{"title":"Thermal expansion of iron phosphides","authors":"Yuan Yin, Wen Wen, Shuangmeng Zhai","doi":"10.1007/s00269-026-01354-y","DOIUrl":null,"url":null,"abstract":"<div><p>Iron-rich phosphides are functional materials for the hydrogen evolution reaction and also analogues of Fe-Ni-P minerals found in meteorites and pyrometamorphic rocks on Earth. They are also potential components in solid metallic cores of the Earth, Mars, and other terrestrial planets. The thermal expansion coefficients (<i>α</i>) of three iron-rich phosphides (FeP, Fe<sub>2</sub>P, and Fe<sub>3</sub>P) were investigated by in-situ synchrotron X-ray powder diffraction from room temperature to 1073 K. By fitting the obtained volume-temperature (<i>V</i>-<i>T</i>) data using a function of α(<i>T</i>) = α<sub>0</sub> + α<sub>1</sub>⋅<i>T</i> (Fei model), the parameters α<sub>0</sub> and α<sub>1</sub> for FeP’s volume are 2.60(22) ⋅10<sup>− 5</sup> K<sup>− 1</sup> and 3.57(36) ⋅10<sup>− 8</sup> K<sup>− 2</sup>, for Fe<sub>2</sub>P’s volume are 3.26(37) ⋅10<sup>− 5</sup> K<sup>− 1</sup> and 3.70(64) ⋅10<sup>− 8</sup> K<sup>− 2</sup>, and for Fe<sub>3</sub>P’s volume are 1.96(20) ⋅10<sup>− 5</sup> K<sup>− 1</sup> and 4.01(32) ⋅10<sup>− 8</sup> K<sup>− 2</sup>, respectively. Axial thermal expansions are different in three iron phosphides. Combined with previous results, the density profiles of solid Fe<sub>3</sub>P and FeP in the Martian core conditions were calculated and compared with those of Fe<sub>3</sub>S, FeS and fcc Fe. Fe<sub>3</sub>P has a similar density to Fe<sub>3</sub>S under Martian core conditions, suggesting that phosphorus can exist in the Martian solid inner core if the core comprises iron sulfide.</p></div>","PeriodicalId":20132,"journal":{"name":"Physics and Chemistry of Minerals","volume":"53 2","pages":""},"PeriodicalIF":1.5000,"publicationDate":"2026-05-18","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Physics and Chemistry of Minerals","FirstCategoryId":"89","ListUrlMain":"https://link.springer.com/article/10.1007/s00269-026-01354-y","RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q4","JCRName":"MATERIALS SCIENCE, MULTIDISCIPLINARY","Score":null,"Total":0}
引用次数: 0
Abstract
Iron-rich phosphides are functional materials for the hydrogen evolution reaction and also analogues of Fe-Ni-P minerals found in meteorites and pyrometamorphic rocks on Earth. They are also potential components in solid metallic cores of the Earth, Mars, and other terrestrial planets. The thermal expansion coefficients (α) of three iron-rich phosphides (FeP, Fe2P, and Fe3P) were investigated by in-situ synchrotron X-ray powder diffraction from room temperature to 1073 K. By fitting the obtained volume-temperature (V-T) data using a function of α(T) = α0 + α1⋅T (Fei model), the parameters α0 and α1 for FeP’s volume are 2.60(22) ⋅10− 5 K− 1 and 3.57(36) ⋅10− 8 K− 2, for Fe2P’s volume are 3.26(37) ⋅10− 5 K− 1 and 3.70(64) ⋅10− 8 K− 2, and for Fe3P’s volume are 1.96(20) ⋅10− 5 K− 1 and 4.01(32) ⋅10− 8 K− 2, respectively. Axial thermal expansions are different in three iron phosphides. Combined with previous results, the density profiles of solid Fe3P and FeP in the Martian core conditions were calculated and compared with those of Fe3S, FeS and fcc Fe. Fe3P has a similar density to Fe3S under Martian core conditions, suggesting that phosphorus can exist in the Martian solid inner core if the core comprises iron sulfide.
期刊介绍:
Physics and Chemistry of Minerals is an international journal devoted to publishing articles and short communications of physical or chemical studies on minerals or solids related to minerals. The aim of the journal is to support competent interdisciplinary work in mineralogy and physics or chemistry. Particular emphasis is placed on applications of modern techniques or new theories and models to interpret atomic structures and physical or chemical properties of minerals. Some subjects of interest are:
-Relationships between atomic structure and crystalline state (structures of various states, crystal energies, crystal growth, thermodynamic studies, phase transformations, solid solution, exsolution phenomena, etc.)
-General solid state spectroscopy (ultraviolet, visible, infrared, Raman, ESCA, luminescence, X-ray, electron paramagnetic resonance, nuclear magnetic resonance, gamma ray resonance, etc.)
-Experimental and theoretical analysis of chemical bonding in minerals (application of crystal field, molecular orbital, band theories, etc.)
-Physical properties (magnetic, mechanical, electric, optical, thermodynamic, etc.)
-Relations between thermal expansion, compressibility, elastic constants, and fundamental properties of atomic structure, particularly as applied to geophysical problems
-Electron microscopy in support of physical and chemical studies
-Computational methods in the study of the structure and properties of minerals
-Mineral surfaces (experimental methods, structure and properties)