Research Article | Open Access
Yong-Ki Ma, "Correlated Log-Normal Random Variables under a Multiscale Volatility Model", Advances in Mathematical Physics, vol. 2021, Article ID 5916312, 7 pages, 2021. https://doi.org/10.1155/2021/5916312
Correlated Log-Normal Random Variables under a Multiscale Volatility Model
The study focuses on extending the fast mean-reversion volatility, which was developed by the author in a previous work, to the multiscale volatility model so that it can express a well-separated time scale. The leading-order term and first-order correction terms are analytically computed using the perturbation theory based on the Lie–Trotter operator splitting method. Finally, the study is concluded by deriving the numerical results that further validate the effectiveness of the model.
A stochastic process provides a useful tool to analyze time series data and wide applications in many fields such as physics, finance, biotechnology, and telecommunication studies. The transition density function of a continuous-time process plays an important role in understanding and explaining the dynamics of the process. However, the transition density functions are unknown for general diffusion processes except for a few special cases (refer to Aït‐Sahalia , Black and Scholes , Cox et al. , and Vasicek ). So finding analytical approximations to them is important as numerical methods, such as finite-difference method, Monte Carlo simulation, and Fourier inversion, because of much faster and precise at least under certain model parameter regime.
In particular, the multivariate log-normal distribution is a widely used stochastic model in social sciences. What is the probability of the sum or difference of log-normal random variables? The solution to this question has wide applications in many fields such as finance , physics , and actuarial science . However, to the best of the author of this paper’s knowledge, almost nothing is known about the question yet (see ).
Fat-tailed distribution and volatility clustering are widely utilized to yield stylized facts in the field of financial modeling. It is known that high volatility leads to high volatility and low volatility leads to low volatility. Generally, such phenomena are observed on different time scales and are characterized by the tendency of short-run volatility clustering (or fast mean-reversion) and long-run volatility clustering. In addition, these phenomena can only be delineated by multiscale models and not by single-scale models. Therefore, this study focuses on extending the fast mean-reversion volatility (FMRV) model, which is a previously proposed model by the author, to multiscale volatility (MSV) model. This extension would aid the researchers and practitioners, such as Adrian and Rosenberg , Chernov et al. , Fouque et al. , and Gallant et al. , in obtaining financial derivatives, especially those with derived empirical evidence.
Based on the observation that the well-separated time scale exists in financial time series data, in this work, a slow varying process is incorporated into the previously derived results. Moreover, approximate transition density under the MSV model is derived by the perturbation theory based on the Lie–Trotter operator splitting method.
2. Asymptotic Analysis
2.1. Problem Formulation
We denote and as and , respectively. The probability distribution of the sum or difference of the two correlated log-normal distributions can be obtained by calculating the integral where is the joint probability distribution of the two log-normal random variables and is the Dirac delta function. However, a closed-form representation for this probability distribution does not exist. Thus, we derive an analytic approximation of the transition density function of the sum or difference of the two correlated log-normal distributions (refer to ).
We start with a process describing the conditionally log-normal random variables and and two processes and to express a well-separated time scale. These two processes represent a fast scale factor and a slow scale factor of the volatility, respectively. The dynamics of the joint process are given by the following stochastic differential equations (SDEs) under a risk-neutral measure: where , , , and are standard Brownian motions correlated as follows: with . Here, the functions and are assumed to be bounded, smooth, and strictly positive. The functions and satisfy the Lipschitz and growth conditions such that the corresponding SDE yields a unique strong solution. The parameters , and are positive constants with the same order of . Notably, the process is an ergodic process such that its invariant distribution is given by the Gaussian probability distribution function as
This provides an important averaging tool for the unobserved process that is well documented in . Notation is adopted for the expectation with respect to this invariant distribution.
By using the four-dimensional Feynman–Kac formula (cf. ), we obtain a singularly and regularly perturbed partial differential equation (PDE) problem given by where
Here, is the infinitesimal generator of the Ornstein–Uhlenbeck (OU) process . consists of the mixed partial derivatives due to the correlations of the two Brownian motions and and and , respectively. corresponds to the operator of a generalized version of the two-dimensional standard Brownian motion at the volatility levels and instead of constant volatilities and , respectively. includes the mixed partial derivatives due to the correlations of the two standard Brownian motions and and and , respectively. is the infinitesimal generator of the process . Finally, denotes the mixed partial derivative due to the correlation of the two standard Brownian motions and .
2.2. Multiscale Analysis
Since it is difficult to solve the PDE problem (5), we are interested in the following asymptotic expansions: such that is a series of the general term . Substituting the expansion (9) into (5) gives and , given by the solutions of the PDEs
2.3. Perturbation Theory Based on Lie–Trotter Operator Splitting Method
Theorem 1. Assume that the partial derivative of with respect to does not grow as much as as tends to infinity. Then, the leading-order term of the expansion (9) with is independent of the fast-scale variable , and it takes the following form: where Here, and are defined by respectively, in terms of (the invariant distribution of ).
Proof of Theorem 1. Applying the expansion with to leads to
By multiplying (15) with and then letting tend to zero, we obtain the ordinary differential equation (ODE)
Reiterating the fact that the operator is the generator of the OU process , the solution of this ODE must be a constant with respect to the variable because of the assumed growth condition:
In addition, we have the PDE . Applying the -independence of to this PDE reduces it to the ODE =0. Therefore, is independent of because of the same reason as :
Hitherto, the first two terms and did not depend on the current level of the fast-scale volatility, which is driving the process .
