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HAL Id: hal-01081470

https://hal.archives-ouvertes.fr/hal-01081470v2

Preprint submitted on 25 Feb 2015

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Parameter estimation for stochastic diffusion process

Elotma H

To cite this version:

Elotma H. Parameter estimation for stochastic diffusion process. 2015. �hal-01081470v2�

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Parameter estimation for stochastic diffusion process with drift proportional to Weibull density

function

H El otmany (version 0) [email protected]

Abstract. In the present paper we propose a new stochastic diffusion process with drift proportional to the Weibull density function defined as

Xε=x, dXt

t(1−tγ+1)−tγ

Xtdt+σXtdBt, t >0,

with parametersγ >0 andσ >0, whereBis a standard Brownian motion andt=ε is a time near to zero. First we interested to probabilistic solution of this process as the explicit expression of this process. By using the maximum likelihood method and by considering a discrete sampling of the sample of the new process we estimate the parameters γandσ.

Keyword: Maximum LikeLihoode, Itˆo’s formula, Weibul density, stochastic diffu- sion process, parameter estimation

1 Introduction

In the present paper we propose a new stochastic Weibull process X = { X

t

, t > 0 } given by the following linear stochastic differential equation

X

ε

= x > 0; dX

t

= γ

t (1 − t

γ+1

) − t

γ

X

t

dt + σX

t

dB

t

, t > 0

where µ(t, X

t

; γ) =

γt

(1 − t

γ+1

)X

t

− t

γ

X

t

and g(X

t

; σ) = σX

t

. We denote by B a standard Brownian motion and γ and σ are an unknown parameters. An interesting problem is to estimate the parameters γ and σ are time independent reel parameters to be estimate when one observes the whole trajectory of X.

The estimation for diffusion processes by discrete observation has been studied by several authors ( see for example [6], [7], [1], [2], [5])and its references. Prakasa Rao [7] treats this problem and shows that the least square estimator is asymptotically normal and efficient under the assumption h √

N −→ 0, the condition for ”rapidly increasing experimental design” [7].

The organization of our paper is as follows. Section 2 contains the presentation of the basic tools that we will need throughout the paper: basic properties of of standard Brownian motion and It’s formula . The aim of section 3 is twofold.

Firstly, we prove the close formula of SDE under the conditions (1) − (3). Secondly,

we invesigate the mean of X

t

an explicit solution of SDE and we prove that the drift

is proportionnel to Weibul density. The section 4 is devoted to estimate a parameters

by using Maximum likelihood. In the last section we present a numerical test.

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Given the general one-dimensional time-homogeneous SDE

X

ε

= x > 0; dX

t

= µ(X

t

; γ)dt + g(X

t

; σ)dB

t

, t > 0. (1.1) where µ(t, X

t

; γ) =

γt

(1 − t

γ+1

)X

t

− t

γ

X

t

and g(X

t

; σ) = σX

t

. The following condi- tions are assumed in this article :

(1) There is a constant L > 0 such that

| µ(t, x; γ) | + | g(x; σ) | ≤ L(1 + | x | ) (2) There is a constant L > 0 such that

| µ(t, x; γ) − µ(t, y; γ ) | + | g(x; σ) − g(y; σ) | ≤ L | x − y | (3) For each q > 0, sup

t

E ( | X

t

|

q

) < ∞ .

2 Preliminaries

In this section we start by recalling the definition of Brownian motion, which is a funda- mental example of a stochastic process. The underlying probability space (Ω, F , P ) of Brownian motion can be constructed on the space Ω = C

0

( R

+

) of con- tinuous real-valued functions on R

+

started at 0. For more complete presentation on the subject, see [4], [3].

Definition 2.1. The standard Brownian motion is a stochastic process (B

t

, t ≥ 0) such that

(a) B

0

almost surely;

(b) With probability one t −→ B

t

is continuous.

(c) For any finite sequence of times t

0

< t

1

< · · · < t

n

the increments B

t1

− B

t0

, B

t2

− B

t1

, · · · B

tn

− B

tn1

are independent.

(d) for any given times 0 ≤ s < t, B

t

− B

s

has the Gaussien distribution N (0, t − s) with mean zero and variance t − s.

