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partial differential equation In mathematics, a partial differential equation (PDE) is an equation which involves a multivariable function and one or more of its partial derivatives. The function is often thought of as an "unknown" that solves the equation, similar to ho ...
can be reduced to a simpler form with a known solution by a suitable change of variables. The article discusses change of variable for PDEs below in two ways: #by example; #by giving the theory of the method.


Explanation by example

For example, the following simplified form of the Black–Scholes PDE : \frac + \frac S^2\frac + S\frac - V = 0. is reducible to the
heat equation In mathematics and physics (more specifically thermodynamics), the heat equation is a parabolic partial differential equation. The theory of the heat equation was first developed by Joseph Fourier in 1822 for the purpose of modeling how a quanti ...
: \frac = \frac by the change of variables: : V(S,t) = v(x(S),\tau(t)) : x(S) = \ln(S) : \tau(t) = \frac (T - t) : v(x,\tau)=\exp(-(1/2)x-(9/4)\tau) u(x,\tau) in these steps: * Replace V(S,t) by v(x(S),\tau(t)) and apply the
chain rule In calculus, the chain rule is a formula that expresses the derivative of the Function composition, composition of two differentiable functions and in terms of the derivatives of and . More precisely, if h=f\circ g is the function such that h ...
to get ::\frac\left(-2v(x(S),\tau)+2 \frac \frac +S\left(\left(2 \frac + S\frac\right) \frac + S \left(\frac\right)^2 \frac\right)\right)=0. * Replace x(S) and \tau(t) by \ln(S) and \frac(T-t) to get ::\frac\left( -2v(\ln(S),\frac(T-t)) -\frac +\frac +\frac\right)=0. * Replace \ln(S) and \frac(T-t) by x(S) and \tau(t) and divide both sides by \frac to get ::-2 v-\frac+\frac+ \frac=0. * Replace v(x,\tau) by \exp(-(1/2)x-(9/4)\tau) u(x,\tau) and divide through by -\exp(-(1/2)x-(9/4)\tau) to yield the heat equation. Advice on the application of change of variable to PDEs is given by mathematician J. Michael Steele:


Technique in general

Suppose that we have a function u(x,t) and a change of variables x_1,x_2 such that there exist functions a(x,t), b(x,t) such that :x_1=a(x,t) :x_2=b(x,t) and functions e(x_1,x_2),f(x_1,x_2) such that :x=e(x_1,x_2) :t=f(x_1,x_2) and furthermore such that :x_1=a(e(x_1,x_2),f(x_1,x_2)) :x_2=b(e(x_1,x_2),f(x_1,x_2)) and :x=e(a(x,t),b(x,t)) :t=f(a(x,t),b(x,t)) In other words, it is helpful for there to be a
bijection In mathematics, a bijection, bijective function, or one-to-one correspondence is a function between two sets such that each element of the second set (the codomain) is the image of exactly one element of the first set (the domain). Equival ...
between the old set of variables and the new one, or else one has to * Restrict the domain of applicability of the correspondence to a subject of the real plane which is sufficient for a solution of the practical problem at hand (where again it needs to be a bijection), and * Enumerate the (zero or more finite list) of exceptions (poles) where the otherwise-bijection fails (and say why these exceptions don't restrict the applicability of the solution of the reduced equation to the original equation) If a bijection does not exist then the solution to the reduced-form equation will not in general be a solution of the original equation. We are discussing change of variable for PDEs. A PDE can be expressed as a
differential operator In mathematics, a differential operator is an operator defined as a function of the differentiation operator. It is helpful, as a matter of notation first, to consider differentiation as an abstract operation that accepts a function and retur ...
applied to a function. Suppose \mathcal is a differential operator such that :\mathcalu(x,t)=0 Then it is also the case that :\mathcalv(x_1,x_2)=0 where :v(x_1,x_2)=u(e(x_1,x_2),f(x_1,x_2)) and we operate as follows to go from \mathcalu(x,t)=0 to \mathcalv(x_1,x_2)=0: * Apply the
chain rule In calculus, the chain rule is a formula that expresses the derivative of the Function composition, composition of two differentiable functions and in terms of the derivatives of and . More precisely, if h=f\circ g is the function such that h ...
to \mathcal v(x_1(x,t),x_2(x,t))=0 and expand out giving equation e_1. * Substitute a(x,t) for x_1(x,t) and b(x,t) for x_2(x,t) in e_1 and expand out giving equation e_2. * Replace occurrences of x by e(x_1,x_2) and t by f(x_1,x_2) to yield \mathcalv(x_1,x_2)=0, which will be free of x and t. In the context of PDEs, Weizhang Huang and Robert D. Russell define and explain the different possible time-dependent transformations in details.


Action-angle coordinates

Often, theory can establish the existence of a change of variables, although the formula itself cannot be explicitly stated. For an integrable Hamiltonian system of dimension n , with \dot_i = \partial H/\partial p_j and \dot_j = - \partial H/\partial x_j , there exist n integrals I_i . There exists a change of variables from the coordinates \ to a set of variables \ , in which the equations of motion become \dot_i = 0 , \dot_i = \omega_i(I_1, \dots, I_n) , where the functions \omega_1, \dots, \omega_n are unknown, but depend only on I_1, \dots, I_n . The variables I_1, \dots, I_n are the action coordinates, the variables \varphi_1, \dots, \varphi_n are the angle coordinates. The motion of the system can thus be visualized as rotation on torii. As a particular example, consider the simple harmonic oscillator, with \dot = 2p and \dot = - 2x , with Hamiltonian H(x,p) = x^2 + p^2 . This system can be rewritten as \dot = 0 , \dot{\varphi} = 1 , where I and \varphi are the canonical polar coordinates: I = p^2 + q^2 and \tan(\varphi) = p/x . See V. I. Arnold, `Mathematical Methods of Classical Mechanics', for more details. V. I. Arnold, ''Mathematical Methods of Classical Mechanics'', Graduate Texts in Mathematics, v. 60, Springer-Verlag, New York, 1989


References

Multivariable calculus *