Partial Differential Equations with Applications to Finance Seminar 3: A reciprocal supershare option Group 4: Bertan Yilmaz, Stephane Dumanois and Azza Alghamdi May 21, 2015 -. 1 A reciprocal supershare option In this seminar, we consider the following problem. Exam 2012-08-22, Problem 4: (a) Assume that the price process S(t) of a risky asset evolves as a geometric Brownian motion. Let L, U, M > 0 be positive constants such that L < U . Suppose that T > 0 is the expiration date of the reciprocal supershare option which at maturity pays the amount M U/S(T ) if S(T ) ∈ [L, U ], or nothing if S(T ) ∈ / [L, U ]. Using the standard Black-Scholes approach, derive the price of such an option at time t ∈ [0, T ]. (b) Specify the partial differential equation that the pricing function for the above option must satisfy. 2 Solution: (a) Remark first of all that, although the similarity, we are not dealing with any type of barrier option as the pay-off in that case would automatically be zero if the price process S(t) ever hit L or U before expiration. We will start our solution by stating some fundamental assumptions made in the solution of the problem. Assumption 1: We assume that: 1. The derivative instrument in question can be bought and sold on a market. 2. The market is free of arbitrage. 3. The price process of the derivative asset of the form: Π(t; X ) = F (t, S(t)) where F is some smooth function. We will in the solution of the problem employ the notation of the price process of the asset according to S(t) = St . In order to solve the given problem, we start by defining a Geometric Brownian Motion (GBM). Definition 1 (Geometric Brownian Motion): A Geometric Brownian Motion is a stochastic process Xt that satisfies the Stochastic Differential Equation (SDE): dXt = rXt dt + σXt dWt (1) together with some initial condition X0 = x where (r, σ) ∈ R2 , σ > 0 and Wt is a Wiener process. 3 We are thereafter in the need of stating the Black-Scholes equation. Theorem 1 (Black-Scholes equation): The price process of a European call or put option in the framework of the Black–Scholes model on an underlying stock paying no dividends is governed by the partial differential equation: ( Ft + rsFs + 12 σ 2 s2 Fss − rF = 0, t ∈ (0, T ), x > 0 F (T, s) = Ψ(s) where F = F (s, t) is the price of the option as a function of the stock price s and time t. Moreover, σ is the volatility of the stock, r is the risk-free interest rate and Ψ(s) is known as the payoff function. From the problem formulation, we realize that our payoff function mathematically can be expressed as: Ψ(ST ) = 1[L,U ] (ST ) MU . S(T ) (2) Now, we know that the price process of the asset evolves as a GBM as written in (1). Using the denotation for the price of the stock at time t as St we obtain the SDE: ( dSt = rSt dt + σSt dWt St = s. Define f (St ) = log St and apply Itô’s Lemma which we state before proceeding. Theorem 2 (Itô’s Lemma): Let X = (Xt )t≥0 be an Itô process given by: dXt = rdt + σdWt . Let g(t, x) ∈ C 2 ([0, ∞) × R). Then Y = (Yt )t≥0 , where: Yt = g(t, Xt ) is again an Itô process, and: ∂g 1 ∂ 2g ∂g (t, Xt )dt + (t, Xt )dXt + (t, Xt )(dXt )2 . dYt = 2 ∂t ∂x 2 ∂x 4 We employ Itô’s Lemma and hence obtain: 1 1 2 d log St0 = rSt0 f 0 (St0 )dt0 +σSt0 f 0 (St0 )dWt + σ 2 S 0t f 00 (St0 )dt = rdt0 +σdWt0 − σ 2 dt0 . 