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DEFORM 和CAE软件在模拟金属塑性变形过程中的应用

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DEFORM - 2D 和DEFORM - 3D CAE 软件在模拟金属塑性变形过程中的应用

林新波

(上海交通大学 塑性成形工程系,上海 200030)



摘 要:介绍了塑性变形有限元分析软件 DEFORM 的模块结构,并通过实例分析介绍了此软件在应力 、应变分布、载荷计算、点的跟踪、模具填充、缺陷分析和缺陷预防等方面的应用。

关键词:DEFORM 软件: 有限元分析;塑性变形

中图分类号:TG113.25 + 3 文献标识码:A


Abstract : In (his paper , the nodule structure ot* DEFORM is described sinply. Some typical applications are an alyzed to dennnstrate the feasibility of DEFORM in simulating nietal plastic deformation such as the distribution of effective stress and effective strain ,calculation of load- 

stroke , tracing of point ,fill of nnuld, an alysis and prevention of defect.

Key words : DEFORM software ; FEM ana lysis;plastic deformation


0 引言

最近几年 .随着计算科学的快速发展和有限元技术应用的日益成熟 ,CAE技术模拟分析金 属在塑性变形过程中的流动规律在现实生产中得到愈来愈广泛的应用。6E技术的成功运用,不仅大大缩短了模具和新产品的开发周期 .降低了生产成本 .提高企业的市场竞争能力 ,而且有利于将有限元分析法和传统的实验方法结合起来 ,从而推动模具现代制造业的快速发展

1DEFORM 系统简介

DEFORM(Design environment for tbmiing) 是由美国Battelle Cblumbus 实验室在八十年代早期 着手开发的一套有限元分析软件。早期的DEFORM - 2D 软件只能局限于分析等温变形的平  面问题或者轴对称问题。随着有限元技术的日益成熟 QEP0RM 软件也在不断发展完善,目 前 DEFORM 软件已经能够成功用于分析考虑热力耦和的非等温变形问题和三维变形(DH FORM - 3D) .此外,DEHDRM 软件可视化的操作界面以及强大而完善的网格自动再划分技术, 都使 DEFORM 这一商业化软件在现代工业生产中变得愈来愈实用而可靠。

2DEFORM 软件的模块结构

DEPORM- 2D 和 DEFORM - 3D 的模块结构基本相同 .都由前处理器、模拟处理器和后处理器三大模块组成 ,不同的是 DEPDRM- 2D 自身可以制作简易的线框模具 .DEFORM- 3D 不具备实体造型能力,但它提供一些通用的 CAD 数据接口 .如 IGES 和 S1L 接口。

2.1 前处理器

前处理器包括三个子模块⑴数据输入模块 .便于数据的交互式输入 ,如 :初始速度场、温 度场、边界条件、冲头行程以及摩擦系数等初始条件。(2)网格的自动划分与自动再划分模块。 

(3)数据传递模块 ,当网格重划分后 ,能够在新旧网格之间实现应力 、应变 、速度场、边界条件等

数据的传递 .从而保证计算的连续性。

2.2 模拟处理器

真正的有限元分析过程是在模拟处理器中完成的,DERDRM 运行时 ,首先通过有限元离散化将平衡方程 、本构尧系和边界条件转化为非线形方程组.然后通过直接迭代法和 Neuton -

Raphson 法进行求解 .求解的结果以二进制的形式进行保存.用户可在后处理器中获取所需要的结果。

2.3 后处理器

后处理器用于显示计算结果 ,结果可以是图形形式 .也可以是数字、文字混编的形式。可获取的结果可为每一步的(1)有限元网格(;2)等效应力 、等效应变以及破坏程度的等高线和等色图; 速度场:⑷温度场; 压力行程曲线等。此外用户还可以列点进行跟踪 .对个别点的轨迹、应力 、应变 、破坏程度进行跟踪观察 .并可根据需要抽取数据。

