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Cottrell atmosphere

In materials science, the concept of the Cottrell atmosphere was introduced by A. H. Cottrell and B. A. Bilby in 1949[1] to explain how dislocations are pinned in some metals by boron, carbon, or nitrogen interstitials.

A carbon atom below a dislocation in iron, forming a Cottrell atmosphere

Cottrell atmospheres occur in body-centered cubic (BCC) and face-centered cubic (FCC) materials, such as iron or nickel, with small impurity atoms, such as boron,[2] carbon,[3] or nitrogen.[citation needed] As these interstitial atoms distort the lattice slightly, there will be an associated residual stress field surrounding the interstitial. This stress field can be relaxed by the interstitial atom diffusing towards a dislocation[citation needed], which contains a small gap at its core (as it is a more open structure), see Figure 1. Once the atom has diffused into the dislocation core the atom will stay. Typically only one interstitial atom is required per lattice plane of the dislocation.[citation needed] The collection of solute atoms around the dislocation core due to this process is the Cottrell atmosphere.

Influence on Mechanical Behavior edit

 
A dislocation moving with a Cottrell Atmosphere around it. At high stresses (top), the dislocation can "break free" of the atmosphere, while at low stresses (bottom), the dislocation must drag the solutes with it, and motion is much slower.

The collection of solute atoms at the dislocation relieves the stresses associated with the dislocation, which lowers the energy of the dislocation's presence. Thus, moving the dislocation out of this Cottrell atmosphere constitutes an increase in energy, so it is not favorable for the dislocation to move forward in the crystal. As a result, the dislocation is effectively pinned by the Cottrell atmosphere.

Once a dislocation has become pinned, a large force is required to unpin the dislocation prior the yielding, thus at room temperature, the dislocation will not get unpinned.[4] This produces an observed upper yield point in a stress–strain graph. Beyond the upper yield point, the pinned dislocation will act as Frank–Read source to generate new dislocations that are not pinned. These dislocations are free to move in the crystal, which results in a subsequent lower yield point, and the material will deform in a more plastic manner.

Leaving the sample to age, by holding it at room temperature for a few hours, enables the carbon atoms to rediffuse back to dislocation cores, resulting in a return of the upper yield point.

Cottrell atmospheres lead to formation of Lüders bands and large forces for deep drawing and forming large sheets, making them a hindrance to manufacture. Some steels are designed to remove the Cottrell atmosphere effect by removing all the interstitial atoms. Steels such as interstitial free steel are decarburized and small quantities of titanium are added to remove nitrogen.

The Cottrell atmosphere also has important consequences for material behavior at high homologous temperatures, i.e. when the material is experiencing creep conditions. Moving a dislocation with an associated Cottrell atmosphere introduces viscous drag, an effective frictional force that makes moving the dislocation more difficult[5] (and thus slowing plastic deformation). This drag force can be expressed according to the equation:

 ,

where   is the diffusivity of the solute atom in the host material,   is the atomic volume,   is the velocity of the dislocation,   is the diffusion flux density, and   is the solute concentration.[5] The existence of the Cottrell atmosphere and the effects of viscous drag have been proven to be important in high temperature deformation at intermediate stresses, as well as contributing to the power-law breakdown regime.[6]

Similar phenomena edit

While the Cottrell atmosphere is a general effect, there are additional related mechanisms that occur under more specialized circumstances.

Suzuki effect edit

The Suzuki effect is characterized by the segregation of solutes to stacking fault defects. When dislocations in an FCC system split into two partial dislocations, a hexagonal close-packed (HCP) stacking fault is formed between the two partials. H. Suzuki predicted that the concentration of solute atoms at this boundary would differ from the bulk. Moving through this field of solute atoms would therefore produce a similar drag on dislocations as the Cottrell atmosphere.[7] Suzuki later observed such segregation in 1961.[8] The Suzuki effect is often associated with adsorption of substitutional solute atoms to the stacking fault, but it has also been found to occur with interstitial atoms diffusing out of the stacking fault.[9]

Once two partial dislocations have split, they cannot cross-slip around obstacles anymore. Just as the Cottrell atmosphere provided a force against dislocation motion, the Suzuki effect in the stacking fault will lead to increased stresses for recombination of partials, leading to increased difficulty in bypassing obstacles (such as precipitates or particles), and therefore resulting in a stronger material.

