Inference of a “Hot Ice” Layer in Nitrogen-Rich Planets: Demixing the Phase Diagram and Phase Composition for Variable Concentration Helium–Nitrogen Mixtures Based on Isothermal Compression-Reference-Cited by-同舟云学术

Inference of a “Hot Ice” Layer in Nitrogen-Rich Planets: Demixing the Phase Diagram and Phase Composition for Variable Concentration Helium–Nitrogen Mixtures Based on Isothermal Compression

Published:2022-06-01 Issue:23 Volume:126 Page:3745-3757
ISSN:1089-5639
Container-title:The Journal of Physical Chemistry A
language:en
Short-container-title:J. Phys. Chem. A

Author:

Li Xiangdong¹,Su Hao¹,Liang Wentao¹,Zhou Wenju²,Rahman Azizur¹,Xu Zilong¹,Zhong Cheng¹,Mai Di¹,Dai Rucheng³⁴,Gou Huiyang²^ORCID,Wang Zhongping³⁴,Zheng Xianxu⁵,Wu Qiang⁵,Zhang Zengming³⁴^ORCID

Affiliation:

1. Department of Physics, University of Science and Technology of China, Hefei, Anhui 230026, China

2. Center for High Pressure Science and Technology Advanced Research, Beijing 100094, China

3. The Centre for Physical Experiments, University of Science and Technology of China, Hefei, Anhui 230026, China

4. Frontiers Science Center for Planetary Exploration and Emerging Technologies, University of Science and Technology of China, Hefei, Anhui 230026, China

5. Institute of Fluid Physics, China Academy of Engineering Physics, Mianyang, Sichuan 360001, China

Funder

National Natural Science Foundation of China

National Key Laboratory of Shock Wave and Detonation Physics Foundation

Publisher

American Chemical Society (ACS)

Subject

Physical and Theoretical Chemistry

Link

https://pubs.acs.org/doi/pdf/10.1021/acs.jpca.2c02132

Reference87 articles.

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4. Gas-phase chemistry in dense interstellar clouds including grain surface molecular depletion and desorption

5. Estimates of N2 abundances in dense molecular clouds