We refer to Theorem 10.8 of [4] and to Chapter of [4] for the proof of the existence of Brownian motion as a stochastic process (B

t

, t ≥ 0) satisfying the above properties (a) − (d). In the sequel the filtration ( F

t

)

t≥0

will be generated by the Brownian paths up to time t, in other words we write

F

t

= σ(B

s

: 0 ≤ s ≤ t), t ≥ 0.

we give a basic properties of Brownian motion and extentions ([?]):

• The crucial fact about Brownian motion, which we need is (dB )

2

= dt;

• For every 0 ≤ s ≤ t, B

t

− B

s

is independent of { B

u

, u ≤ s } and has a

N (0, t − s);

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• Brownian motion (B

t

) is a process Markov property;

• ( − B

t

)

t≥0

is a Brownian motion;

• X

t

= X

0

+ µt + σB

t

is a Brownian motion with drift with mean equal to X

0

+ µt;

• X

t

= X

0

exp(µt + σB

t

) is a Geometric Brownian motion with mean equal to X

0

exp(µt + σ

2

/2).

We introduce the following two version of It’s formula

Theorem 2.2. ( Itˆo’s formula v.1) Let f ∈ C

2

( R ). Then for a < t, f (B

t

) − f (B

a

) =

Z

t

a

f

(B

s

) ds + 1 2

Z

t

a

f

′′

(B

s

) ds (2.1) Theorem 2.3. ( Itˆo’s formula v.2) Let = f (t, x) be a continuous in [a, b] × R with f

t

, f

x

, and f

xx

continuos (a, b) × R . Then for a < t < b,

f(t, B

t

) − f(a, B

a

) = Z

t

a

f

x

(s, B

s

) dB

s

+ Z

t

a

f

t

(s, B

s

) + 1

2 f

xx

(s, B

s

)

ds. (2.2)

3 Closed formula and mean of X t

By curiosity, we focus on the explicit formula for the SDE to find the mean and variance of X

t

. By using the It’s formula to Y

t

= ln(X

t

) we obtain

dY

t

= γ

t (1 − t

γ+1

) − t

γ

− σ

2

2

dt + σdB

t

, Y

ε

= ln x. (3.1) By integrating between ε and t it follows

Y

t

= ln x + γ ln t

ε

− (t

γ+1

− ε

γ+1

) − σ

2

2 (t − ε) + σ(B

t

− B

ε

). (3.2) Then the explicit solution of SDE is given by

X

t

= x t

ε

γ

exp

− (t

γ+1

− ε

γ+1

) − σ

2

2 (t − ε) + σ(B

t

− B

ε

)

, ∀ t > 0. (3.3) We intersted now to mean of X

t

. By using the conditional expectation or the Geomtric Brownian we prove that the trend of the process X

t

is given by

E (X

t

) = x t

ε

γ

exp ε

γ+1

− t

γ+1

, (3.4)

then it follows that the trend of X

t

is proportional to Weibul density.

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4 Maximum likelihood estimators for the param- eters of SDE

A formal statement of the parameter estimation problem to be addressed is as follows. Given the general one-dimensional time-homogeneous SDE

X

ε

= x > 0; dX

t

= µ(X

t

; γ)dt + g(X

t

; σ)dB

t

, t > 0. (4.1) where µ(t, X

t

; γ) =

γt

(1 − t

γ+1

)X

t

− t

γ

X

t

and g(X

t

; σ) = σX

t

.

The task is to estimate the parameters θ = (γ, σ

2

) of this SDE from a sample of N + 1 observations X

1

, X

2

, · · · , X

N

of the stochastic process at known times t

1

, · · · , t

N

. In the statement of equation (4.1), dB is the differential of the Brownian motion and the instantaneous drift µ(t, x; γ) and instantaneous diffusion g(x; σ).

Assuming that P (X

t1

= x) = p 6 = 0, for the sake of simplicity, let us assume that p = 1.