3DEFOM - 2D 和 DEFORM - 3D 实例分析



3.1 徽粗

为了评估DEFORM - 2D 和DEFORM - 3D 的计算结果 ,现将一徽粗过程分别在2D 与 3D 平

台上进行模拟计算,虽然在网格划分上有些不同 .但两者在材料流动、应力 、应变分布、行程载荷方面的计算结果都显得十分吻合。

图 1 ,2 和图 3,4 分别为圆柱在DERORM - 2D 与 DEFORM - 3D 平台上的网格变形图(圆柱

起始高度 叩1)为 30,徽粗后 叩50)为 15).图 5,6 为应力分布等高线 周7,8 为应变分布等高线 .图 9 为各示意图等高线数据 .将图示形状和数据大小进行比较,如图 5 对应等高线 I数值为 1.7878,图 6 对应等高线B 数值为 1.7440,其结果非常接近。图 10 为 1/4 圆柱在3D 平台上的压力行程曲线,从图示可得最大载荷约为 6. 8t.图 11 为整个圆柱在 2D 平台上的压力行程曲线 .图示可得最大载荷约为 28t ,约为前者的 4 倍 .整个计算结果的比较都显得非常接近。

image.png

image.png

3.2 点的跟踪与缺陷分析

下面实例为一铝件的正向挤压模拟,实际生产中 .当变形量达到一定的程度 .在零件后端中心会出现凹状缩孔。

图 12 以有限元网格的形式显示了挤压过程中金属的流动情况 .在难变形区,网格会自动 进行重划分 ,在图示中可以明显观察到网格的畸变和重划分情况 ,整个变形过程共进行了 12 次网格自动重划分。 

图 13 则对配料表面三个点进行点的跟踪 ’当变形量达到一定程度时,可以明显观察到表面上的点开始向中心转移 .从而导致凹状缩孔的形成,从点的移动情况可以看出 .适当地控制变形量可以阻止缺陷的形成。

3.3 极爪零件的温徽成形

极爪是汽车发动机电极零件 .它的成形过程:首先将一圆形坯料温徽成形获取枝丫状毛坯,然后对枝丫进行剪切和弯曲 ,获取最终产品,其中 .将枝丫尺寸锹挤到位是成形的关键。由于变形体有 6 个爪 .且形状对称 .故只选取工件的 1/12 进行模拟。成形材料:08F 钢,初始坯料

尺寸:如. 4mm X21.6mni,冲头速度:120mm/ s ,温度 :700 ℃,摩擦系数:0.15 0

初始网格如图 14,它是由 DEPORM- 3D 自动生成的四面体单元网格,对变形剧烈的区域预先实行网格局部细化分,该网格包括 1 406 个节点和 5 678 个单元。

从变形过程网格的重划分情况(如图 15,16)可以看出 .材料的难变形区在模具的入口处, 在此处材料发生剧烈变形 .离开入口处后 .材料变形趋向均匀 .网格分布也比较均匀。另外 ,对毛坯变形过程的破坏程度进行分析 ,发现靠近枝丫末端处破坏因子较大且呈层状分布(如图 ,说明变形过程中 .上层的金属流动较下面的快.结果在金属内部形成拉应力 .随着变形程 度的加剧,拉应力增大 .破坏程度也随着增大 ,但是破坏因子的数值比较小,在 D 等高线处数值仅达到0.0760,尚不会引起裂纹。

image.png

4 结论

利用类似 DETORM 等有限元软件 .模拟分析金属的流动规律 .有利于帮助设计人员优化工艺参数和模具设计 .减少模具的前期开发费用 .其健壮而有效的有限元代码,方便而可行的前后模拟处理器,以及现在愈来愈快的工作站都大大减少了设计人员的工作量 ,从而有利于缩短模具的设计开发周期。

image.png

image.png

但是 ,对于一些复杂的工艺过程进行模拟时 .模拟.过程的计算量会很大.可达凡个星期甚至几个月 .有时这种模拟是很不经济的.为此 .可根据实际需要对模拟过程做适当的简化,以期在较短的时间内获取所需的主要信息。下面一些假设是在有限元模拟中常用的一些简化方法。

