CARBOTHERMIC REDUCTION OF OXIDES DURING NITROGEN SINTERING OF MANGANESE AND CHROMIUM STEELS

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Powder Metallurgy Progress, Vol.4 (004), No 3 13 CARBOTHERMIC REDUCTION OF OXIDES DURING NITROGEN SINTERING OF MANGANESE AND CHROMIUM STEELS S. C. Mitchell, A. Cias Abstract To interpret nitrogen sintering of chromium manganese steels without the formation of deleterious oxides, but with manganese carbon modifying the local microclimate, the role of the volatile Mn carbothermic reactions were considered. Reduction of Cr O 3 by Mn vapour is always favourable. CO is an effective reducing agent, however, whereas at atmospheric pressure it will reduce FeO at ~730 C, temperatures some 500 700 C higher, i.e. above those for conventional sintering, are necessary for reducing Cr O 3 MnO, respectively. Accordingly partial pressures must be considered the sintering process is modelled at a conglomerate of several surface oxidised alloy particles surrounding a pore with graphite present a tortuous access to the nitrogen-rich atmosphere containing some water vapour oxygen. The relevant partial pressures were calculated reduction reactions become thermodynamically favourable from ~00 C. Kinetics, however, dictates availability of CO the relevant reactions are the water-gas, C + H O = CO + H from ~500 C the Boudouard, C + CO = CO, from ~700 C. Discussion of sintering mechanisms is extended to processing in semi-closed containers, also possessing specific microclimates. Keywords: PM chromium manganese steels, nitrogen sintering, carbothermic reduction of oxides INTRODUCTION Šlesár et al, who have recently reexamined sintering of Fe-C [1], noted the critical importance of its initial stages, including removal of particle surface oxides, formation of sinter necks, dissolution of carbon, pore elimination density development. They conducted isothermal sintering experiments in the temperature range 600-100 C complemented these with EDX, tensile testing, micrography fractography. Kremel et al [] went on to examine Astaloy CrM-C sintered in N -0% H with additional dilatometric/degassing experiments. The importance of carbothermic reactions was stressed general correlations with reducing reactions proposed. Most recently Bocchini [3], when reviewing controlled atmospheres in the proper sintering of carbon steels, considered equilibrium constants of relevant reactions, including those between CO H O, C CO CO H O. Concurrently Mitchell et al [4-13] examined Fe-Cr-Mn-Mo-C systems, including sintering in nitrogen in semi-closed containers, with special reference to the volatile Mn [14], as shown in Table 1 Fig.1, as well as carbothermic reactions. It is also to be noted [15] that Mn + H O = MnO + H gas. Stephen C. Mitchell, Engineering Materials Group, University of Bradford, U.K. Andrzej Cias, Faculty of Metallurgy Powder Metallurgy, University of Mining Metallurgy, Krakow, Pol.

Powder Metallurgy Progress, Vol.4 (004), No 3 133 Tab.1. Calculated equilibrium partial pressure of Mn vapour versus temperature, as reported by Barin [16,17]. Temperature [ C] Mn Vapour Pressure (Atmospheres) 0 1.65E-47 100 5.36E-33 00 1.E-4 300 3.E-19 400.0E-15 500 1.8E-1 600 1.81E-10 700 9.06E-09 800.09E-07 900.78E-06 1000.4E-05 Fig.1. Manganese vapour equilibrium partial pressure showing its substantial increase from ~740 C (Note: Due to graph scaling resolution there is the illusion that vapour pressure is zero below ~680 C. See data in Table 1). Fig.. Reducing partial pressures of CO in pore or semi-closed container in relation to Fe, Cr Mn oxides, as a function of temperature.