To simplify the equation, one can continue to eliminate the terms of order and so forth. From the order 1 terms of (15), we get . Then, this PDE becomes due to the -independence of . Equation (19) is a Poisson equation for with respect to the operator in the variable. It is well known from the Fredholm alternative (solvability condition) that it has a solution only if the source term is centered with respect to the invariant distribution of ; namely, Then, solves the PDE (20).
Note that is identical to the transition density function of Lo’s result such that the coefficients and are replaced by and , respectively. Furthermore, we employ the leading-order solution obtained above to derive the first-order correction terms and , respectively.
Theorem 2. Assume that the partial derivative of with respect to does not grow as much as as tends to infinity. The correction term is independent of the variable, and the first-order correction term satisfies the PDE where . Then, one obtains the solution of the PDE where the constant parameters Here, the functions and are defined by the solution of
Proof of Theorem 2. The order terms in (15) lead to which is a Poisson equation for whose centering condition is given by Meanwhile, from (19) and the operator , we get for some function that does not depend on the variable. Substituting (27) into (26), a PDE for is obtained as This implies that is -independent. Since we focus on the first-order correction terms of , we reconstruct (28) with respect to as follows: To calculate the operator , we aim to derive Thus, the operator can be expressed as where , and are those given in Theorem 2. Subsequently, we obtain the result of Theorem 2 by direct computation.
Similarly, the correction term can be obtained.
Theorem 3. Assume that the partial derivative of with respect to does not grow as much as as tends to infinity. The first correction term is independent of the variable, and the first-order correction term satisfies the PDE problem where which makes obtaining the solution to the PDE feasible where
Proof of Theorem 3. To obtain another first-order correction term, it is necessary to consider another singular perturbation problem. Applying expansion (9) with and leads to
By multiplying (36) with and then letting tend to zero, we find the first two leading-order terms as follows:
(the solution of ) must be a constant with respect to the variable because the operator is the generator of the OU process . Since has a derivative with respect to the variable and is independent of , we obtain
Moreover, because each term of has a derivative with respect to , holds. In light of the above observations, the equation
which implies does not depend on the variable. Hence, the two terms and do not depend on the current level of the fast-scale volatility driving process :
This makes the continuous elimination of order 1 terms, e.g., and , possible.
For the order 1 term, we have As and are -independent, the preceding PDE (42) can be expressed as This represents a Poisson equation for with respect to the operator in the variable, which has a solution only if is centered with respect to the invariant distribution of . Since and do not depend on the variable , we have Then, we obtain the result of Theorem 3 by direct computation.
As a result, one can approximate to the summation of the leading-order term and the first correction terms and as follows:
Note that the distributions of the sum and difference of correlated log-normal random variables under the MSV model are observed to follow a combination of shifted log-normal distribution and their mixed partial derivatives. In addition, all the original parameters are absorbed in the group parameters , and . The present level of the hidden process that drives the fast time scale volatility need not be specified in the present approximation.
3. Numerical Experiment
In this section, we strengthen the effectiveness of the derived result (46) by showing numerical results.
Several parameter sets are obtained from the study of Ma except for new group parameters. Three main results can be observed from the left of Figure 1. First, the constant volatility is the leading-order term (shifted log-normal distribution). Second, the short-scale volatility is a combination of the leading-order term and the first correction term driven by the fast moving fluctuation (shifted log-normal distributions under the FMRV model). Finally, two different time scale volatility is a combination of the leading-order term and the first correction terms (shifted log-normal distributions under the MSV model). The right of Figure 1 depicts the errors calculated by subtracting the log-normal distributions under the FMRV model and the MSV model from the log-normal distribution, respectively. Additionally, we applied the same result to the difference in the probability density function in Figure 2. Numerical results delineate that the short-scale volatility and the multiscale volatility shift to the left (or to the right) from the constant volatility. The left and right skew scenarios are presented through the first-order correction terms, and the major discrepancies appear around the peak of the probability density function. There is a small gap between the FMRV model and the MSV model; this implies that the prices of financial derivatives with short-term maturity levels are ruled by a fast-scale volatility process. On the contrary, those of financial derivatives with long-term maturity levels are dominated by a slow-scale volatility process in the area of financial modeling. Finally, a simulation result shows that our result could explain a financial point of view. Note that the numerical result clearly outlines that this domain is sensitive to the choice of the involved parameters and provides considerable flexibility to the shape of the transition density.
4. Final Remarks
We incorporate a slow varying process into the previously published result of the author. A two-factor stochastic volatility model is formulated that comprises a slow varying process representing one persistent factor for volatility and one ergodic process for displaying rapidly moving fluctuations. Using perturbation theory based on the Lie–Trotter operator splitting method, we compute the leading-order term, the first-order correction terms, and the effectiveness of the slow-scale volatility factor by outlining numerical results.
This paper offers various possible directions for further development. This result can provide a very useful guide for credit risk management (see [13, 15–17]). We leave these issues as future research topics.
Our paper contains numerical experimental results, and values for these experiments are included in the paper. The data is freely available.
Conflicts of Interest
The author declares that there is no conflict of interests regarding the publication of this paper.
This work was supported by Basic Science Research Program through the National Research Foundation of Korea (NRF) funded by the Ministry of Education (No. 2018R1D1A1B07049623).
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