Snoek effect edit

Under an applied stress, interstitial solute atoms, such as carbon and nitrogen can migrate within the α-Fe lattice, a BCC metal. These short-range migrations of carbon and nitrogen solute atoms result in an internal friction or an elastic effect, called the Snoek effect. The Snoek effect was discovered by J. L. Snoek in 1941. At room temperature, the solubility of carbon and nitrogen in solid solutions is exceedingly small.[10] By raising, the temperature beyond 400oC and cooling at a moderate rate, it is easy to keep a few hundredths of a percent of either element within the solution, while the remainder is supersaturated.[10] This revelation led to observed special magnetic phenomena in iron, mainly the presence of magnetism and time decrease of permeability due to small amount of carbon and nitrogen remaining in the iron.[10] Moreover, the additional presence of magnetism leads to an elastic-after effect.[11]

By preparing samples containing a larger amount of carbon or nitrogen in solid solution, magnetic and elastic phenomena are greatly enhanced. The solubility of nitrogen is much larger than the solubility of carbon in solid solution.[10] The study of the Snoek effect on annealed irons provides a reliable mechanism for calculating the solubility of carbon and nitrogen in α-iron.[12] A sample in a mixture of hydrogen and ammonia (or carbon monoxide) is mixed and heated until a stationary state was reached, where the mass of carbon and nitrogen taken up during the process can be found by estimating the changes in the weight of the sample.[10]

Carbon and nitrogen atoms occupy octahedral interstices at the midpoints of the cube edges and at the centers of the cube faces.[13] If a stress is applied a long the z, or [001] direction, the octahedral interstices along the x- and y-axes will contract, while the octahedral interstices along the z-direction expand.[13] Eventually, the interstitial atoms move to sites along the z-axis.[13] When the interstitial atoms move, this leads to a reduction in strain energy. In BCC metals, interstitial sites of an unstrained lattice are equally favorable. The interstitial solutes create elastic dipoles.[14] However, once a strain is applied on the lattice, such as that formed by a dislocation, 1/3 of the sites become more favorable than the other 2/3. Solute atoms will therefore move to occupy the favorable sites, forming a short ranged order of solutes immediately within the vicinity of the dislocation.[15] The motion of the interstitial solutes to these other sites constitutes a change in the elastic dipoles, so there is a relaxation time associated with this change which can be connected to the diffusivity and migration enthalpy of the solute atoms.[14] In the new, relaxed solute configuration, more energy is therefore required to break a dislocation from this order.

However, a stress applied in the [111] direction will not lead to any changes in the locations of the interstitial atoms as the three directions of the cube will be equally stressed, and on average, equally occupied by carbon atoms.[13] When a stress is applied along a cube edge and at an amount below the yield stress, the interstitial atom will lead to strain lagging before stress, showing the presence of internal friction.[13] A torsional pendulum is typically used as a means of studying this lagging effect. The angle of lag is taken to be δ and tan δ is considered a measure of internal friction.[13] The internal friction is expressed according to the equation:

 

Where the logarithmic decrement is the ratio of consecutive magnitudes of one cycle of the pendulum.[13] When the magnitude of one cycle decreases to   of its original value in time  , then the internal fraction behaves according to the equation:

 

Where   is the vibrational frequency of the pendulum.[13]

The interstitials that occupy the normal sites in an unstressed lattice will promote internal friction.[13] Substituted solute atoms and interstitials in strain fields of a dislocation or at grain boundaries have their internal friction changed.[13] Therefore, the Snoek effect can measure carbon and nitrogen concentration in BCC alpha-Fe and other solutes present in ternary alloys.[16]

Materials edit

Materials in which dislocations described by Cottrell atmosphere include metals and semiconductor materials such silicon crystals.