Powder Metallurgy Progress, Vol.4 (004), No 3 134 On examination of thermodynamics of reduction reactions involving metal oxides on alloy powder particles, it is evident that, Fig., whereas CO at atmospheric pressure will reduce FeO at ~730 C, temperatures some 500 700 C higher than those for conventional sintering are necessary for reduction of Cr O 3 MnO, respectively. It should be recalled that the sintering pressure is usually just above 1 atmosphere the predominant partial pressures are usually of nitrogen hydrogen. Accordingly for proper analysis of the relevant reactions, partial pressures must be considered Fig. illustrates the effect of reducing the partial pressure of the C + O reaction by 1, 3 orders of magnitude. Accordingly sintering will be modelled for a conglomerate of several surface oxidised alloy powder particles surrounding a pore with graphite present tortuous access to nitrogen-rich atmosphere containing some water vapour oxygen. Theoretical calculations involve use of several algorithms for calculating reaction energies [18,19] the availability of HSC Chemistry for Windows [19] allows, in some instances, speedy theoretical calculations. The enthalpy, H, entropy, S heat capacity, Cp data used for the HSC calculations are taken from the most reliable recent sources available should therefore be more consistent with external (absolute) scales. This ensures that the accuracy is adequate for most thermo-chemical calculations. REDUCTION OF OXIDES WITH SOLID CARBON Assumptions: total pressure is ~ 1 atmosphere nitrogen is inert at sintering temperature. If FeO, Cr O 3 MnO are to be reduced by solid carbon, then the maximum pressure of active gases which can be tolerated in the system can be calculated at absolute temperature T, by considering free enthalphy changes ΔG o, where Kp is the equilibrium constant. Temperatures chosen, with reference to Fig., were: 740 C (1013 K), also considered by Danninger et al [1,], for FeO, 1100 C for Cr O 3 1140 C for MnO. The following reactions will be considered: FeO (s) = Fe (s) + 0.5O (g) ΔG o = 6050 14.95T calories (1) 1/3Cr O 3 (s) = /3Cr (s) + 0.5O (g) ΔG o = 8950 0.7T calories () MnO (s) = Mn (s) + 0.5O (g) ΔG o = 91950 17.31T calories (3) : C (s) + O (g) = CO (g) ΔG o = -9400 0.0T calories (4) C (s) + O (g) = CO (g) ΔG o = - 53400 41.9T calories (5) CO (g) + O (g) = CO (g) ΔG o = - 135000 + 41.50T calories (6) C (s) + CO (g) = CO (g) ΔG o = + 40800 41.70T calories (7) Iron Oxide ΔG o 1013 = 46905.65 calories = - (1.987 x ln10) x 1013 log K p Therefore logk p = 46905.65/(-4.575 x 1013) = -10.11 But K p = P 0.5 O (eq,t)

Powder Metallurgy Progress, Vol.4 (004), No 3 135 so log PP = x 10.11 = -0.4 O (eq,1013) Therefore PP = 5.73 x 10-1 atmospheres. O (eq,1013) If it is considered that C is reducing FeO to form Fe + CO, then the pertinent reaction is : FeO (s) + C = Fe + CO, for which where Thus so: ΔG o = 35350 35.9T calories = -RTlnK p = -1016.7 Kp = P CO(eq,T) ΔG o 1013 = -1016.7 calories = -4.575 x 1013 log P CO (eq,1013) log P CO(eq,1013) = 0.1938 P CO(eq,1013) = 1.657 atmospheres. This implies that for reduction of FeO to proceed spontaneously, CO pressure must be less than 1.657 atmospheres. If CO is in equilibrium with solid C, then a CO pressure must be exerted by: C + CO = CO for which: C (s) + CO (g) = CO (g) ΔG o = + 40800 41.70T calories = -RTlnK p = -144.1 (7) where K p CO ρ = CO ρ eq, T Thus ΔG o 1013 = -144.1 calories = - 4.575 x 1013 log K p or Hence log ρ CO ρco eq,1013 = 0.311 log P CO = log P CO - 0.311 = ( x 0.1938) - 0.311 = 0.1759 P CO(eq,1013) = 1.34 atmospheres. Thus, if the reaction is considered to be FeO + 0.5C = Fe + 0.5CO then the CO pressure must be lower than 1.34 atmospheres. For this reaction ΔG o = + 14950 15.05T calories = - 95.65 = -RTlnK p

