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combustion Combustion, or burning, is a high-temperature exothermic redox chemical reaction between a fuel (the reductant) and an oxidant, usually atmospheric oxygen, that produces oxidized, often gaseous products, in a mixture termed as smoke. Combusti ...
, Frank-Kamenetskii theory explains the thermal explosion of a homogeneous mixture of reactants, kept inside a closed vessel with constant temperature walls. It is named after a Russian scientist
David A. Frank-Kamenetskii David Albertovich Frank-Kamenetskii (russian: Давид Альбертович Франк-Каменецкий, August 3, 1910 – June 2, 1970) was a Soviet theoretical physicist and chemist, professor and doctor of physical, chemical and mathe ...
, who along with Nikolay Semenov developed the theory in the 1930s.


Problem description

Sources: Consider a vessel maintained at a constant temperature T_o, containing a homogeneous reacting mixture. Let the characteristic size of the vessel be a. Since the mixture is homogeneous, the density \rho is constant. During the initial period of
ignition Ignition may refer to: Science and technology * Firelighting, the human act of creating a fire for warmth, cooking and other uses * Combustion, an exothermic chemical reaction between a fuel and an oxidant * Fusion ignition, the point at which a ...
, the consumption of reactant concentration is negligible (see t_f and t_e below), thus the explosion is governed only by the energy equation. Assuming a one-step global reaction \text + \text \rightarrow \text + q, where q is the amount of heat released per unit mass of fuel consumed, and a reaction rate governed by
Arrhenius law In physical chemistry, the Arrhenius equation is a formula for the temperature dependence of reaction rates. The equation was proposed by Svante Arrhenius in 1889, based on the work of Dutch chemist Jacobus Henricus van 't Hoff who had noted in 1 ...
, the energy equation becomes :\rho c_v \frac = \lambda \nabla^2 T + q \rho B Y_ e^ where


Non-dimensionalization

Non-dimensional scales of time, temperature, length, and heat transfer may be defined as :\tau = \frac, \quad \theta = \frac, \quad \eta^j = \frac a, \quad \delta = \frac where ;Note: :''In a typical combustion process, \gamma\approx 68,\ \beta\approx 30100 so that \beta\gamma\gg 1.'' :''Therefore, t_f = \beta\gamma t_e \gg 1. That is, fuel consumption time is much longer than ignition time, so fuel consumption is essentially negligible in the study of ignition.'' :''This is why the fuel concentration is assumed to remain the initial fuel concentration Y_.'' Substituting the non-dimensional variables in the energy equation from the introduction :\frac = \frac 1 \frac 1 \frac \left(\eta^j \frac\right) + e^ Since \beta\gg 1, the exponential term can be linearized e^\approx e^\theta, hence :\frac = \frac 1 \delta \frac 1 \frac \partial \left(\eta^j \frac\right) + e^\theta At \tau=0, we have \theta(\eta,0)=0 and for \tau>0, \theta needs to satisfy \theta(1,\tau)=0 and \partial\theta/\partial \eta , _ = 0.


Semenov theory

Before Frank-Kamenetskii, his doctoral advisor Nikolay Semyonov (or Semenov) proposed a thermal explosion theory with a simpler model with which he assumed a linear function for the heat conduction process instead of the
Laplacian In mathematics, the Laplace operator or Laplacian is a differential operator given by the divergence of the gradient of a scalar function on Euclidean space. It is usually denoted by the symbols \nabla\cdot\nabla, \nabla^2 (where \nabla is the ...
operator. Semenov's equation reads as :\frac = e^\theta - \frac, \quad \theta(0)=0 in which the exponential term e^\theta will tend to increase \theta as time proceeds whereas the linear term -\theta/\delta will tend to decrease \theta. The relevant importance between the two terms are determined by the Damköhler number \delta. The numerical solution of the above equation for different values of \delta is shown in the figure.


Steady-state regime

When 0<\delta, the linear term eventually dominates and the system is able to reach a steady state as \tau\rightarrow \infty. At steady state (d\theta/d\tau=0), the balance is given by the equation :\delta e^\theta= \theta, \quad \Rightarrow \quad \theta = -W(-\delta) where W represents the
Lambert W function In mathematics, the Lambert function, also called the omega function or product logarithm, is a multivalued function, namely the Branch point, branches of the converse relation of the function , where is any complex number and is the expone ...
. From the properties of Lambert W function, it is easy to see that the steady state temperature provided by the above equation exists only when \delta\leq \delta_c=1/e, where \delta_c is called as Frank-Kamenetskii parameter as a critical point where the system bifurcates from the existence of steady state to explosive state at large times.