References edit

  1. ^ Cottrell, A. H.; Bilby, B. A. (1949), "Dislocation Theory of Yielding and Strain Ageing of Iron", Proceedings of the Physical Society, 62 (1): 49–62, Bibcode:1949PPSA...62...49C, doi:10.1088/0370-1298/62/1/308
  2. ^ Blavette, D.; Cadel, E.; Fraczkiewicz, A.; Menand, A. (1999). "Three-Dimensional Atomic-Scale Imaging of Impurity Segregation to Line Defects". Science. 286 (5448): 2317–2319. doi:10.1126/science.286.5448.2317. PMID 10600736.
  3. ^ Waseda, Osamu; Veiga, Roberto GA; Morthomas, Julien; Chantrenne, Patrice; Becquart, Charlotte S.; Ribeiro, Fabienne; Jelea, Andrei; Goldenstein, Helio; Perez, Michel (March 2017). "Formation of carbon Cottrell atmospheres and their effect on the stress field around an edge dislocation". Scripta Materialia. 129: 16–19. doi:10.1016/j.scriptamat.2016.09.032. ISSN 1359-6462.
  4. ^ Veiga, R.G.A.; Goldenstein, H.; Perez, M.; Becquart, C.S. (1 November 2015). "Monte Carlo and molecular dynamics simulations of screw dislocation locking by Cottrell atmospheres in low carbon Fe–C alloys". Scripta Materialia. 108: 19–22. doi:10.1016/j.scriptamat.2015.06.012. ISSN 1359-6462.
  5. ^ a b Takeuchi, S.; Argon, A. S. (1976-10-01). "Steady-state creep of alloys due to viscous motion of dislocations". Acta Metallurgica. 24 (10): 883–889. doi:10.1016/0001-6160(76)90036-5. ISSN 0001-6160.
  6. ^ Mohamed, Farghalli A. (1979-04-01). "Creep behavior of solid solution alloys". Materials Science and Engineering. 38 (1): 73–80. doi:10.1016/0025-5416(79)90034-X. ISSN 0025-5416.
  7. ^ Suzuki, Hideji (1952-01-01). "Chemical Interaction of Solute Atoms with Dislocations". Science Reports of the Research Institutes, Tohoku University. Ser. A, Physics, Chemistry and Metallurgy (in Japanese). 4: 455–463.
  8. ^ Suzuki, Hideji (1962-02-15). "Segregation of Solute Atoms to Stacking Faults". Journal of the Physical Society of Japan. 17 (2): 322–325. Bibcode:1962JPSJ...17..322S. doi:10.1143/JPSJ.17.322. ISSN 0031-9015.
  9. ^ Hickel, T.; Sandlöbes, S.; Marceau, R. K. W.; Dick, A.; Bleskov, I.; Neugebauer, J.; Raabe, D. (2014-08-15). "Impact of nanodiffusion on the stacking fault energy in high-strength steels". Acta Materialia. 75: 147–155. Bibcode:2014AcMat..75..147H. doi:10.1016/j.actamat.2014.04.062. ISSN 1359-6454.
  10. ^ a b c d e Snoek, J. L. (1941-07-01). "Effect of small quantities of carbon and nitrogen on the elastic and plastic properties of iron". Physica. 8 (7): 711–733. Bibcode:1941Phy.....8..711S. doi:10.1016/S0031-8914(41)90517-7. ISSN 0031-8914.
  11. ^ Koiwa, M. (1971-09-01). "Theory of the snoek effect in ternary b.c.c. alloys". The Philosophical Magazine. 24 (189): 539–554. Bibcode:1971PMag...24..539K. doi:10.1080/14786437108217028. ISSN 0031-8086.
  12. ^ Gavriljuk, V. G.; Shyvaniuk, V. N.; Teus, S. M. (2021-12-15). "Mobility of dislocations in the iron-based C-, N-, H-solid solutions measured using internal friction: Effect of electron structure". Journal of Alloys and Compounds. 886: 161260. doi:10.1016/j.jallcom.2021.161260. ISSN 0925-8388.
  13. ^ a b c d e f g h i j Marc Meyers, Krishan Chawla (2009). Mechanical Behavior of Materials. Cambridge, UK: Cambridge. pp. 569–570. ISBN 978-0-511-45557-5.
  14. ^ a b Weller, M. (2006-12-20). "The Snoek relaxation in bcc metals—From steel wire to meteorites". Materials Science and Engineering: A. Proceedings of the 14th International Conference on Internal Friction and Mechanical Spectroscopy. 442 (1): 21–30. doi:10.1016/j.msea.2006.02.232. ISSN 0921-5093.
  15. ^ Hosford, William F. (2005). Mechanical behavior of materials. Cambridge: Cambridge University Press. ISBN 0-521-84670-6. OCLC 56482243.
  16. ^ Koiwa, M. (1971-09-01). "Theory of the snoek effect in ternary b.c.c. alloys". The Philosophical Magazine. 24 (189): 539–554. Bibcode:1971PMag...24..539K. doi:10.1080/14786437108217028. ISSN 0031-8086.

