2019
DOI: 10.1080/09506608.2018.1560984
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Cementite

Abstract: Cementite occurs in steels, in meteorites, possibly at the core of the Earth and has uses in its pure form. It's composition can deviate from Fe 3 C, but not by much because the Fe-C bond contributes to its cohesion. Its crystallographic unit cell is orthorhombic and primitive, with large lattice parameters, explaining its hardness. Many of its properties are anisotropic. Its single-crystal elastic properties have been investigated using first-principles calculations and by clever experiments. The iron atoms i… Show more

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Cited by 103 publications
(57 citation statements)
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“…Therefore, in the low-temperature region, the most stable clusters in the melt are formed on the basis of cementite Fe 3 C, which has a melting point of 1923 K [30]. Iron in cementite can be replaced by Mn or other transition metals [31].…”
Section: Resultsmentioning
confidence: 99%
“…Therefore, in the low-temperature region, the most stable clusters in the melt are formed on the basis of cementite Fe 3 C, which has a melting point of 1923 K [30]. Iron in cementite can be replaced by Mn or other transition metals [31].…”
Section: Resultsmentioning
confidence: 99%
“…Upper limit of the shape anisotropy ( K d ) estimated from the dependence , which is valid for non-interacting particles having an oblate spheroidal shape (b >> a) [ 46 , 48 ] and lower limit calculated for prolate nanoparticles [ 47 ]. Density for cementite: 7.6 g/cm 3 [ 49 , 50 ] . In parentheses, K d values are given for weighted average density: 6.5 g/cm 3 ; in this case 5.3 g/cm 3 for Fe 2 O 3 , ~4.0 g/cm 3 for ferrihydrates [ 51 ], 7.9 g/cm 3 for Fe, and 7.6 g/cm 3 for Fe 3 C. Contributions of these iron phases were taken from the Mössbauer spectra at 85K ( Table S1 ).…”
Section: Figurementioning
confidence: 99%
“…Meteoric irons, known as Fe–Ni alloys with various nickel contents from a minimum of 5 up to 60 mass%, can be classified into several types exhibiting different microstructural features based on their overall nickel content 1 . The main phases of meteoric iron are kamacite with a body-centred cubic (BCC) structure, taenite with a face-centred cubic (FCC) structure, and cohenite with an orthorhombic structure, which correspond to α-ferrite, γ-austenite, and Fe 3 C cementite in artificial steel, respectively 2 6 . The unique microstructure of meteoric iron is formed by the nucleation and growth of kamacite from taenite during the slow cooling of the parent body 1 , with the cooling period for a 1 K temperature decrease estimated as a few hundred to thousands of years 1 .…”
Section: Introductionmentioning
confidence: 99%