Explosive regime

For \delta_c<\delta<\infty, the system explodes since the exponential term dominates as time proceeds. We do not need to wait for a long time for \theta to blow up. Because of the exponential forcing, \theta\rightarrow\infty at a finite value of \tau. This time is interpreted as the ignition time or induction time of the system. When \delta\gg \delta_c, the heat conduction term -\theta/\delta can be neglected in which case the problem admits an explicit solution, :\frac = e^\theta, \quad \Rightarrow \quad \theta = \ln \left(\frac 1 \right) At time \tau=1, the system explodes. This time is also referred to as the ''adiabatic induction period'' since the heat conduction term -\theta/\delta is neglected. In the near-critical condition, i.e., when \delta-\delta_c\rightarrow 0^+, the system takes very long time to explode. The analysis for this limit was first carried out by Frank-Kamenetskii., although proper asymptotics were carried out only later by D. R. Kassoy and
Amable Liñán Amable Liñán Martínez (born Noceda de Cabrera, Castrillo de Cabrera, León, Spain in 1934) is a Spanish aeronautical engineer considered a world authority in the field of combustion. Biography He holds a PhD in Aeronautical Engineering f ...
including reactant consumption because reactant consumption is not negligible when \tau\sim \beta\gamma. A simplified analysis without reactant consumption is presented here. Let us define a small parameter \epsilon\rightarrow 0^+ such that \delta=\delta_c(1+\epsilon). For this case, the time evolution of \theta is as follows: first it increases to steady-state temperature value corresponding to \delta=\delta_c, which is given by \theta=-W(-\delta_c)=1 at times of order \tau\sim O(1), then it stays very close to this steady-state value for a long time before eventually exploding at a long time. The quantity of interest is the long-time estimate for the explosion. To find out the estimate, introduce the transformations \zeta=\sqrt\tau and \theta=1+\sqrt\psi(\zeta) -\epsilon that is appropriate for the region where \theta stays close to 1 into the governing equation and collect only the leading-order terms to find out :\delta_c\frac = 1+\frac, \quad \psi(0)\rightarrow -(1-\theta)/\sqrt=-\infty where the boundary condition is derived by matching with the initial region wherein \tau,\theta\sim 1. The solution to the above-mentioned problem is given by :\psi= - \sqrt\cot\left(\frac\right) which immediately reveals that \psi\rightarrow \infty when \zeta= \sqrt 2 \pi \delta_c. Writing this condition in terms of \tau, the explosion time in the near-critical condition is found to be :\tau = \sqrt which implies that the ignition time \tau\rightarrow \infty as \delta-\delta_c\rightarrow 0^+ with a square-root singularity.


Frank-Kamenetskii steady-state theory

The only parameter which characterizes the explosion is the Damköhler number \delta. When \delta is very high, conduction time is longer than the chemical reaction time and the system explodes with high temperature since there is not enough time for conduction to remove the heat. On the other hand, when \delta is very low, heat conduction time is much faster than the chemical reaction time, such that all the heat produced by the chemical reaction is immediately conducted to the wall, thus there is no explosion, it goes to an almost steady state,
Amable Liñán Amable Liñán Martínez (born Noceda de Cabrera, Castrillo de Cabrera, León, Spain in 1934) is a Spanish aeronautical engineer considered a world authority in the field of combustion. Biography He holds a PhD in Aeronautical Engineering f ...
coined this mode as slowly reacting mode. At a critical Damköhler number \delta_c the system goes from slowly reacting mode to explosive mode. Therefore, \delta<\delta_c, the system is in steady state. Instead of solving the full problem to find this \delta_c, Frank-Kamenetskii solved the steady state problem for various Damköhler number until the critical value, beyond which no steady solution exists. So the problem to be solved is : \frac 1 \frac d \left(\eta^j \frac\right) = - \delta e^\theta with boundary conditions :\theta(1)=0, \quad \frac_=0 the second condition is due to the symmetry of the vessel. The above equation is special case of
Liouville–Bratu–Gelfand equation : ''For Liouville's equation in differential geometry, see Liouville's equation.'' In mathematics, Liouville–Bratu–Gelfand equation or Liouville's equation is a non-linear Poisson equation, named after the mathematicians Joseph Liouville, G. B ...
in
mathematics Mathematics is an area of knowledge that includes the topics of numbers, formulas and related structures, shapes and the spaces in which they are contained, and quantities and their changes. These topics are represented in modern mathematics ...
.


