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On estimation for the fractional Ornstein-Uhlembeck process - - PowerPoint PPT Presentation

On estimation for the fractional Ornstein-Uhlembeck process observed at discrete time Stefano M. Iacus Department of Economics, Management and Quantitative Methods University of Milan & Core Team joint work with A. Brouste (Univ. Le


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SLIDE 1

On estimation for the fractional Ornstein-Uhlembeck process

  • bserved at discrete time

Stefano M. Iacus

Department of Economics, Management and Quantitative Methods

University of Milan & Core Team joint work with A. Brouste (Univ. Le Mans, FR)

ISI Tokyo Satellite Meeting, Tokyo, 2-9-2013

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SLIDE 2

Fractional Brownian Motion

2 / 33

Let W H =

  • W H

t , t ≥ 0

  • be a normalized fractional Brownian motion (fBM), i.e.

the zero mean Gaussian processes with covariance function EW H

s W H t

= 1 2

  • |s|2H + |t|2H − |t − s|2H

with Hurst exponent H ∈ (0, 1).

the process is self-similar (W H

at ∼ aHW H t )

presents long range dependence (persistency - antipersistency)

has dependent increments (apart for H = 1

2).

For H = 1

2, W H t

= Wt is a standard Brownian motion, i.e. independent increments.

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SLIDE 3

Fractional Brownian Motion

3 / 33

0 < H < 1

2

H = 1

2 1 2 < H < 1

antipersistent independence persistent negative Brownian positive correlated motion correlated

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SLIDE 4

fractional Ornstein-Uhlenbeck (fOU)

4 / 33

Let X = (Yt, t ≥ 0) be a fractional Ornstein-Uhlenbeck process (fOU), i.e. the solution of Yt = y0 − λ t Ysds + σW H

t ,

t > 0, Y0 = y0, (1) where unknown parameter ϑ = (λ, σ, H) belongs to an open subset Θ of (0, Λ) × [σ, σ] × (0, 1), 0 < Λ < +∞, 0 < σ < σ < +∞ and W H = (W H

t , t ≥ 0)

is a standard fractional Brownian motion [10, 12] of Hurst parameter H ∈ (0, 1), The fOU process is not Markovian nor a semimartingale for H = 1

2 but

nevertheless Gaussian and ergodic. ([2]) We denote discrete observations of Yt by Xj = Ytj = Y (tj), where 0 = t0 < t1 < · · · < tN = T is a grid of deterministic times.

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SLIDE 5

Auxiliary known facts about fBm

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Let H ∈ (0, 1), t > s, {Wt, t ∈ [0, T]} a standard Brownian motion and KH(t, s) = cHs

1 2 −H

t

s

(u − s)H− 3

2 uH− 1 2 du

with cH =

  • H(2H−1)

Beta(2−2H,H− 1

2)

1

2

. The fBM can be written as follows: W H

t

= t KH(t, s)dWs, t ∈ [0, T] The following is called random walk approximation to fBM, t ∈ [0, T], BH,N

t

=

[Nt]

  • i=1

√ N   

i N

  • i−1

N

KH

[Nt] N , s

  • ds

   ξi ξi’s i.i.d., E(ξi) = 0, Var(ξi) = 1. Then, as N → ∞, BH,N

t w

→ W H

t

in Skorohod topology [14].

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SLIDE 6

fOU estimation: QMLE

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Bertin et al. (2011) [1] considered the following statistical problem dYt = λdt + dW H

t

with λ ∈ R unknown and H ∈ ( 1

2, 1) known.

Using random walk approximation & Euler scheme for the fOU, with Xj = Ytj, tj = j∆, j = 0, 1, . . . , N, N∆ = T Xj+1 = Xj + a∆ +

  • BH,N

tj+1 − BH,N tj

  • the following QMLE estimator of λ

ˆ λN = N

Nα−1

  • j=0

(1+αj)(Xj+1−Xj−hj(X1,...,Xj)) F 2

j

Nα−1

  • j=0

(1+αj)2 F 2

j

where αj, Fj and hj(· · · ) are explicit functions on the data.

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SLIDE 7

fOU estimation: true MLE

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Bertin et al. (2011) proved that, under the asymptotic: N → ∞, T = N∆ → ∞ and ∆ =

1 Nα with α < 1 the QMLE estimator ˆ

λN is unbiased and consistent for λ given the known H ∈ ( 1

2, 1).

Let SN =

N−1

  • i=0
  • X i+1

N − X i N

2 and given that [15] N 2H−1SN ∼ 1, for large N if H is estimated from the data with ˆ HN = 1 + log SN log N by simulation results only it has been shown that the estimator ˆ λN is consistent and its variance is an increasing function of H.