(I) 用等温变形代替非等温变形。这种假设能够获取基本数据 .常用于变形过程对温度变化不非常敏感的材料,如碳素钢等;另外,也适用于变形速度比较快 .模具冷却效果不明显的场合 ,如机械压力机锻造或者螺旋压力机锻造等。

(2)忽略模具上一些次要的几何特征。例如 ,忽略零件上定位槽的几何形状 ,不会对金属的流动产生明显的影响.但是 .这种简化却能大大减少计算时间以及网格重划分的次数。

(3)确定适当的网格数目 ,合理的分配网格密度。网格数目过多或者过少都不利于有限元的模拟计算 ,可根据零件变形情况 ,适当的预设定网格数目,并对变形剧烈的区域预先实行细划分 .可大大减少计算时间。

显而易见 .为了保证模拟过程的不间断性 .网格的自动划分与再划分技术 .网格密度分布的自动优化技术 ,以及新旧网格间数据的自动传递技术在有限元代码中是必需的。

参考文献:

[ 1 ] laylan Altan,Markus Knoerr. Application of the 2D Rnite Bement Method to Simulation of Cbld - Fbrgjng Piucesses

[J ]. Journal of Materials Pressing Technology ,1992 ,35 :275~302.

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The kinetic model accurately predicts our measured flame speeds and the non-premixed counterflow ignition temperatures determined in our previous study, as well as homogeneous system data from literature, such as concentration profiles from flow reactor and ignition delay time from shock tube experiments.◎ 2006 The Combustion Institute. Published by Elsevier Inc. All rights reserved.Keywords: Laminar flame speeds; Kinetics; Reaction mechanis m; CO–H2 oxidation1. IntroductionNext to H2, the oxidation of CO–H2 mixtures is perhaps the most important building block in the hierarchy of hydrocarbon oxidation. As a result, extensive investigations based on both homogeneous chemical systems, such as the shock tube and flow reactor, and inhomogeneous diffu- sive systems, such as the laminar flame speed and the counterflow ignition/extinction states, have been performed to determine this oxidation mechanis m comprehensively. 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Therefore, the low-pressure limit rate recommended by Troe [27] was adopted in our mechanism to model the experimental data considered herein.The reaction H + O2 + M → HO2 + M pro- vides another route for the conversion of CO to CO2 through CO + HO2 → CO2 + OH at high pressures or in the initial stages of CO oxidation [29]. However, the rate constant for CO + HO2 at temperatures above 800 K is limited to indirect determinations [30–33]. Atri et al. [33] reported this reaction rate as k = 5.97 × 1013 exp(_22.94 kcal/RT) cm3 mol__1 s__1 based on their results from thermal reactions at 713– 773 K. Volman et al. [34] theoretically investigat- ed the reaction of CO + HO2 using ab initio CISD calculations based on unrestricted Hartee–Fock (UHF) optimized geometries. Their calculated activation energy is in agreement with that from Atri et al. [33], and as such a rate constants at 250–800 K based on the rate constant of Atri et al. [33] and the hard-sphere-collision Arrhenius modification was recommended [37]. However, the practical applications support the lower reac- tion rate above 1000 K, and a 50% reduction of the rate by Atri et al. [33] has been used in the development of reaction mechanisms [10,11,35]. To further investigate this reaction rate, we per- formed high-level ab initio calculations with Gaussian [36]. We follow the reaction mechanism as proposed by Volman [37], with the first stage in the reaction being the formation of a free radical intermediate HO2 + CO → HOOC . O which then decomposes to yield the products, and with the rate of formation of the intermediate equal to the formation of the products. The calculated acti- vation energies for the formation of the intermedi- ate are 16.82, 17.18, 17.02, 17.81, 16.73, and 16.11 kcal/mol at the G2, G2(MP2), G3, G3(MP2), CBS-QB3, and CBS-Q levels, respec- tively, which shows that different ab initio meth- ods are in good agreement. By evaluating the forward/reverse barriers and heats of reaction, we found that the G3(MP2) energies can better characterize the potential energy surface of CO + HO2. Because the calculated heat of reaction based on the G3(MP2) energies (_62.89 kcal/mol) is closer to the value derived from currently accepted