Exercise: Reducing Black-Scholes to the heat equation
The Black-Scholes PDE
Vt+21σ2S2VSS+rSVS−rV=0,S>0,0≤t<T
can be reduced to the standard heat equation
uτ=21σ2uxx
by a sequence of changes of variables. This was Black, Scholes, and Merton's original path to the closed-form formula.
Tasks
Substitute τ=T−t (time to expiry). Show the PDE becomes −Vτ+21σ2S2VSS+rSVS−rV=0 (note the sign flip).
Substitute x=lnS. Convert the derivatives: VS=Vx/S, VSS=(Vxx−Vx)/S2. Show that the PDE becomes
Vτ=21σ2Vxx+(r−21σ2)Vx−rV.
The first-order term (r−21σ2)Vx is an advection term. Use the substitution V(x,τ)=eax+bτu(x′,τ) with x′=x+cτ and well-chosen a,b,c to eliminate it.
Specifically: choosing c=−(r−21σ2) shifts the drift away; choosing a=−(r−21σ2)/σ2 may also eliminate it. Pick one consistent set that gives
uτ=21σ2uxx.
Transform the terminal condition for a European call: V(S,T)=(S−K)+ becomes u(x′,0)=? in the new variables.
The heat equation has fundamental solution G(x,τ)=(2πσ2τ)−1/2exp(−x2/(2σ2τ)). Use it to write u(x,τ)=∫G(x−y,τ)u(y,0)dy, and back-transform to recover the Black-Scholes formula. (Details optional — outline the integral and identify the Gaussian integral that produces Φ(d1) and Φ(d2).)
Hint
For part 3, try V=eαx+βτu where α,β are chosen to cancel the Vx and V terms simultaneously. You'll get two algebraic equations in α,β.