cottrell, atmosphere, materials, science, concept, introduced, cottrell, bilby, 1949, explain, dislocations, pinned, some, metals, boron, carbon, nitrogen, interstitials, carbon, atom, below, dislocation, iron, forming, occur, body, centered, cubic, face, cent. In materials science the concept of the Cottrell atmosphere was introduced by A H Cottrell and B A Bilby in 1949 1 to explain how dislocations are pinned in some metals by boron carbon or nitrogen interstitials A carbon atom below a dislocation in iron forming a Cottrell atmosphereCottrell atmospheres occur in body centered cubic BCC and face centered cubic FCC materials such as iron or nickel with small impurity atoms such as boron 2 carbon 3 or nitrogen citation needed As these interstitial atoms distort the lattice slightly there will be an associated residual stress field surrounding the interstitial This stress field can be relaxed by the interstitial atom diffusing towards a dislocation citation needed which contains a small gap at its core as it is a more open structure see Figure 1 Once the atom has diffused into the dislocation core the atom will stay Typically only one interstitial atom is required per lattice plane of the dislocation citation needed The collection of solute atoms around the dislocation core due to this process is the Cottrell atmosphere Contents 1 Influence on Mechanical Behavior 2 Similar phenomena 2 1 Suzuki effect 2 2 Snoek effect 3 Materials 4 ReferencesInfluence on Mechanical Behavior edit nbsp A dislocation moving with a Cottrell Atmosphere around it At high stresses top the dislocation can break free of the atmosphere while at low stresses bottom the dislocation must drag the solutes with it and motion is much slower The collection of solute atoms at the dislocation relieves the stresses associated with the dislocation which lowers the energy of the dislocation s presence Thus moving the dislocation out of this Cottrell atmosphere constitutes an increase in energy so it is not favorable for the dislocation to move forward in the crystal As a result the dislocation is effectively pinned by the Cottrell atmosphere Once a dislocation has become pinned a large force is required to unpin the dislocation prior the yielding thus at room temperature the dislocation will not get unpinned 4 This produces an observed upper yield point in a stress strain graph Beyond the upper yield point the pinned dislocation will act as Frank Read source to generate new dislocations that are not pinned These dislocations are free to move in the crystal which results in a subsequent lower yield point and the material will deform in a more plastic manner Leaving the sample to age by holding it at room temperature for a few hours enables the carbon atoms to rediffuse back to dislocation cores resulting in a return of the upper yield point Cottrell atmospheres lead to formation of Luders bands and large forces for deep drawing and forming large sheets making them a hindrance to manufacture Some steels are designed to remove the Cottrell atmosphere effect by removing all the interstitial atoms Steels such as interstitial free steel are decarburized and small quantities of titanium are added to remove nitrogen The Cottrell atmosphere also has important consequences for material behavior at high homologous temperatures i e when the material is experiencing creep conditions Moving a dislocation with an associated Cottrell atmosphere introduces viscous drag an effective frictional force that makes moving the dislocation more difficult 5 and thus slowing plastic deformation This drag force can be expressed according to the equation Fdrag kTWvDsol J JcdA displaystyle F drag frac kT Omega vD sol int frac J centerdot J c dA nbsp where Dsol displaystyle D sol nbsp is the diffusivity of the solute atom in the host material W displaystyle Omega nbsp is the atomic volume v displaystyle v nbsp is the velocity of the dislocation J displaystyle J nbsp is the diffusion flux density and c displaystyle c nbsp is the solute concentration 5 The existence of the Cottrell atmosphere and the effects of viscous drag have been proven to be important in high temperature deformation at intermediate stresses as well as contributing to the power law breakdown regime 6 Similar phenomena editWhile the Cottrell atmosphere is a general effect there are additional related mechanisms that occur under more specialized circumstances Suzuki effect edit The Suzuki effect is characterized by the segregation of solutes to stacking fault defects When dislocations in an FCC