ΔH98 values (_61.91 kcal/mol), and an activation energy of 17.81 kcal/mol based on the G3(MP2) calculation is closer to the experimentally obtained value (22.94 kcal/mol) [33]. By using the MP2(full)/6- 31G(d,p) optimized geometries and canonical transition state theory, we calculated this rate con- stant to be k = 1.15 × 105 T2.278exp(_17.55 kcal/ RT) cm3 mol__1 s__1 at 300–2500 K, and this is the rate used in our reaction mechanism.4. Results and comparisons4.1. Laminar flame speedsThe measured laminar flame speeds for CO/ H2/air and CO/H2/O2/helium mixtures as a func- tion of equivalence ratio at different mixing ratios for pressures of 1, 2, 5, 10, 20, and 40 atmospheres are shown in Figs. 1 and 2, with comparisons to measured data from literature and also to calcu- lated flame speed data using different mechanisms. The measured flame speeds increase with increas- ing H2 content in the CO/H2 mixtures, while they decrease with increasing pressure for the helium-diluted mixtures. For the air-diluted mixture of CO:H2 = 95:5, our measured flame speed data are slightly lower (2–6 cm/s) than those of McLean et al. [3]. As shown in Fig. 1, our mea- sured flame speed data for the mixture of CO:H2 = 50:50 at atmospheric conditions show excellent agreement with those of Faeth et al. [2] for fuel-lean conditions; the maximum value in the curve is ca. 7 cm/s lower than that of McLean et al. [3], but they show agreement with the data of McLean et al. [3] at fuel-rich conditions.Fig. 1. Measured and calculated laminar flame speeds vs. equivalence ratio for different CO/H2/air mixtures at 1 and 2 atmospheres. Solid line, model from this work; dashed line, model from Davis et al. [11], dotted line: model from Li et al. [10].Fig. 2. Measured and calculated laminar flame speeds vs. equivalence ratio for different CO/H2/He/O2 mix- tures at 5, 10, 20, and 40 atmospheres. Solid line, model from this work; dashed line, model from Davis et al. [11].Overall, the model predictions using our mech- anism agree very well with our experimental data at different fuel concentrations and pressures. The calculated flame speeds using the mechanism of Li et al. [9] show good agreement with the data of McLean et al. [3], but it over-predicts our mea- sured flame speed data at rich conditions. The cal- culated flame speeds from the optimized mechanism of Davis et al. [11] show close agree- ment with our experimental results at pressures of 1–5 atmospheres, but the discrepancy increases at fuel-rich condition when the chamber pressure is above 5 atmospheres. Our model predictions show much better agreement than those from the optimized model at higher pressures even though a discrepancy of 4–5 cm/s still exists.However, for these fast flames, such a discrepancy is within the error range of the experiment. Because we used ultra high purity grade fuels and certified oxygen/nitrogen in our experiments, and had a very good vacuum procedure, trace amount of water, if any, should be in the ppm range. Such small amount of water should have negligible effect on the flame speeds, especially giv- en that the CO used already has hydrogen added as an ‘‘impurity’’ as compared to pure CO, which would be very sensitive to even trace amount of water. The satisfactory performance of our model is ascribed to the accurate elementary rate con- stants for the nature of fundamental reaction mechanism. As the laminar flame propagation rate is determined by chemical reaction rates and heat release, which are coupled with heat conduc- tion and molecular diffusion, this discrepancy could be the results of both kinetic and transport uncertainties.4.2. Counterflow ignition temperaturesIgnition temperatures provide good target points for the testing of kinetic mechanisms in the moderate temperature regime. Figure 3 com- pares the