Planar vessel

For planar vessel, there is an exact solution. Here j=0, then :\frac = -\delta e^\theta If the transformations \Theta= \theta_m-\theta and \xi^2 = \delta e^ \eta^2, where \theta_m is the maximum temperature which occurs at \eta=0 due to symmetry, are introduced :\frac = e^, \quad \Theta(0)=0, \quad \frac_=0 Integrating once and using the second boundary condition, the equation becomes :\frac = \sqrt and integrating again :e^ = \cosh \left(\eta \sqrt \right) The above equation is the exact solution, but \theta_m maximum temperature is unknown, but we have not used the boundary condition of the wall yet. Thus using the wall boundary condition \theta=0 at \eta=1, the maximum temperature is obtained from an implicit expression, :e^ = \cosh \sqrt \quad \text \quad \delta = 2 e^ \left(\operatorname e^\right)^ Critical \delta_c is obtained by finding the maximum point of the equation (see figure), i.e., d\delta/d\theta_m=0 at \delta_c. :\frac=0, \quad \Rightarrow \quad e^ - \sqrt\operatorname e^ =0 :\theta_= 1.1868, \quad \Rightarrow \quad \delta_c = 0.8785 So the critical Frank-Kamentskii parameter is \delta_c=0.8785. The system has no steady state (or explodes) for \delta>\delta_c=0.8785 and for \delta<\delta_c=0.8785, the system goes to a steady state with very slow reaction.


Cylindrical vessel

For cylindrical vessel, there is an exact solution. Though Frank-Kamentskii used numerical integration assuming there is no explicit solution, Paul L. Chambré provided an exact solution in 1952. H. Lemke also solved provided a solution in a somewhat different form in 1913. Here j=1, then :\frac 1 \eta \frac d \left(\eta\frac\right) = -\delta e^\theta If the transformations \omega= \eta d\theta/d\eta and \chi = e^ \eta^2 are introduced :\frac = -\frac, \quad \omega(0)=0 The general solution is \omega^2 + 4\omega + C = -2\delta\chi. But C=0 from the symmetry condition at the centre. Writing back in original variable, the equation reads, :\eta^2 \left(\frac\right)^2+ 4\eta \frac = - 2\delta\eta^2 e^\theta But the original equation multiplied by 2\eta^2 is :2\eta^2 \frac + 2\eta \frac = -2 \delta \eta^2 e^\theta Now subtracting the last two equation from one another leads to :\frac - \frac \frac - \frac \left(\frac\right)^2 =0 This equation is easy to solve because it involves only the derivatives, so letting g(\eta)=d\theta/d\eta transforms the equation :\frac - \frac - \frac=0 This is a
Bernoulli differential equation In mathematics, an ordinary differential equation is called a Bernoulli differential equation if it is of the form : y'+ P(x)y = Q(x)y^n, where n is a real number. Some authors allow any real n, whereas others require that n not be 0 or 1. The e ...
of order 2, a type of
Riccati equation In mathematics, a Riccati equation in the narrowest sense is any first-order ordinary differential equation that is quadratic in the unknown function. In other words, it is an equation of the form : y'(x) = q_0(x) + q_1(x) \, y(x) + q_2(x) \, y^2(x ...
. The solution is :g(\eta) = \frac = -\frac Integrating once again, we have \theta = A - 2\ln ( B\eta^2 + 1) where B = 1/B'. We have used already one boundary condition, there is one more boundary condition left, but with two constants A, \ B. It turns out A and B are related to each other, which is obtained by substituting the above solution into the starting equation we arrive at A = \ln (8B/\delta) . Therefore, the solution is :\theta = \ln \frac Now if we use the other boundary condition \theta(1)=0, we get an equation for B as \delta(B+1)^2 - 8B =0. The maximum value of \delta for which solution is possible is when B=1, so the critical Frank-Kamentskii parameter is \delta_c=2. The system has no steady state( or explodes) for \delta>\delta_c=2 and for \delta<\delta_c=2, the system goes to a steady state with very slow reaction. The maximum temperature \theta_m occurs at \eta=0 :\theta_m= \ln \frac \quad \text \quad \delta= 8B e^ For each value of \delta, we have two values of \theta_m since B is multi-valued. The maximum critical temperature is \theta_ = \ln 4.


