2014
DOI: 10.1016/j.actamat.2014.06.066
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Understanding sigma-phase precipitation in a stabilized austenitic stainless steel (316Nb) through complementary CALPHAD-based and experimental investigations

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Cited by 56 publications
(22 citation statements)
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“…As an example, A. Perron et al [34] have studied the influence of σ phase in a 316Nb austenitic stainless steel. They observed two different mechanisms of precipitation of sigma phase.…”
Section: Introductionmentioning
confidence: 99%
See 1 more Smart Citation
“…As an example, A. Perron et al [34] have studied the influence of σ phase in a 316Nb austenitic stainless steel. They observed two different mechanisms of precipitation of sigma phase.…”
Section: Introductionmentioning
confidence: 99%
“…Another important aspect is that the kinetics of sigma phase's nucleation is very fast at 850 • C due to the eutectoid decomposition of the ferrite into sigma phase and secondary austenitic phase [29][30][31][32][33][34]. As an example, A. Perron et al [34] have studied the influence of σ phase in a 316Nb austenitic stainless steel.…”
Section: Introductionmentioning
confidence: 99%
“…Since the Sigma phase is stable in all four constituent ternaries [8,10,17] and has been frequently reported in the austenitic stainless steels, [2,3,[5][6][7]23] the experimental phase equilibrium data in literature can reasonably constrain the modeling of these end-members and interaction terms. The Chi phase has a bcc unit cell (space group I 143 m) containing 58 atoms and having a reported lattice parameter varying between 0.8807 and 0.892 nm [3,24] phase.…”
Section: ðYþ: ½2mentioning
confidence: 99%
“…A good understanding of the solubilities of Cr, Ni, and Mo in the Fe-rich facecentered cubic (fcc) matrix phase and the intermetallic phases is essential for making robust choices regarding alloy compositions and heat treatment parameters, and to ensure better microstructures and mechanical properties. While the stability of Sigma phase in austenitic stainless steels has been studied in depth recently, [5][6][7] the Chi and Laves phases are less investigated. The composition and temperature regions of stable Chi and Laves phases have been studied in constituent ternaries of the Fe-Cr-Mo, Fe-Mo-Ni, Fe-Cr-Ni, and Cr-Mo-Ni systems, [8][9][10][11][12][13] but knowledge on their stability in the quaternary Fe-Cr-Ni-Mo space is still lacking.…”
Section: Introductionmentioning
confidence: 98%
“…More precisely, precipitation of r phase has been reported after aging in the temperature range from 773 K to 1173 K (500°C to 900°C). [1][2][3][4] 1138 K (865°C) has been identified as the most critical temperature for r phase formation [5] and certainly corresponds to the nose of the Time-Temperature-Transformation curve. Secondary M 23 C 6 carbides start precipitating below 1323 K (1050°C).…”
Section: Introductionmentioning
confidence: 99%