di Stasio Stefano, Konstandopoulos Athanasios G, Kostoglou Margaritis
Istituto Motori C.N.R. Via Marconi 8, Napoli, 80125, Italy.
J Colloid Interface Sci. 2002 Mar 1;247(1):33-46. doi: 10.1006/jcis.2001.8095.
The agglomeration kinetics of growing soot generated in a diffusion atmospheric flame are here studied in situ by light scattering technique to infer cluster morphology and size (fractal dimension D(f) and radius of gyration R(g)). SEM analysis is used as a standard reference to obtain primary particle size D(P) at different residence times. The number N(P) of primary particles per aggregate and the number concentration n(A) of clusters are evaluated on the basis of the measured angular patterns of the scattered light intensity. The major finding is that the kinetics of the coagulation process that yields to the formation of chain-like aggregates by soot primary particles (size 10 to 40 nm) can be described with a constant coagulation kernel beta(c,exp)=2.37x10(-9) cm3/s (coagulation constant tau(c) approximately = 0.28 ms). This result is in nice accord with the Smoluchowski coagulation equation in the free molecular regime, and, vice versa, it is in contrast with previous studies conducted by invasive (ex situ) techniques, which claimed the evidence in flames of coagulation rates much larger than the kinetic theory predictions. Thereafter, a number of numerical simulations is implemented to compare with the experimental results on primary particle growth rate and on the process of aggregate reshaping that is observed by light scattering at later residence times. The restructuring process is conjectured to occur, for not well understood reasons, as a direct consequence of the atomic rearrangement in the solid phase carbon due to the prolonged residence time within the flame. Thus, on one side, it is shown that the numerical simulations of primary size history compare well with the values of primary size from SEM experiment with a growth rate constant of primary diameter about 1 nm/s. On the other side, the evolution of aggregate morphology is found to be predictable by the numerical simulations when the onset of a first-order "thermal" restructuring mechanism is assumed to occur in the flame at about 20 ms residence time leading to aggregates with an asymptotic fractal dimension D(f,infinity) approximately = 2.5.
本文采用光散射技术原位研究了扩散大气火焰中生成的生长烟灰的团聚动力学,以推断团簇形态和尺寸(分形维数D(f)和回转半径R(g))。扫描电子显微镜(SEM)分析用作标准参考,以获取不同停留时间下的初级颗粒尺寸D(P)。基于散射光强度的测量角度模式,评估每个聚集体中的初级颗粒数量N(P)和团簇的数量浓度n(A)。主要发现是,由烟灰初级颗粒(尺寸为10至40纳米)形成链状聚集体的凝聚过程动力学可以用恒定的凝聚核β(c,exp)=2.37×10(-9)立方厘米/秒(凝聚常数τ(c)约为0.28毫秒)来描述。这一结果与自由分子状态下的斯莫卢霍夫斯基凝聚方程非常吻合,反之,它与之前采用侵入性(非原位)技术进行的研究形成对比,那些研究声称在火焰中观察到的凝聚速率远大于动力学理论预测值。此后,进行了一些数值模拟,以与初级颗粒生长速率以及在后期停留时间通过光散射观察到的聚集体重塑过程的实验结果进行比较。由于尚未完全理解的原因,推测重组过程是火焰中固相碳由于长时间停留导致原子重排的直接结果。因此,一方面,结果表明初级尺寸历史的数值模拟与扫描电子显微镜实验得到的初级尺寸值吻合良好,初级直径的生长速率常数约为1纳米/秒。另一方面,当假设在约20毫秒停留时间的火焰中发生一阶“热”重组机制,导致聚集体具有渐近分形维数D(f,∞)约为2.5时,聚集体形态的演变可以通过数值模拟预测。