calculated counterflow ignition tempera- tures from different models with our previous experimental data at atmospheric pressure [5]. Our model prediction is very close to that of Davis et al. [11] at lower H2 concentrations, and close to that of Li et al. [10] at higher H2 concentrations. Overall, the prediction of our model shows much closer agreement with the experimental data than other models. Figure 4 compares the calculated ignition temperatures as a function of pressure with the experimental data at strain rates of 100 s__1 for 5% H2 in CO [5]. The calculated igni- tion temperatures show very good agreement with the experimental data [5] over the entire experi- mental pressure range, while the predictions fromFig. 3. Comparison of calculated ignition temperatures vs. H2 concentration with the experimental data at atmospheric conditions with the strain rate of 100 s .Fig. 4. Comparison of calculated ignition temperatures vs. pressure with the experimental data at the strain rate of 100 s__1 for 5% H2 in CO.the other mechanisms [8,11] are either within or beyond the experimental error limit (±15 K) at both lower and higher pressures. A sensitivity an alysis indicated that the reactions of H + O2 = O + OH, O + H2 = H + OH, H + HO2 = OH + OH, H2 + O2 = HO2 + H, and CO + OH = CO2 + H are the most important for the prediction of ignition temperatures around 900 K at pressures lower than 0.3 atmospheres. Our satisfactory predictions strongly support the accuracy of the rate constants used in the current model.4.3. Flow reactor and shock tube dataAdiabatic flow reactor and shock tube experi- ments provide well-characterized environments that minimize mixing and diffusion effects, and are therefore very well suited for detailed chemical kinetic modeling. Because the modeling uncertain- ties in flow reactor are relatively large, it is com- mon to shift the simulated values along the time axis to match the 50% fuel consumption [9,12,38]. Dryer et al. [35,38,39] recently per- formed several H2/O2 and CO/H2 studies utilizing these configurations. They indicated that the reac- tion of H + HO2 → OH + OH is a dominant reaction pathway in their flow reactor and kinetic modeling study of H2–O2 reaction [38]. However, there are a few rate data in the higher temperature range and the scatter is large. They estimated this rate constant as k = 7.08 × 1013 exp(_0.3 kcal/ RT) cm3 mol__1 s__1 to model the H2, O2, and H2O reaction profiles in their flow reactor experiment. Our mechanism supports a slightly lower rate for this reaction: k = 6.0 × 1013 exp(_0.3 kcal/RT) cm3 mol__1 s__1. After incorpo- rating this modified rate constant and the afore- mentioned time shifting technique, our mechanism predictions yields very close agree- ment with the experimental reaction profiles for both H2/O2/N2 and CO/H2O/O2/N2 mixtures at atmospheric pressure, as shown in Figs. 5 and 6. Furthermore, because this reaction is also domi- nant in modeling the global combustion parame- ters of flame speed and ignition temperature, the good agreements between our model and our combustion experiments provides further support for the accuracy of this modified reaction rate.Fig. 5. Comparison of calculated and experimental reaction profiles of H2/O2/N2 mixtures in an atmospher- ic pressure flow reactor. Symbol, Muller et al. [8].Fig. 6. Comparison of calculated and experimental reaction profiles of CO/H2O/O2/N2 mixtures in an atmospheric pressure flow reactor. Symbol, Yetter et al. [39]. (a) Model prediction was time shifted by 0.003 s. (b) Model prediction was time shifted by 0.04 s.As indicated above, the reaction of CO + HO2 is another important route for CO consumption at higher pressures, and as such, our model predicts the CO consumption rate well at elevated pres- sures of 1, 2.4, and 9.6 atmospheres [8] even with- out a time shift. When using the rate from Mueller et al. [8] in our model, the predicted CO concen- tration at 9.6 atmospheres shows a larger discrep- ancy with the experimental data at longer reaction times as shown by the dashed line in Supplemental material (Fig. S1). The good agreement between the experiment and our model supports the accu- racy of the CO + HO2 rate constant based on our theoretical calculations. Our model also shows satisfactory agreement for the shock tube ignition time delays [40], as shown in Fig. S2.5. Concluding remarksExperimental laminar flame speeds were accu- rately measured for CO/H2/air and CO/H2/O2/ He mixtures at different equivalence ratios and mixing ratios up to 40 atmospheres using the con- stant-pressure spherical flame technique. The reaction rate constant of CO + HO2 → CO2 + OH was calculated based on ab initio theo- ry and canonical transition state theory. A kinetic mechanism based on recently published and calcu- lated rate constants is presented to model the mea- sured laminar flame speeds as well as the experimental data from counterflow ignition, flow reactor, and shock tube experiments in the litera- ture. The comparison between the modeling results and the laboratory measurements suggests that the accuracy of the thermochemical data and the elementary rate constants is crucial for a satis- factory performance of the reaction mechanism.AcknowledgmentsThis work was supported by the Air Force Of- fice of Scientific Research and the Army Research Office, under the technical monitoring of Drs. Ju- lian Tishkoff and Kevin McNes by, respectively.Appendix A. Supplementary dataSupplementary data associated with this article can be found in the online version at doi:10.1016/ j.proci.2006.07.193.References[1] M.J. Brown, I.C. Mclean, D.B. Smith, et al., Proc. Combust. Inst. 26 (1996) 875–881.[2] M.I. Hassan, K.T. Aung, G.M. Faeth, J. Prop. 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Ryu, K.J.D. Witt, et al., Chem. Phys. Lett. 408 (1–3) (2005) 107–111.[24] C. Kappel, K. Luthe, J. Troe, Phys. Chem. Chem. Phys. 4 (2002) 4392–4398.[25] J.C. Michael, J.W. Sutherland, L.B. Harding, et al., Proc. Combust. Inst. 28 (2000) 1471–1478.[26] M.S. Wooldridge, R.K. Hanson, C.T. Bowman, Proc. Combust. Inst. 25 (1994) 741–748.[27] J.R. Troe, Proc. Combust. Inst. 27 (1998) 167–175.[28] D. Fulle, H.F. Hamann, H. Hippler, et al., J. Chem. Phys. 105 (3) (1996) 983–1000.[29] I. Glassman, Combustion, Academic, San Diego, CA, 1996.[30] J. Vandooren, L. Oldenhove de Guertechin, P.J. van Tiggelen, Combust. Flame 64 (1986) 127–139.[31] I.A. Vardanyan, G.A. Sachyan, A.B. Nalbandyan, Int. J. Chem. Kinet. 7 (1975) 23.[32] M.B. Colket III, D.W. Naegeli, I. Glassman, Proc. Combust. Inst. 16 (1977) 1023.[33] G.M. Atri, R.R. Baldwin, D. Jackson, et al., Combust. Flame 30 (1977) 1–12.[34] T.L. Allen, W.H. Fink, D.H. Volman, J. Phys. Chem. 100 (13) (1996) 5299–5302.[35] M.A. Mueller, R.A. Yetter, F.L. Dryer, Int. J. Chem. Kinet. 32 (6) (2000) 317–339.[36] M.J. Frisch et al., Gaussian 03, Gaussian Inc., Pitts burgh PA, 2003.[37] D.H. Volman, J. Photochchem. Photobiol. A: Chem. 100 (1–3) (1996) 1–3.[38] M.A. Mueller, T.J. Kim, R.A. Yetter, et al., Int. J. Chem. Kinet. 31 (2) (1999) 113–125.[39] R.A. Yetter, F.L. Dryer, H. Rabitz, Combust. Sci. Technol. 79 (1-3) (1991) 129–140.[40] A.M. Dean, D.C. Steiner, E.E. Wang, Combust. Flame 32 (1978) 73–83.[41] N. Cohen, K.R. Westberg, J. Phys. Chem. Ref. Data 12 (3) (1983) 531–590.[42] W. Tsang, R.F. Hampson, J. Phys. Chem. Ref. Data 15 (1986) 1087–1279.[43] H. Hippler, J. Troe, J. Willner, J. Chem. Phys. 93 (3) (1990) 1755–1760.[44] H. Hippler, H. Neunaber, J. Troe, J. Chem. Phys. 103 (9) (1995) 3510–3516.[45] R.R. Baldwin, D. Jackson, A. Melvin, et al., Int. J. Chem. Kinet. 4 (1972) 277.