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SLIDE 8

fOU estimation: true MLE

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Hu et al. (2011) [6] considered the following statistical problem dYt = λdt + σdW H

t

with λ ∈ R, σ ∈ R+ unknown and H ∈ (0, 1) known. Let t = (∆, 2∆, . . . , N∆)′, X = (X1, X2, . . . , XN)′, and ΓH = [Cov(W H

i∆, W H j∆)]i,j=1,2,...,N

Then, by Malliavin calculus, it is possible to prove that the true MLE estimators ˆ µN = t′Γ−1

H X

t′Γ−1

H t

and ˆ σN = 1 N (X′Γ−1

H X)(t′Γ−1 H t) − (t′Γ−1 H X)2

t′Γ−1

H t

are strongly consistent as N → ∞ [ though E(ˆ σ2

N) = N−1 N σ2 ]

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SLIDE 9

fOU estimation: true MLE

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Central Limit Theorems. Further, it is possible to prove that

  • t′Γ−1

H t(ˆ

µN − µ) d → N

  • 0, σ2

and 1 σ2

  • N

2

  • ˆ

σ2

N − σ2 d

→ N

  • 0, σ2

as N → ∞. Simulations show that the empirical variance of ˆ µN increases with H.

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SLIDE 10

fOU estimation: contrast functions

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Ludena (2004) [11] Let H ∈ ( 1

2, 3 4) be known and consider the “vanishing drift”

fOU process Yt = y0 + t σ(θ, Ys)dBH

s

Let UN(θ) = 1

N N

  • k=1

h(θ, Xk∆, ∆XknH) with h = h(θ, x, y) at most of polynomial growth in x and y. The minimum contrast estimator ˆ θN = arg min

θ∈Θ UN(θ)

is asymptotically Gaussian, i.e. √ N(ˆ θN − θ) d → N. Result extends to the following fOU model dYt = −λYtdt + σ(θ)dW H

t

with λ > 0 known.

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SLIDE 11

fOU estimation: contrast functions

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Neuenkirch and Tindel (2011) [13] Let H ∈ ( 1

2, 1) be known and consider the fSDE

Yt = y0 + t b(Ys; θ)ds +

m

  • j=1

σjW (j)H

t

where WH

t = (W (1)H t

, W (2)H

t

, . . . , W (m)H

t

)′ is an m-dimensional fBM, σj, j = 1, 2, . . . , m and b(y, θ) are known (up to θ). Let ∆ = κN −α, α ∈ (0, 1) and κ > 0. Let QN(θ) = 1 N∆2

N−1

  • k=0

 |∆Xk − b(Xk; θ)∆|2 −

m

  • j=1

|σj|2∆2H   then, the least squares estimator ˆ θN = arg minθ∈Θ |QN(θ)| is strongly consistent. For the special case dYt = θYtdt + dW H

t , ˆ

θN is explicit.

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SLIDE 12

fOU estimation: plug-in

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Xiao et al. (2011) [16] Let H ∈ ( 1

2, 1) be known and consider the fOU process

dYt = −λYtdt + σdW H

t

The estimator ˆ σ2

N = Γ(3−2H) 2HΓ3( 3

2 −H)Γ(H+ 1 2 )(N∆)2−2H ×

N

  • j=1
  • j
  • i=1

(i∆)

1 2 −H(j∆ − ∆ − i∆) 1 2 −H∆Xi −

j

  • i=1

(i∆)

1 2 −H(j∆ − i∆) 1 2−H∆Xi

2 is strongly consistent for σ2. Moreover, for H ∈ ( 1

2, 3 4) the estimator ˆ

λN (with σ known) ˆ λN =

  • 1

σ2HΓ(2H)N

N

  • i=0

X2

i

− 1

2H

is also strongly consistent for λ.

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SLIDE 13

Our proposal

13 / 33

The present work exposes an estimation procedure for estimating all three components of ϑ = (λ, σ, H) given the regular discretization of the sample path Y T = (Yt, 0 ≤ t ≤ T) dYt = λYtdt + σdW H

t ,

t ∈ [0, T] from discrete observations (Xn := Yn∆N, n = 0, 1, . . . , N) , where T = TN = N∆N − → +∞ and ∆N − → 0 as N − → +∞. Goal: estimate all three elements of ϑ. As H and σ can be efficiently estimated without the knowledge of λ we propose a two stage procedure.

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SLIDE 14

Quadratic generalized variations

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Let a = (a0, . . . , aK) be a discrete filter of length K + 1, K ∈ N, and of order L ≥ 1, K ≥ L, i.e.