Powder Metallurgy Progress, Vol.4 (004), No 3 136 where Kp = P 0.5 CO (eq,t) Thus ΔG o = -95.65 calories = - 4.575 x 1013 log P 0.5 1013 CO (eq,t) From which log P CO(eq,873) = 0.1759 or P CO(eq,1013) = 1.34 atmospheres, in full agreement with the above. CO CO, which are in equilibrium with the solid C, give rise to an oxygen pressure via the equilibrium reaction CO (g) + O (g) = CO (g) for which where ΔG o = - 135000 + 41.50T calories =-RTlnK p. (6) K p ρ = ρ CO CO ρ o eq, T ΔG o = - 9960.5 calories hence log ρ CO = 0.05847 ρ CO ρo Thus so eq,1013 log P O = log P CO log P CO 0.05847 = ( x 0.1756) - ( x 0.194) 0.05847 = -0.4 P O (eq, 1013) = 5.7 x 10 1 atmospheres, in agreement with above. This tells us that at 1013K, for FeO, Fe C to be in equilibrium with a gaseous atmosphere, this atmosphere must be of composition: P CO = 1.65 atmospheres P CO = 1.34 atmospheres P O = 5.7 x 10 1 atmospheres,, if the total pressure of the reactive gases is less than 1.65 + 1.34 =.99 atmospheres, then spontaneous reduction of FeO will occur. At equilibrium at 1013 K, the P CO /P CO ratio in the atmosphere is 1.65/1.34 = 1.3. It should be stressed, however, that the principal constituent of the ~ 1 atmosphere is nitrogen that equilibrium is not attained. In reality the partial pressure of CO is considerably lower. The P CO /P CO ratio, however, noting that due to the Boudouard reaction converting CO to CO, this ratio will be at least equal to, or probably larger than, 1.3. Chromium Oxide ΔG o 1373 = 8950 0.7T calories = -RTlnK p () Therefore log K p = 6089/(-4.575 x 1373) = -9.684

Powder Metallurgy Progress, Vol.4 (004), No 3 137, following the methodology for iron oxide, above: p O(eq,1373) = 4.3 x 10-0 atmospheres. If it is considered that C is reducing Cr O 3 to form Cr + CO, then the pertinent reaction is : 1/3Cr O 3 (s) + C = /3Cr + CO for which ΔG o = 8950 0.7T calories () -6700-0.9T 1/ of (5) = 6550-41.6T = -RTlnK p i.e. ΔG o 1373 = 5433 calories = -4.575 x 1373 log P CO (eq,1373) P CO(eq,1373) = 0.136 atmospheres. This says that for reduction of Cr O 3 to proceed spontaneously at 1373K that CO pressure must be less than 0.136 atmospheres. If CO is in equilibrium with solid C: C + CO = CO (7) ΔG o 1373 = - 16454 calories = - 4.575 x 1373 log K p or log ρ CO =.6 ρco eq,1373 i.e. P CO(eq,1373) = 0.000045 atmospheres. Thus if the reaction is considered to be 1/3Cr O 3 (s) = /3Cr (s) + 0.5O (g) then the CO pressure must be lower than 0.000045 atmospheres. For this reaction ΔG o = + 8950 0.70T calories = -RTlnK p - 47100-0.10T 1 mole of C 1/ of (4) + 4150-0.8T Calories = -RTlnK p. Resultant formula P CO(eq,1373) = 0.000047 atmospheres, in full agreement with the above. For CO CO in equilibrium with the solid C at 1373K: ΔG o = - 7800 calories = -4.575 x 1373log K 1373 p hence P O (eq, 1373) = 4.4 x 10 0 atmospheres, in close agreement with above. This tells us that, at 1373K for Cr O 3, Cr C to be in equilibrium with a gaseous atmosphere, this atmosphere must be of composition P CO = 0.1365 atmospheres P CO = 0.00005 atmospheres. P O = 4.4 x 10 0 atmospheres,, if the total pressure of the reactive gases is less than 0.1365 + 0.00005 = 0.13655 atmosphere, spontaneous reduction of Cr O 3 will occur.