2 2 which after integration from t to T yields: Z T Z T 1 2 0 r − σ dt + σdWt0 . log ST − log St = 2 t t Note on the change of notation from t to t0 done in order to distinguish it from the lower integration limit t. Hence, we finally obtain: 1 2 St = s exp r − σ (T − t) + σ(WT − Wt ) . 2 which, using the properties of the Wiener process, we can rewrite as: (3) √ 1 r − σ 2 (T − t) + σ T − tv (4) 2 where v ∼ N (0, 1) and consequently: √ √ 1 1 r − σ 2 (T − t) + σ T − tZ ∼ N ( r − σ 2 (T − t), σ T − t). 2 2 St = s exp Using the risk-neutral valuation, we have that the arbitrage free price is given by: F (t, s) = e−r(T −t) EQ [Ψ(ST )|St = s] where the Q-dynamics is such that: dSt = rSt dt + σSt dW t where W t is a Q-Brownian motion. Our problem is consequently reduced to solving the integral: −r(T −t) F (t, s) = e Z∞ 1 √ v2 (r− 21 σ 2 )(T −t)+σ T −tv √ e− 2 dv Ψ se 2π (5) −∞ Using our payoff function as expressed in (2), we obtain: √ √ 1 2 1 2 Ψ(ST ) = Ψ se(r− 2 σ )(T −t)+σ T −tv = 1[L,U ] (se(r− 2 σ )(T −t)+σ T −tv ) 5 MU se ((r− 21 σ 2 )(T −t)+σ (6) √ T −tv) Since we are dealing with the indicator function, we can reduce the integration limits from the whole of R by solving for v in the inequalities: 1 L ≤ se((r− 2 σ 2 )(T −t)+σ √ T −tv) ≤U By simple algebraic manipulations, we arrive at: ln Us − r − 12 σ 2 (T − t) ln Ls − r − 21 σ 2 (T − t) √ √ ≤v≤ σ T −t σ T −t | | {z } {z } = d1 = d2 and hence we obtain the integral: −r(T −t) d2 Z F (t, s) = M U e 1 1 se((r− 2 σ d1 2 )(T −t)+σ √ v2 1 √ e− 2 dv T −tv) 2π (7) which we can write as: Z d2 F (t, s) = a e d1 √ −σ T −tv v2 1 √ e− 2 dv = a 2π Z d2 d1 √ v2 1 √ e− 2 −σ T −tv dv 2π (8) where M U e−r(T −t) (9) 1 2 se(r− 2 σ )(T −t) We can now rewrite the integral in (8) by completing the square in the exponential function in the integrand as: a= Z d2 F (t, s) = a d1 √ (v 2 +2σ T −tv+σ 2 (T −t)−σ 2 (T −t)) 1 2 √ e− dv = a 2π Z d2 d1 √ 1 1 2 σ2 √ e− 2 (v+σ T −t) + 2 (T −t) dv 2π (10) We denote b = ae σ2 (T −t) 2 (11) and rewrite (10) as Z d2 F (t, s) = b d1 √ 1 1 2 √ e− 2 (v+σ T −t) dv. 2π 6 (12) We now perform the variable substitution √ ξ = v + σ T − t ⇒ dv = dξ. (13) Consequently, we now integrate from √ d˜1 = d1 + σ T − t to √ d˜2 = d2 + σ T − t and our integral thus reduces to: Z d˜2 F (t, s) = b d˜1 1 2 1 √ e− 2 ξ dξ 2π (14) which we recognize as the normalized form of the cumulative normal distribution function. Our final answer thus becomes: F (t, s) = b(N (d˜2 ) − N (d˜1 )) where 1 2 √ − r − σ (T − t) 2 √ d˜1 = + σ T − t, σ T −t U 1 2 √ σ (T − t) ln − r − x √ 2 d˜2 = +σ T −t σ T −t ln L x and b= M U e−r(T −t) se e (r− 1 σ 2 )(T −t) σ2 (T −t) 2 2 7 = M U (σ2 −2r)(T −t) e . s (15) (b) We easily realize that the pricing function F (t, s) must satisfy the Black-Scholes equation as: ( Ft + rsFs + 21 σ 2 s2 Fss − rF = 0, Ψ(s) = MsU 1{L≤s≤U } (s). 8 t ∈ (0, T ), x>0
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