K

  • k=0

akkℓ = 0 for 0 ≤ ℓ ≤ L − 1 and

K

  • k=0

akkL = 0. (2) Let it be normalized with

K

  • k=0

(−1)1−kak = 1 . (3) In the following, we will also consider dilatated filter a2 associated to a defined by a2

k =

ak′ if k = 2k′

  • therwise.

for 0 ≤ k ≤ 2K . Since

2K

  • k=0

a2

kkr = 2r K

  • k=0

krak, filter a2 as the same order than a.

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SLIDE 15

Quadratic generalized variations estimators of H and σ

15 / 33

Denote by VN,a =

N−K

  • i=0

K

  • k=0

akXi+k 2 the generalized quadratic variations associated to the filter a (see for instance [7]). Then, the estimators of H and σ are as follows

  • HN = 1

2 log2 VN,a2 VN,a and

  • σN =

 −2 · VN,a

  • k,ℓ akaℓ|k − ℓ|2

HN∆2 HN N

 

1 2

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SLIDE 16

Properties of estimators of H and σ

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Theorem 1. Let a be a filter of order L ≥ 2. Then, both estimators HN and σN are strongly consistent, i.e. ( HN, σN) a.s. − → (H, σ) as N − → +∞. Moreover, we have asymptotical normality property, i.e. as N → +∞, for all H ∈ (0, 1), √ N( HN − H)

L

− → N(0, Γ1(ϑ, a)) and √ N log N ( σN − σ)

L

− → N(0, Γ2(ϑ, a)) where Γ1(ϑ, a) and Γ2(ϑ, a) symmetric definite positive matrices depending on σ, H, λ and the filter a (see next slide). Proof: based on an application of [7, Theorem 3(i)].

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SLIDE 17

Asymptotic variances of ˆ HN and ˆ σN

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Let ρam,an

H

(i) =

mK

  • m=0

nK

  • ℓ=0

am

k an ℓ |mk − nℓ + i|2H

(mn)H

k,ℓ

akaℓ|k − ℓ|2H Γ1(ϑ, a) = 1 2 log(2)2

  • j∈Z
  • ρa,a

H (i)2 + ρa2,a2 H

(i)2 − 2ρa,a2

H

(i)2 and Γ2(ϑ, a) = σ2 4 Γ1(ϑ, a) see also [3].

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SLIDE 18

Properties of estimators of H and σ

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Remark 1. Classical filters of order L ≥ 1 are defined by ak = cL,k = (−1)1−k 2K K k

  • = (−1)1−k

2K K! k!(K − k)! for 0 ≤ k ≤ K. Daubechies filters of even order can also be considered (see [4]), for instance the

  • rder 2 Daubechies’ filter:

1 √ 2 (.4829629131445341, −.8365163037378077, .2241438680420134, .1294095225512603)

Remark 2. For classical order 1 quadratic variations (L = 1) and a =

  • −1

2, 1 2

  • we

can also obtain consistency for any value of H, but the central limit theorem holds

  • nly for H < 3

4 (see [7]).

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SLIDE 19

Estimator of λ

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From [5], we know the following result lim

t− →∞ Var(Yt) = lim t− →∞

1 t t Y 2

t dt = σ2Γ (2H + 1)

2λ2H =: µ2 . This gives a natural plug-in estimator of λ, namely

  • λN =

  2 µ2,N

  • σ2

  • 2

HN + 1

1 2 HN

where µ2,N is the empirical moment of order 2, i.e

  • µ2,N = 1

N

N

  • n=1

X2

n.

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SLIDE 20

Properties of the estimator of λ

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Theorem 2. Let H ∈ 1

2, 3 4

  • and a mesh satisfying the condition N∆p

N −

→ 0, p > 1, as N − → +∞. Then, as N − → +∞,

  • λN

a.s.

− → λ and

  • TN
  • λN − λ
  • L

− → N(0, Γ3(ϑ)), where Γ3(ϑ) = λ σH

2H

2 and σ2

H = (4H − 1)

  • 1 + Γ(1 − 4H)Γ(4H − 1)

Γ(2 − 2H)Γ(2H)

  • .

(4)

  • Proof. based on [5], [9, Lemma 8], [8] and [2].
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SLIDE 21

Properties of the estimator of λ

21 / 33

Remark 3. The different conditions on ∆N raise the question of whether such a rate actually exists. One possible mesh is ∆N = log N

N .

Remark 4. As in the classical case H = 1

2, the limit variance Γ3(ϑ) does not

depend on the diffusion coefficient σ. Let us also notice that the quantity σ2

H

appearing in Γ3(ϑ) is an increasing function of H.