Powder Metallurgy Progress, Vol.4 (004), No 3 138 =.7 x 10 3. At equilibrium at 1373K, the P CO /P CO ratio in the atmosphere is 0.1365/0.00005 Manganese Oxide ΔG o 1413 = 91950 17.31T calories = -RTlnK p (3) Therefore at 1413K log K p = 67491/(-4.575 x 1413) = -10.44, following the methodology for iron chromium oxides, above: PP = 1.3 x 10-1 atmospheres. O (eq,1413) If it is considered that C is reducing MnO to form Mn + CO then the pertinent reaction is: MnO (s) + C = Mn + CO for which ΔG o = 91950 17.31T calories (3) 1413-6700 - 0.9T 1/ of (5) = 6550-38.1T = -RTlnK p P CO(eq,1413) = 0.018 atmospheres. This says that for reduction of MnO to proceed spontaneously at 1413K that CO pressure must be less than 0.018 atmospheres. If CO is in equilibrium with solid C CO ΔG o = + 40800 41.70T calories = -RTlnK p (7) P CO(eq,1413) = 0.0000005 atmospheres. Thus if the reaction is considered to be MnO (s) = Mn (s) + 0.5O (g) then the CO pressure must be lower than 0.0000005 atmospheres. For this reaction ΔG o = + 91950 17.31T calories (3) - 47100-0.1T 1 mole of C 1/ of (4) + 44850-17.41T Calories = -RTlnK p. Resultant formula P CO(eq,1413) = 0.00000055 atmospheres, in full agreement with the above. CO CO, which are in equilibrium with the solid C, give rise to an oxygen pressure via the equilibrium CO (g) + O (g) = CO (g) (6) for which ΔG o = - 135000 + 41.50T calories =-RTlnK p (6) log P O = ( x 6.6) - ( x -1.74) 11.81 = -0.85 P O (eq, 1413) = 1.41 x 10 1 atmospheres, in close agreement with above. This tells us that, at 1413K for MnO, Mn C to be in equilibrium with a gaseous atmosphere, this atmosphere must be of composition: P CO = 0.018 atmospheres

Powder Metallurgy Progress, Vol.4 (004), No 3 139 P CO = 0.00000055 atmospheres P O = 1.41 x 10 1 atmospheres,, if the total pressure of the reactive gases is less than 0.018 + 0.00000055 = 0.0180055 atmospheres, then spontaneous reduction of MnO will occur. At equilibrium at 1413 K, the P CO /P CO ratio in the gas is 0.018/0.00000055 = 33.1 x 10 3. DISCUSSION In extending the processing analysis of Mn steels to Cr-Mn alloys in nitrogen, it is necessary to consider the reaction of Cr O 3 with Mn vapour. Figure 3 shows that it is always favourable accordingly the availability of Mn (determined by its vapour pressure, Fig.1, Table 1) will be controlling. Useful reaction rates are expected from ~ 700 C. Similarly carbon can always be converted to CO (Fig.4). Fig.3. The thermodynamically favourable reduction reaction of chromium oxide by manganese vapour. Fig.4. The (permanently) thermodynamically favourable conditions for formation of carbon dioxide from solid carbon.