[46] G. Friedrichs, J.T. Herbon, D.F. Davidson, et al., Phys. Chem. Chem. Phys. 4 (23) (2002) 5778–5788.[47] D.L. Baulch, C.J. Cobos, R.A. Cox, et al., J. Phys. Chem. Ref. Data 21 (3) (1992) 411–429.[48] C.-C. Hsu, A.M. Mebel, M.C. Lin, J. Chem. Phys. 105 (6) (1996) 2346–2352.CommentsJohn Griffiths, University of Leeds, UK. It is very interesting to see your revision of the rate parameters for the reaction HO2 + CO. This agrees with our under- standing that the reaction should be slower than is pre- dicted by the parameters from Mueller et al. The values you give would put the distribution of the predicted igni- tion delay in Fig. 4 of our preceding paper (Mittal et al.) at a position corresponding to logA = _10.9, which isclose to our expectations.Steve Klippenstein kindly did some transition state theory calculations for us after our paper was accepted, which also lead to a lower rate constant. He gave two functions, one based on a single activation barrier and another based on a double activation barrier.The data are as follows.TST1: k = 2.703 × 10__20 . T2.482 . exp(__8472/T) cm3 molecule__1 s__1TST2: k = 1.149 × 10__17 . T1.609 . exp(__8805/T) cm3 molecule__1 s__1Reply. We are pleased to see that your experimental observation supports our theoretical rate constant for the CO + HO2 reaction. We have, in addition, found that the first function of the CO + HO2 rate constant by Klip- penstein is only a factor of0.8lower than our recommend- ed rate constant within the temperature range of 800– 2500 K. Furthermore, our QRRK-master equation an al- ysis indicated that the forward rate constant to products based on our double activation barriers as presented at the meeting is also consistent with Klippenstein’s second function of the CO + HO2 rate constant.●Anthony Dean, Colorado School of Mines, USA. For your calculated value of k for CO + HO2 = CO2 + OH, why was it necessary to assume that the product forma- tion was the same as the rate of formation of the inter- mediate complex?Reply. This is a very good question. This rate constant based on double activation barriers is about a factor of 1.1–1.7 (T = 300–2500 K) lower than that based on a single activation barrier, since the second barrier is only few kcal/mol, so our calculated k using the assumption presents this rate constant very reason- ably, and it does not contain errors introduced from the uncertainties of parameters used in QRRK-master equation an alysis.●John Simmie, National University of Ireland, Ireland. You are to be congratulated for comparing your exper- iments against three mechanisms and not just your own. But what are the essential differences between them that make yours better—is it the chemistry and/or the trans- port properties?Reply. Since the comparison was conducted for dif- ferent reaction mechanisms, but basically the same transport properties, it is reasonable to infer that it is the revised rates that affected the difference.●Ken Brezinsky, University of Illinois at Chicago, USA. I was surprised to see that you were using Dean’s shock tube ignition delay data from 1978 (in paper). Is there no other shock tube ignition delay data for you to model?Reply. We used Dean’s shock tube data because it is a widely cited source. The most recent shock tube data are those by Petersen et al. [1]. We have now compared our calculated values against their data for 5 sets of fuel-lean (φ = 0.5) CO/H2/air mixtures for 890 K < T < 1285 K and pressure near 1 atm, and found fairly good agreement.Reference[1] D. Kalitan, E. Petersen, AIAA-2005-3767, 41st AIAA/ASME/SAE/ASEE Joint Propulsion Confer- ence and Exhibit, Tucson, Arizona, 2005.免责声明:本页面/内容部分素材来源于互联网公 开 信 息,旨在传递更多信息,不代表本平台立场。版权归原作者或机构所有,如涉及侵权,请通过平台联系我们,我们将在核实后第一时间处理。本平台对转载内容的真实性、准确性不作任何保证,用户需自行判断并承担使用风险。

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