Math 2.0

Partial differential equations Definition

Black–Scholes equation

Builds on Parabolic partial differential equationPartial derivativeGeometric Brownian motion

Definition

Let σ>0\sigma > 0 and r≥0r \ge 0 be constants and let T>0T > 0. The Black–Scholes equation is the parabolic equation for a function V(S,t)V(S, t) with S>0S > 0 and 0≤t<T0 \le t < T: ∂V∂t+12σ2S2∂2V∂S2+rS∂V∂S−rV=0.\frac{\partial V}{\partial t} + \frac{1}{2}\sigma^2 S^2 \frac{\partial^2 V}{\partial S^2} + r S \frac{\partial V}{\partial S} - r V = 0. Here SS is the price of the underlying asset, modelled by geometric Brownian motion with volatility σ\sigma. The constant rr is the risk-free interest rate, and VV is the price of a derivative security. It is solved with a terminal condition V(S,T)=Φ(S)V(S, T) = \Phi(S) given by the payoff Φ\Phi.

Remarks

Example: V(S,t)=SV(S, t) = S is a solution: Vt=0V_t = 0, VSS=0V_{SS} = 0, and rS⋅1−rS=0r S \cdot 1 - r S = 0. It is the value of holding one share. Another solution is V(S,t)=Ke−r(T−t)V(S, t) = K e^{-r(T - t)}, the value of a bond paying KK at time TT: Vt−rV=0V_t - r V = 0. Non-example: V(S,t)=S2V(S, t) = S^2 fails, since 12σ2S2⋅2+rS⋅2S−rS2=(σ2+r)S2≠0\frac{1}{2}\sigma^2 S^2 \cdot 2 + r S \cdot 2S - r S^2 = (\sigma^2 + r) S^2 \ne 0. With x=log⁡Sx = \log S and τ=T−t\tau = T - t, the equation becomes a heat equation with constant drift and decay terms, so it is backward parabolic in tt.

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  1. Euclidean space object
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Further reading

  1. Web https://en.wikipedia.org/wiki/Black%E2%80%93Scholes_equation
About this page
TagRJ9767FFTF
URIm2://RJ9767FFTF
Kinddefinition
WritingW0 stub
MSC35Q91, 91G20
DefinesBlack–Scholes equation
UsesParabolic partial differential equation, Partial derivative, Geometric Brownian motion

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