Electronic structure analysis reveals significant bond softening in the bct phase with increasing pressure, which may affect the dynamic behavior under finite temperatures. So, we employ the machine learning potential molecular dynamics and the two-phase method to construct the melting curve of oxygen up to 200 TPa (200 TPa, 23,740 K) and identify abnormal melting behavior beyond 100 TPa. We find oxygen exhibits higher thermal conductivity and lower isochoric heat capacity than helium at identical pressures. These results indicate that oxygen-rich envelopes may accelerate the cooling process of white dwarfs.
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id doaj-art-c1d8f0f064d44e7ba988c0314bf6f878
institution Kabale University
issn 2041-1723
language English
publishDate 2025-07-01
publisher Nature Portfolio
record_format Article
series Nature Communications
spelling doaj-art-c1d8f0f064d44e7ba988c0314bf6f8782025-08-20T04:01:36ZengNature PortfolioNature Communications2041-17232025-07-011611710.1038/s41467-025-61390-0Machine Learning simulations reveal oxygen’s phase diagram and thermal properties at conditions relevant to white dwarfsYunlong Wang0Jiuyang Shi1Zhixin Liang2Tianheng Huang3Junjie Wang4Chi Ding5Chris J. Pickard6Hui-Tian Wang7Dingyu Xing8Dongdong Ni9Jian Sun10National Laboratory of Solid State Microstructures, School of Physics and Collaborative Innovation Center of Advanced Microstructures, Nanjing UniversityNational Laboratory of Solid State Microstructures, School of Physics and Collaborative Innovation Center of Advanced Microstructures, Nanjing UniversityNational Laboratory of Solid State Microstructures, School of Physics and Collaborative Innovation Center of Advanced Microstructures, Nanjing UniversityNational Laboratory of Solid State Microstructures, School of Physics and Collaborative Innovation Center of Advanced Microstructures, Nanjing UniversityNational Laboratory of Solid State Microstructures, School of Physics and Collaborative Innovation Center of Advanced Microstructures, Nanjing UniversityNational Laboratory of Solid State Microstructures, School of Physics and Collaborative Innovation Center of Advanced Microstructures, Nanjing UniversityDepartment of Materials Science & Metallurgy, University of Cambridge, 27 Charles Babbage RoadNational Laboratory of Solid State Microstructures, School of Physics and Collaborative Innovation Center of Advanced Microstructures, Nanjing UniversityNational Laboratory of Solid State Microstructures, School of Physics and Collaborative Innovation Center of Advanced Microstructures, Nanjing UniversityInstitute of Science and Technology for Deep Space Exploration, Nanjing UniversityNational Laboratory of Solid State Microstructures, School of Physics and Collaborative Innovation Center of Advanced Microstructures, Nanjing UniversityAbstract Current studies show that oxygen does not aggregate into a polymeric phase even under pressures up to 10 TPa. To address the critical knowledge gap in understanding dense oxygen, here we show the complete polymerization process of oxygen, by using structure prediction methods. We determine the crystal structures of oxygen up to 1 PPa (1000 TPa), identifying a novel two-dimensionally bonded body-centered tetragonal (bct) phase and a fully polymerized hexagonal close-packed (hcp) phase. Electronic structure analysis reveals significant bond softening in the bct phase with increasing pressure, which may affect the dynamic behavior under finite temperatures. So, we employ the machine learning potential molecular dynamics and the two-phase method to construct the melting curve of oxygen up to 200 TPa (200 TPa, 23,740 K) and identify abnormal melting behavior beyond 100 TPa. We find oxygen exhibits higher thermal conductivity and lower isochoric heat capacity than helium at identical pressures. These results indicate that oxygen-rich envelopes may accelerate the cooling process of white dwarfs.https://doi.org/10.1038/s41467-025-61390-0
spellingShingle Yunlong Wang
Jiuyang Shi
Zhixin Liang
Tianheng Huang
Junjie Wang
Chi Ding
Chris J. Pickard
Hui-Tian Wang
Dingyu Xing
Dongdong Ni
Jian Sun
Machine Learning simulations reveal oxygen’s phase diagram and thermal properties at conditions relevant to white dwarfs
Nature Communications
title Machine Learning simulations reveal oxygen’s phase diagram and thermal properties at conditions relevant to white dwarfs
title_full Machine Learning simulations reveal oxygen’s phase diagram and thermal properties at conditions relevant to white dwarfs
title_fullStr Machine Learning simulations reveal oxygen’s phase diagram and thermal properties at conditions relevant to white dwarfs
title_full_unstemmed Machine Learning simulations reveal oxygen’s phase diagram and thermal properties at conditions relevant to white dwarfs
title_short Machine Learning simulations reveal oxygen’s phase diagram and thermal properties at conditions relevant to white dwarfs
title_sort machine learning simulations reveal oxygen s phase diagram and thermal properties at conditions relevant to white dwarfs
url https://doi.org/10.1038/s41467-025-61390-0
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