The ML estimate of θ is generated by minimising the negative log-likelihood function of the observed sample, namely

LL(X

1

, X

2

, · · · , X

n

; θ) = log f

1

(X

1

| θ) −

N

X

k=2

log f (X

k+1

| X

k

; θ) (4.2) with respect to the parameters θ = (γ, σ

2

). In this expression, f

1

(X

1

| θ) is the density of the initial state and f(X

k+1

| X

k

; θ) ≡ f ((X

k+1

, t

k+1

) | (X

k

, t

k

); θ) is the value of the transitional PDF at (X

k+1

, t

k+1

) for a process starting at (X

k

, t

k

) and evolving to (X

k+1

, t

k+1

) in accordance with equation (4.1). Note that the Markovian property of equation (4.1) ensures that the transitional density of X

k+1

at time t

k+1

depends on X

k

alone.

ML estimation relies on the fact that the transitional PDF, f(x, t), is the solution of the Fokker-Planck equation

∂f

∂t = ∂

∂x 1

2

∂ (g (x; σ)f)

∂x − µ(x; γ)f

(4.3) satisfying a suitable initial condition and boundary conditions. Suppose, further- more, that the state space of the problem is [a, b] and the process starts at x = X

k

at time t

k

. In the absence of measurement error, the initial condition is

f (x, t

k

) = δ(x − X

k

) (4.4)

where δ is the Dirac delta function, and the boundary conditions required to conserve unit density within this interval are

x−→a

lim

+

1

2

∂ (g(x; σ)f )

∂x − µ(x; γ)f

= 0, lim

x−→b

1 2

∂ (g(x; σ)f )

∂x − µ(x; γ)f

= 0.

By using Itˆo formula to Y

t

= ln(X

t

) we have the linear diffusion dY

t

=

γ

t (1 − t

γ+1

) − t

γ

− σ

2

2

dt + σdB

t

, (4.5)

By integrating between t

k

and t

k+1

, the exact discret model correspond to (4.14) is given by

ln(X

k+1

) = ln(X

k

)+γ ln t

k+1

t

k

− (t

γ+1k+1

− t

γ+1k

) − σ

2

2 (t

k+1

− t

k

)+σ(B

tk+1

− B

tk

), (4.6)

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From the above, the variance and esperance of ln(X

k+1

) is given by E (ln(X

k+1

) | X

k

) = ln(X

k

) + γ ln

t

k+1

t

k

− (t

γ+1k+1

− t

γ+1k

) − σ

2

2 (t

k+1

− t

k

), V (ln(X

k+1

) | X

k

) = σ

2

(t

k+1

− t

k

),

then the transitional probability density function (PDF) for SDE has the following closed form expression:

X

k+1

| X

k

∼ N

ln(X

k

) + γ ln t

k+1

t

k

− (t

γ+1k+1

− t

γ+1k

) − σ

2

2 (t

k+1

− t

k

), σ

2

(t

k+1

− t

k

)

(4.7) Now, the classical approach to the ML method requires the computation of the first-order partial derivatives of the log-likelihood function with respect to each of its parameters, equating them equal to zero and then solving the resulting system of equations. So, the first-order partial derivatives are obtained as follows:

∂LL

∂γ = 1 2σ

2

N

X

k=2

2

+ 2A

k

(X

k

, t

k

))

ln( t

k

t

k−1

) − (γ + 1)(t

γk

− t

γk−1

)

= 0, (4.8)

∂LL

∂σ

2

= − n − 1 2σ

2

+ 1

4

N

X

k=2

2

+ 2A

k

(X

k

, t

k

))

2

− 1 4σ

2

N

X

k=2

2

+ 2A

k

(X

k

, t

k

)) = 0 (4.9) with A

k

(X

k

, t

k

) = ln(

XXk

k1

) − γ ln(

ttk

k1

) + t

γ+1k

− t

γ+1k−1

. From the equation (4.9) we obtain

4(N − 1)ˆ σ

2

− (N − 1)ˆ σ

4

= 4

N

X

k=2

A ˆ

2k

(X

k

, t

k

) (4.10)

By using the positivity of ˆ σ

2

we have the following expression of estimator ˆ σ

2

ˆ

σ

2

= 4 − 4 N − 1

N

X

k=2

A ˆ

2k

(X

k

, t

k

)

!

1/2

− 2. (4.11)

Consequently, we prove the non-linear expression of estimator ˆ γ by replacing ˆ σ

2

in (4.8) :

N

X

k=2

(ˆ σ

2

+ 2 ˆ A

k

(X

k

, t

k

))

ln( t

k

t

k−1

) − (ˆ γ + 1)(t

γkˆ

− t

γk−1ˆ

)

= 0 (4.12) where ˆ A

k

(X

k

, t

k

) = ln(

XXk

k1

) − ˆ γ ln(

ttk

k1

) + t

γ+1kˆ

− t

ˆγ+1k−1

.