system split into two partial dislocations a hexagonal close packed HCP stacking fault is formed between the two partials H Suzuki predicted that the concentration of solute atoms at this boundary would differ from the bulk Moving through this field of solute atoms would therefore produce a similar drag on dislocations as the Cottrell atmosphere 7 Suzuki later observed such segregation in 1961 8 The Suzuki effect is often associated with adsorption of substitutional solute atoms to the stacking fault but it has also been found to occur with interstitial atoms diffusing out of the stacking fault 9 Once two partial dislocations have split they cannot cross slip around obstacles anymore Just as the Cottrell atmosphere provided a force against dislocation motion the Suzuki effect in the stacking fault will lead to increased stresses for recombination of partials leading to increased difficulty in bypassing obstacles such as precipitates or particles and therefore resulting in a stronger material Snoek effect edit Under an applied stress interstitial solute atoms such as carbon and nitrogen can migrate within the a Fe lattice a BCC metal These short range migrations of carbon and nitrogen solute atoms result in an internal friction or an elastic effect called the Snoek effect The Snoek effect was discovered by J L Snoek in 1941 At room temperature the solubility of carbon and nitrogen in solid solutions is exceedingly small 10 By raising the temperature beyond 400oC and cooling at a moderate rate it is easy to keep a few hundredths of a percent of either element within the solution while the remainder is supersaturated 10 This revelation led to observed special magnetic phenomena in iron mainly the presence of magnetism and time decrease of permeability due to small amount of carbon and nitrogen remaining in the iron 10 Moreover the additional presence of magnetism leads to an elastic after effect 11 By preparing samples containing a larger amount of carbon or nitrogen in solid solution magnetic and elastic phenomena are greatly enhanced The solubility of nitrogen is much larger than the solubility of carbon in solid solution 10 The study of the Snoek effect on annealed irons provides a reliable mechanism for calculating the solubility of carbon and nitrogen in a iron 12 A sample in a mixture of hydrogen and ammonia or carbon monoxide is mixed and heated until a stationary state was reached where the mass of carbon and nitrogen taken up during the process can be found by estimating the changes in the weight of the sample 10 Carbon and nitrogen atoms occupy octahedral interstices at the midpoints of the cube edges and at the centers of the cube faces 13 If a stress is applied a long the z or 001 direction the octahedral interstices along the x and y axes will contract while the octahedral interstices along the z direction expand 13 Eventually the interstitial atoms move to sites along the z axis 13 When the interstitial atoms move this leads to a reduction in strain energy In BCC metals interstitial sites of an unstrained lattice are equally favorable The interstitial solutes create elastic dipoles 14 However once a strain is applied on the lattice such as that formed by a dislocation 1 3 of the sites become more favorable than the other 2 3 Solute atoms will therefore move to occupy the favorable sites forming a short ranged order of solutes immediately within the vicinity of the dislocation 15 The motion of the interstitial solutes to these other sites constitutes a change in the elastic dipoles so there is a relaxation time associated with this change which can be connected to the diffusivity and migration enthalpy of the solute atoms 14 In the new relaxed solute configuration more energy is therefore required to break a dislocation from this order However a stress applied in the 111 direction will not lead to any changes in the locations of the interstitial atoms as the three directions of the cube will be equally stressed and on average equally occupied by carbon atoms 13 When a stress is applied along a cube edge and at an amount below the yield stress the interstitial atom will lead to strain lagging before stress showing the presence of internal friction 13 A torsional pendulum is typically used as a means of studying this lagging effect The angle of lag is taken to be d and tan d is considered a measure of internal friction 13 The internal friction is expressed according to the equation tan d log decrement p Q 1 displaystyle tan delta left frac log decrement pi right Q 1 nbsp Where the