2015
DOI: 10.1080/09500839.2015.1087652
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Kinetics of interstitial segregation in Cottrell atmospheres and grain boundaries

Abstract: Trapping of interstitial (e.g. carbon) atoms is driven by the reduction in energy in the system. Diffusion of interstitials, together with their trapping in dislocation cores and/or grain boundaries, is studied by the thermodynamic extremal principle. In addition to the total Gibbs energy, a well-established formulation of the total dissipation is applied. Dimension-free evolution equations are derived, whose solution is well approximated by an easy to handle kinetic equation. Cottrell's power law can be verif… Show more

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Cited by 21 publications
(12 citation statements)
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“…The rate of C segregating from the undisturbed crystal into the stress field of dislocations has been derived using the Thermodynamic Extremal Principle, [ 15 ] yieldingtruey˙normalT=2Dπρf4extrue(ln4extrue(1f4extrue)344extrue)ynormalL(lnynormalLfalse(1ynormalTfalse)ynormalTfalse(1ynormalLfalse)+ΔERnormalgT)where D is the bulk diffusion coefficient of C, ρ the dislocation density, f the volume fraction of dislocation trap sites, y L the site fraction of C uniformly distributed in the matrix, y T the site fraction of C in dislocation traps, Δ E the trapping energy for C in dislocations, R g the gas constant, and T the temperature. The volume fraction of dislocation trap sites, f , is given byf=Zcdcwhere c dc is the volume fraction of atoms located in the dislocation cores and Z the coordination numbercdc=2πrc2ρZ=AT2…”
Section: Modelingmentioning
confidence: 99%
See 2 more Smart Citations
“…The rate of C segregating from the undisturbed crystal into the stress field of dislocations has been derived using the Thermodynamic Extremal Principle, [ 15 ] yieldingtruey˙normalT=2Dπρf4extrue(ln4extrue(1f4extrue)344extrue)ynormalL(lnynormalLfalse(1ynormalTfalse)ynormalTfalse(1ynormalLfalse)+ΔERnormalgT)where D is the bulk diffusion coefficient of C, ρ the dislocation density, f the volume fraction of dislocation trap sites, y L the site fraction of C uniformly distributed in the matrix, y T the site fraction of C in dislocation traps, Δ E the trapping energy for C in dislocations, R g the gas constant, and T the temperature. The volume fraction of dislocation trap sites, f , is given byf=Zcdcwhere c dc is the volume fraction of atoms located in the dislocation cores and Z the coordination numbercdc=2πrc2ρZ=AT2…”
Section: Modelingmentioning
confidence: 99%
“…The main input parameters for the evolution of C-trapping are temperature, C-content, and dislocation density. The Gibbs energy for trapping can be derived as [15] G…”
Section: Cottrell Atmosphere Formationmentioning
confidence: 99%
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“…The smaller k values for the decarburized iron, ball milled iron, and IF iron measurements, as compared to the mild steel value, illustrate the lesser constraining effect produced at grain boundaries by reduction in the carbon content. A recent report has been made on different aspects of carbon segregation at individual dislocations and relating to pile-ups at grain boundaries [16]. Such segregation applies also for high manganese (fcc) austenitic steels [17].…”
Section: Constrained Polycrystalline Plasticitymentioning
confidence: 99%
“…The problem of interaction between dislocations and interstitial atoms as carbon or hydrogen is of increasing interest with respect to a detailed understanding of Cottrell clouds [1], and their kinetics [2]. To calculate the main physical quantity, i.e., the interaction energy between the stress field of a distinct dislocation and of the interstitial atoms, one can use the superposition of the elastic fields generated by the dislocation and by eigenstrains due to deposition of the atoms in interstitial positions.…”
Section: Introductionmentioning
confidence: 99%