It is assumed that the observation from the realization consists of X

tk

, t

1

= ε, t

k

= kh with h > 0, k = 2, 3, · · · , N . We define the new estimator of σ

2

:

ˆ

σ

2

= 4 − 4 N − 1

N

X

k=2

ln( X

k

X

k−1

) − γ ˆ ln( k

k − 1 ) + h

γ+1ˆ

(k

γ+1ˆ

− (k − 1)

ˆγ+1

)

2

!

1/2

− 2.

(4.13)

Assuming that γ ∼ = ˆ γ. The following proposition is more or less well khnown.

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Proposition 4.1. If condition (1) − (3) hold, then E (ˆ σ

2

− σ

2

) ≤ C

1

N − 1 + h)

.

Proof. By using integrating the following equation between t

k−1

= (k − 1)h and t

k

= kh:

dY

t

= γ

t (1 − t

γ+1

) − t

γ

− σ

2

2

dt + σdB

t

, (4.14) By summing between k = 2 and N and using E (B

tk

− B

tk

1

)

2

= h. Then we prove a result.

5 Numerical test

We present numerical results in the software R for the following SDE:

X

ε

= 10, dX

t

= γ

t (1 − t

γ+1

) − t

γ

X

t

dt + σX

t

dB

t

, t > 0,

with: and we generate sampled data X

tk

with γ = 1, σ = 0.2 and time step ∆ = 10

−3

as following:

• mu <- expression( ((1./t)- 2*t)*x)

• g <- expression(0.2*x)

• Simulation <- SNSDE(drift=mu,diffus=g,N=1000,Dt=0.001,x0=10)

• MyData <- SimulationX

• mux <- expression( gama ∗ x./t − (gama + 1) ∗ t

(gama+1)

∗ x )

• gx <- expression( sigma ∗ x )

• Model <- FDE(data=MyData,drift=mux,diffus=gx,start = list(gama=1,sigma=0.2),”euler”)

• summary(Model) Result :

Pseudo maximum likelihood estimation Method: Euler

Call:

FSDE(data = MyData, drift = mux, diffus = gx, start = list(gamma=1, sigma=1),”euler”) The following table prove the estimate coefficients and standard error with − 2 log L :

8794.337 by unsig our methods.

Estimate coefficient Standard error

γ 0.9856006 0.006651509

σ 0.2310434 0.005168557

Figure 1: Estimate coefficients and Standard Error

By using the command in the R software ” confint(Model,level= 0.9)”, we obtain

the following table. It shows the confidence interval for the estimated variables γ

and σ.

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5% 15% 75% 95%

γ 0.9711487 1.0000124 1.0003527 1.0012685 σ 0.2225419 0.2238546 0.2310215 0.2395449

Figure 2: Confidence interval

References

[1] Dacunha, D.C. and Florens, D.Z.Estimation of the Coefficients of a Diffusion from Discrete Observations. Stochastics. 19, 263-284, (1986).

[2] Florens, D. (1999). Estimation of the diffusion coefficient from the crossings, Stat. Infer. Stochastic Process. 1, 175-195.

[3] Karatzas, I., Shreve, S.E. Brownian Motion and Stochastic Calculus, 2nd edi- tion, Springer-Verlag, New York, (1991).

[4] Lamberton, D. Lapeyre, B. Introduction au Calcul Stochastique Appliqu la Finance, Eclipses, Paris, (1999).

[5] Yoshida, N. Estimation of diffusion processes from discrete observations. Jour- nal of Multivariate Analysis. 41, 220-242 (1992).

[6] PRAKASA RAO, B. L. S. Asymptotic theory for non-linear least square es- timator for diffusion processes, Math. Operationsforsch. Statist. Ser. Statist., Vol. 14, pp. 195-209, Berlin, (1983).

[7] PRAKASA RAO, B. L. S.Statistical inference from sampled data for stochastic

processes. Contemporary Mathematics, Vol. 80, 249-284. Amer. Math. Sot.,

Providence, RI., (1988).

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