Powder Metallurgy Progress, Vol.4 (004), No 3 140 In an EU Copernicus project [6] 3 % Mn - 0.6 % C steel specimens, covered only by alumina powder, were sintered at 1140 C in flowing 75 % hydrogen/5 % nitrogen, with a dewpoint of -60 C. It was noted that the specimens showed a dull, oxidised surface, but that the internal microstructure was free of oxides. If one considers that the inter-connected porosity is best represented by a tortuous path, then it follows that the flowing atmosphere can only have limited effect on the climate within the central pores have greater effect at the surface. The inner pores then can be represented as individual semi-closed containers. For equilibrium the CO/CO ratio will vary dramatically with temperature due to the Boudouard reaction the partial pressure of CO will be in balance with the partial pressure of oxygen CO. It has now been shown that in the atmosphere of predominantly nitrogen, the reduction reactions for Fe, Cr, Mn become thermodynamically favourable from ~00 C, inconsistent with experimental observations. Kinetics, essentially availability of CO, needs to be considered the two relevant reactions are the water-gas: C + H O = CO + H (see Fig.5), effective from ~450 C, the Boudouard, C + CO = CO (see Fig.6), effective from ~700 C. Fig.5. The carbon-water vapour reaction becoming thermodynamically favourable at ~450 C. Fig.6. The Boudouard reaction becoming thermodynamically favourable at ~700 C. Any water vapour in the furnace atmosphere is quickly consumed by the reaction C+H O = H (g)+co(g) this small amount of hydrogen becomes available for reduction of iron oxide during the heating cycle. The oxygen in the atmosphere is consumed by the

Powder Metallurgy Progress, Vol.4 (004), No 3 141 reaction C(s)+O (g)=co (g) on reaching ~600 C the CO is rapidly reduced by carbon to form CO according to the Boudouard reaction. It must be remembered that the furnace atmosphere is largely composed of nitrogen hence the combined partial pressure of the carbonaceous gases is considerably less than 1 atmosphere. This affects the equilibrium ratio pco/pco at given oxygen potential temperature - to favour reduction of difficult oxides (e.g. Cr Mn) at lower temperatures than would be the case for pure CO. From the calculations it can be seen that at temperatures above 900 C the amount of CO is negligible hence the total pressure of carbonaceous gases is approximately equal to the partial pressure of CO. The amount of CO is negligible below ~500 C, so that the reverse must apply. It is well established that graphite reacts directly with both oxygen water vapour - to both dry the atmosphere reduce the amount of available oxygen [0,1]. Also manganese vapour reacts with both oxygen water [10,15,0] to dry the atmosphere generate additional hydrogen, which is then available for early reduction of iron oxides. As the temperature rises, the Boudouard reaction becomes the principal agent in reducing manganese chromium oxides due to the conversion of CO to CO, which improves the CO/CO ratio. The partial pressure of CO, as stated above, is proportional to the oxygen partial pressure, which has been lowered dramatically, hence favourable conditions for reduction have been generated on a local basis [microclimate]. By use of a semi-closed container all the above advantages are retained, but with the extra bonus that surface oxidation is also reduced, because the flowing atmosphere can no longer easily interact with the components' surfaces. It is also relevant to point out that it has long been known that, at a liquid metal/solid interface, 1 % MnO can be ideally dissolved into liquid iron [1]. Now, interrupted quench sintering experiments [] indicate that transient liquid phase exists locally inside Fe/Mn/C compacts, as pores are always larger than the size of the starting manganese donor powder that the pore morphology shows significant internal smoothing. This alloying reduces the thermodynamic activity of manganese dramatically allows reduction of oxides at much lower temperatures higher oxygen partial pressure than would otherwise be the case. CONCLUSIONS Thermodynamic calculations [for an atmosphere predominantly of nitrogen] were carried out for reduction of FeO, Cr O 3 MnO by solid carbon at 740, 1100 1140 C, respectively. The analyses derive the maximum pressures of O, CO CO which can be tolerated in the system also the P CO /P CO ratios. For the oxide of iron it evaluates to 1.3, of chromium to.7 x 10 3 of manganese to 33 x 10 3 with CO partial pressures being 1.65, 0.1365 0.018 atmospheres, respectively. Thermodynamics thus indicates favourable conditions for carbothermic reduction of oxides of iron, chromium manganese at conventional sintering temperatures. Equilibrium, however, is then not attained the reactions kinetics of production of CO were considered. The critical reactions were identified as C + H O = CO + H, effective from ~450 C, the Boudouard, C + CO = CO, effective from ~700 C. Additionally it was shown that from ~700 C there is ready availability of manganese vapour to encourage the direct reduction of chromium oxide earlier in the sintering process than would normally be expected when only the carbothermic reduction mechanism is available.

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