logarithmic decrement is the ratio of consecutive magnitudes of one cycle of the pendulum 13 When the magnitude of one cycle decreases to 1n displaystyle frac 1 n nbsp of its original value in time t displaystyle t nbsp then the internal fraction behaves according to the equation tan d Q 1 ln 1np v t displaystyle tan delta Q 1 frac ln frac 1 n pi times v times t nbsp Where v displaystyle v nbsp is the vibrational frequency of the pendulum 13 The interstitials that occupy the normal sites in an unstressed lattice will promote internal friction 13 Substituted solute atoms and interstitials in strain fields of a dislocation or at grain boundaries have their internal friction changed 13 Therefore the Snoek effect can measure carbon and nitrogen concentration in BCC alpha Fe and other solutes present in ternary alloys 16 Materials editMaterials in which dislocations described by Cottrell atmosphere include metals and semiconductor materials such silicon crystals References edit Cottrell A H Bilby B A 1949 Dislocation Theory of Yielding and Strain Ageing of Iron Proceedings of the Physical Society 62 1 49 62 Bibcode 1949PPSA 62 49C doi 10 1088 0370 1298 62 1 308 Blavette D Cadel E Fraczkiewicz A Menand A 1999 Three Dimensional Atomic Scale Imaging of Impurity Segregation to Line Defects Science 286 5448 2317 2319 doi 10 1126 science 286 5448 2317 PMID 10600736 Waseda Osamu Veiga Roberto GA Morthomas Julien Chantrenne Patrice Becquart Charlotte S Ribeiro Fabienne Jelea Andrei Goldenstein Helio Perez Michel March 2017 Formation of carbon Cottrell atmospheres and their effect on the stress field around an edge dislocation Scripta Materialia 129 16 19 doi 10 1016 j scriptamat 2016 09 032 ISSN 1359 6462 Veiga R G A Goldenstein H Perez M Becquart C S 1 November 2015 Monte Carlo and molecular dynamics simulations of screw dislocation locking by Cottrell atmospheres in low carbon Fe C alloys Scripta Materialia 108 19 22 doi 10 1016 j scriptamat 2015 06 012 ISSN 1359 6462 a b Takeuchi S Argon A S 1976 10 01 Steady state creep of alloys due to viscous motion of dislocations Acta Metallurgica 24 10 883 889 doi 10 1016 0001 6160 76 90036 5 ISSN 0001 6160 Mohamed Farghalli A 1979 04 01 Creep behavior of solid solution alloys Materials Science and Engineering 38 1 73 80 doi 10 1016 0025 5416 79 90034 X ISSN 0025 5416 Suzuki Hideji 1952 01 01 Chemical Interaction of Solute Atoms with Dislocations Science Reports of the Research Institutes Tohoku University Ser A Physics Chemistry and Metallurgy in Japanese 4 455 463 Suzuki Hideji 1962 02 15 Segregation of Solute Atoms to Stacking Faults Journal of the Physical Society of Japan 17 2 322 325 Bibcode 1962JPSJ 17 322S doi 10 1143 JPSJ 17 322 ISSN 0031 9015 Hickel T Sandlobes S Marceau R K W Dick A Bleskov I Neugebauer J Raabe D 2014 08 15 Impact of nanodiffusion on the stacking fault energy in high strength steels Acta Materialia 75 147 155 Bibcode 2014AcMat 75 147H doi 10 1016 j actamat 2014 04 062 ISSN 1359 6454 a b c d e Snoek J L 1941 07 01 Effect of small quantities of carbon and nitrogen on the elastic and plastic properties of iron Physica 8 7 711 733 Bibcode 1941Phy 8 711S doi 10 1016 S0031 8914 41 90517 7 ISSN 0031 8914 Koiwa M 1971 09 01 Theory of the snoek effect in ternary b c c alloys The Philosophical Magazine 24 189 539 554 Bibcode 1971PMag 24 539K doi 10 1080 14786437108217028 ISSN 0031 8086 Gavriljuk V G Shyvaniuk V N Teus S M 2021 12 15 Mobility of dislocations in the iron based C N H solid solutions measured using internal friction Effect of electron structure Journal of Alloys and Compounds 886 161260 doi 10 1016 j jallcom 2021 161260 ISSN 0925 8388 a b c d e f g h i j Marc Meyers Krishan Chawla 2009 Mechanical Behavior of Materials Cambridge UK Cambridge pp 569 570 ISBN 978 0 511 45557 5 a b Weller M 2006 12 20 The Snoek relaxation in bcc metals From steel wire to meteorites Materials Science and Engineering A Proceedings of the 14th International Conference on Internal Friction and Mechanical Spectroscopy 442 1 21 30 doi 10 1016 j msea 2006 02 232 ISSN 0921 5093 Hosford William F 2005 Mechanical behavior of materials Cambridge Cambridge University Press ISBN 0 521 84670 6 OCLC 56482243 Koiwa M 1971 09 01 Theory of the snoek effect in ternary b c c alloys The Philosophical Magazine 24 189 539 554 Bibcode 1971PMag 24 539K doi 10 1080 14786437108217028 ISSN 0031 8086 Retrieved from https en wikipedia org w index php title Cottrell atmosphere amp oldid 1102816842, wikipedia, wiki, book, books, library,

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