Martingale expansion getdoc56cb. 270KB Jun 04 2011 12:04:24 AM

As a practical application, Fouque et al. [8] proposed its use in calibration problem. They derived an expansion of the Black-Scholes implied volatility σ BS of the form σ BS K, T − t ≈ a logK S T − t + b 9 from 7, where K is the strike price, S is the spot price, T − t is the time to the maturity, a and b are constants connecting to V 2 and V 3 as V 2 = ¯ σ ¯ σ − b − ar + 3 2 ¯ σ 2 , V 3 = −a ¯ σ 3 , ¯ σ 2 = Π [ϕ 2 ]. 10 The calibration methodology consists of i estimation of ¯ σ from historical stock returns, ii estima- tion of a and b by fitting 9 to the implied volatility surface, and iii pricing or hedging by using estimated ¯ σ, a and b via 8 and 10. This approach captures the volatility skew as well as the term structure. It enables us to calibrate fast and stably due to parsimony of parameters; we have no more need to specify all the parameters in the underlying stochastic volatility model. The first step i can be eliminated because the number of essential parameters is 2 in light of 2; by using Π η [ϕ 2 ] 1 2 instead of Π [ϕ 2 ] 1 2 for ¯ σ, where Π η is the ergodic distribution of X η , we can see that the right hand side of 8 coincides with that of 2 with V 3 = −αΠ η [ϕ 2 ] and V 2 = 2V 3 . It should be explained what is the intuition of η → 0. To fix ideas, let Λ = 0 for brevity. Then ˜ X t := X η η 2 t satisfies d ˜ X t = m − ˜ X t dt + ν p 2d ˜ W t , where ˜ W t = η −1 W η 2 t is a standard Brownian motion, and it holds dS η t = rS η t dt + ϕ ˜ X t η 2 S η t dW ρ t . Hence η stands for the volatility time scale. Note that 〈logS η 〉 t = Z t ϕ ˜ X s η 2 2 ds ∼ η 2 Z t η 2 ϕX s 2 ds → Π [ϕ 2 ]t by the law of large numbers for ergodic diffusions, where X is a solution of 6. This convergence implies that the log price logS η t is asymptotically normally distributed with mean r t − Π [ϕ 2 ]t2 and variance Π [ϕ 2 ]t by the martingale central limit theorem. The limit is nothing but the Black- Scholes model with volatility Π [ϕ 2 ] 1 2 . The asymptotic expansion formula around the Black- Scholes price can be therefore regarded as a refinement of a normal approximation based on the central limit theorem for ergodic diffusions.

2.2 Martingale expansion

Note that a formal calculation as in 7 does not ensure in general that the asymptotic expansion formula is actually valid. A rigorous validation is not easy if the payoff f or a coefficient of the stochastic differential equation is not smooth. See e.g. Fouque et al. [9]. A general result on the validity is given by Fukasawa [12]. Here we state a simplified version of it. Consider a sequence of models of type 1: dZ n t = r t − 1 2 ϕX n t 2 dt + ϕX n t h ρX n t dW 1 t + Æ 1 − ρX n t 2 dW 2 t i dX n t = b n X n t dt + c n X n t dW 1 t , 768 where b n and c n , n ∈ N are sequences of Borel functions. Theorem 2.1. Suppose that for any p 0, the L p moments of Z T ϕX n t 2 dt, Z T ϕX n t 2 1 − ρX n t 2 dt −1 11 are bounded in n ∈ N and that there exist positive sequences ε n , Σ n with ε n → 0, Σ ∞ := lim n →∞ Σ n such that   M n T p Σ n , 〈M n 〉 T − Σ n ε n Σ n   → N 0, V 12 in law with a 2 × 2 variance matrix V = {V i j } as n → ∞, where M n is the local martingale part of Z n . Then, for every Borel function f of polynomial growth, E [ f Z n T ] = E[1 + p n N f Z − logD − Σ n 2 + p Σ n N ] + o ε n 13 as n → ∞, where N ∼ N 0, 1, D is defined as in 3 and p n z = ε n V 12 2 n − p Σ n z 2 − 1 + z 3 − 3z o . An appealing point of this theorem is that it gives a validation of not only the singular perturbation but also regular perturbation expansions including the so-called small vol-of-vol expansion. It is also noteworthy that the asymptotic skewness V 12 appeared in the expansion formula is represented as the asymptotic covariance between the log price and the integrated volatility. Our interest here is however to deal with the singular case only. Now, suppose that b n and 1 + c 2 n c n are locally integrable and locally bounded on R respectively for each n ∈ N; we take R as the state space of X n by a suitable scale transformation. Further, we assume that s n R = R for each n ∈ N, where s n x = Z x exp ¨ −2 Z v b n w c n w 2 dw « dv is the scale function of X n . This assumption ensures that there exists a unique weak solution of 1. See e.g., Skorokhod [18], Section 3.1. It is also known that the ergodic distribution Π n of X n is, if exists, given by Π n dx = dx ε 2 n s ′ n xc 2 n x with a normalizing constant ε 2 n : ε 2 n = Z ∞ −∞ dx s ′ n xc 2 n x . Theorem 2.2. Suppose that i. for any p 0, the L p boundedness of the sequences 11 holds, ii. ε n → 0 as n → ∞, 769 iii. lim n →∞ Π n [ϕ 2 ] exists and is positive, iv. lim n →∞ Π n [ϕρψ n ] and lim n →∞ Π n [ψ 2 n ] exist, where ψ n x = 2ε n c n xs ′ n x Z x −∞ ϕη 2 − Π n [ϕ 2 ]Π n dη, v. the sequences Z X n T X n ψ n x c n x dx, 1 T Z T ψ n X n t 2 dt − Π n [ψ 2 n ] and 1 T Z T ψ n X n t ρX n t ϕX n t dt − Π n [ψ n ρϕ] converge to 0 in probability as n → ∞. Then, the approximation 2 is valid in that 13 holds with Σ n = Π n [ϕ 2 ]T and p n = p defined as 3 with b = b n , c = c n and Σ = Σ n . Proof: Let us verify 12 with Σ n = Π n [ϕ 2 ]T and V 12 = −2 lim n →∞ Σ −32 n Π n [ϕρψ n ]. Notice that by the Itˆ o-Tanaka formula, 〈M n 〉 T − Π n [ϕ 2 ]T = Z T ϕX n t 2 − Π n [ϕ 2 ]dt = ε n Z X n T X n ψ n x c n x dx − ε n Z T ψ n X n t dW 1 t . It suffices then to prove the asymptotic normality of Z T ϕX n t h ρX n t dW 1 t + Æ 1 − ρX n t 2 dW 2 t i , Z T ψ n X n t dW 1 t . This follows from the martingale central limit theorem under the fifth assumption. The conditions are easily verified in such a case that both Π n and s n do not depend on n ∈ N. The model 4 with Λ ≡ 0 and η = η n , where η n is a positive sequence with η n → 0, is an example of such an easy case. 3 Main results

3.1 Main theorem and remarks

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