Spherical vessel

For spherical vessel, there is no known explicit solution, so Frank-Kamenetskii used numerical methods to find the critical value. Here j=2, then :\frac 1 \frac d \left(\eta^2\frac\right) = -\delta e^\theta If the transformations \Theta= \theta_m-\theta and \xi^2 = \delta e^ \eta^2, where \theta_m is the maximum temperature which occurs at \eta=0 due to symmetry, are introduced : \frac 1 \frac d \left(\xi^2\frac\right)= e^, \quad \Theta(0)=0, \quad \frac_=0 The above equation is nothing but
Emden–Chandrasekhar equation In astrophysics, the Emden–Chandrasekhar equation is a dimensionless form of the Poisson equation for the density distribution of a spherically symmetric isothermal gas sphere subjected to its own gravitational force, named after Robert Emden and ...
, which appears in
astrophysics Astrophysics is a science that employs the methods and principles of physics and chemistry in the study of astronomical objects and phenomena. As one of the founders of the discipline said, Astrophysics "seeks to ascertain the nature of the h ...
describing
isothermal In thermodynamics, an isothermal process is a type of thermodynamic process in which the temperature ''T'' of a system remains constant: Δ''T'' = 0. This typically occurs when a system is in contact with an outside thermal reservoir, and a ...
gas sphere. Unlike planar and cylindrical case, the spherical vessel has infinitely many solutions for \delta<\delta_c oscillating about the point \delta=2, instead of just two solutions, which was shown by
Israel Gelfand Israel Moiseevich Gelfand, also written Israïl Moyseyovich Gel'fand, or Izrail M. Gelfand ( yi, ישראל געלפֿאַנד, russian: Изра́иль Моисе́евич Гельфа́нд, uk, Ізраїль Мойсейович Гел ...
. The lowest branch will be chosen to explain explosive behavior. From numerical solution, it is found that the critical Frank-Kamenetskii parameter is \delta_c=3.3220. The system has no steady state( or explodes) for \delta>\delta_c=3.3220 and for \delta<\delta_c=3.3220, the system goes to a steady state with very slow reaction. The maximum temperature \theta_m occurs at \eta=0 and maximum critical temperature is \theta_ = 1.6079.


Non-symmetric geometries

For vessels which are not symmetric about the center (for example rectangular vessel), the problem involves solving a nonlinear
partial differential equation In mathematics, a partial differential equation (PDE) is an equation which imposes relations between the various partial derivatives of a Multivariable calculus, multivariable function. The function is often thought of as an "unknown" to be sol ...
instead of a nonlinear
ordinary differential equation In mathematics, an ordinary differential equation (ODE) is a differential equation whose unknown(s) consists of one (or more) function(s) of one variable and involves the derivatives of those functions. The term ''ordinary'' is used in contrast w ...
, which can be solved only through numerical methods in most cases. The equation is :\nabla^2\theta + \delta e^\theta =0 with boundary condition \theta=0 on the bounding surfaces.


Applications

Since the model assumes homogeneous mixture, the theory is well applicable to study the explosive behavior of solid fuels (spontaneous ignition of bio fuels, organic materials, garbage, etc.,). This is also used to design explosives and fire crackers. The theory predicted critical values accurately for low conductivity fluids/solids with high conductivity thin walled containers.Zukas, Jonas A., William Walters, and William P. Walters, eds. Explosive effects and applications. Springer Science & Business Media, 2002.


See also

*
Clarke's equation In combustion, Clarke's equation is a third-order nonlinear partial differential equation, first derived by John Frederick Clarke in 1978.Clarke, J. F. (1982). "Non-steady Gas Dynamic Effects in the Induction Domain Behind a Strong Shock Wave", Col ...


References

{{Reflist, 30em


External links

* The Frank-Kamenetskii problem in Wolfram solver http://demonstrations.wolfram.com/TheFrankKamenetskiiProblem/ * Tracking the Frank-Kamenetskii Problem in Wolfram solver http://demonstrations.wolfram.com/TrackingTheFrankKamenetskiiProblem/ * Planar solution in
Chebfun Chebfun is a free/open-source software system written in MATLAB for numerical computation with functions of a real variable. It is based on the idea of overloading MATLAB's commands for vectors and matrices to analogous commands for functions an ...
solver http://www.chebfun.org/examples/ode-nonlin/BlowupFK.html Fluid dynamics Combustion Explosions