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SLIDE 22

Monte Carlo Analysis

22 / 33

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SLIDE 23

Performance of ˆ HN and ˆ σN

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Let λ = 2 and let σ = 1, 2 for H = 0.5, 0.7, 0.9 in dYt = −λYtdt + σdW H

t .

  • HN

H = 0.5 H = 0.7 H = 0.9 σ = 1 0.499 0.697 0.898 (0.035) (0.033) (0.031) σ = 2 0.498 0.700 0.898 (0.033) (0.034) (0.033)

  • σN

H = 0.5 H = 0.7 H = 0.9 σ = 1 1.024 1.016 1.081 (0.262) (0.282) (0.437) σ = 2 2.035 2.073 2.213 (0.510) (0.564) (1.110)

Table 1: Mean average (sd parenthesis) of 500 Monte-Carlo simulations for the estimation of H (left)

and σ (right) for different cases. Here T = 100, N = 1000 and λ = 2.

  • HN

H = 0.5 H = 0.7 H = 0.9 σ = 1 0.500 0.700 0.900 (0.003) (0.003) (0.003) σ = 2 0.500 0.700 0.900 (0.004) (0.003) (0.003)

  • σN

H = 0.5 H = 0.7 H = 0.9 σ = 1 1.000 1.001 0.999 (0.025) (0.026) (0.036) σ = 2 2.001 2.002 1.997 (0.053) (0.053) (0.073)

Table 2: Mean average (sd in parenthesis) of 500 Monte-Carlo simulations for the estimation of H (left)

and σ (right) for different cases, and for TN = 100, N = 100000 and λ = 2.

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SLIDE 24

Performance of ˆ λN

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Let λ = 0.5, 1, H = 0.5, 0.6, 0.7 with σ = 1 in dYt = −λYtdt + σdW H

t .

ˆ λN H = 0.5 H = 0.6 H = 0.7 λ = 0.5 0.093 0.214 0.353 (0.037) (0.057) (0.069) λ = 1 0.138 0.276 0.432 (0.052) (0.068) (0.078) ˆ λN H = 0.5 H = 0.6 H = 0.7 λ = 0.5 0.476 0.514 0.605 (0.148) (0.166) (0.298) λ = 1 0.906 0.940 1.005 (0.227) (0.238) (0.412)

Table 3:

Mean average (and standard deviation in parenthesis) of 500 Monte-Carlo simulation for the estimation of λ for different values of H and λ. Here σ = 1 and TN = 1 and N = 100000 (left) and TN = 100 and N = 1000 (right).

The value of TN is important for the estimation of the drift. The consistency of the estimates are valid for increasing values of TN and decreasing values of the mesh size ∆N. Moreover, the bigger H, the harder the estimation of the drift

  • parameter. This phenomena can be explained by the long-range dependence

property of the fOU process.

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SLIDE 25

Asymptotic distribution of ˆ λ

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  • 4
  • 2

2 4 0.0 0.1 0.2 0.3 Density Estimated Theoretical

Figure 1:

Kernel estimation for the density of √TN

  • λ(m)

N

− λ

  • m=1...M, M = 5000, for TN =

1000 and TN = 100000 (fill line) and the theoretical Gaussian density N(0, Γ3(ϑ)) (dashed line) for ϑ = (λ, σ, H) = (0.3, 1, 0.7) (for the value of Γ3(ϑ) see Theorem 2).

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SLIDE 26

The YUIMA package

26 / 33

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SLIDE 27

The YUIMA R package

27 / 33

The Yuima Project aims at implementing, via the yuima package, a very abstract framework to describe probabilistic and statistical properties of stochastic processes in a way which is the closest as possible to their mathematical counterparts but also computationally efficient.

it is an R package, using S4 classes and methods, where the basic class extends to SDE’s with jumps (simple Poisson, L´ evy), SDE’s driven by fBM, Markov switching regime processes, HMM, etc.

separates the data description from the inference tools and simulation schemes

the design allows for multidimensional, multi-noise processes specification

it includes a variety of tools useful in finance, like asymptotic expansion of functionals of stochastic processes via Malliavin calculus

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SLIDE 28

The yuima object

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The main object is the yuima object which allows to describe the model in a mathematically sound way. Then the data and the sampling structure can be included as well or, just the sampling scheme from which data can be generated according to the model. The package exposes very few generic functions like simulate, qmle, plot, etc. and some other specific functions for special tasks. Before looking at the details, let us see an overview of the main object.

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SLIDE 29

Yuima

Simulation

Exact Euler- Maruyama Space discr.

Nonparametrics

Covariation p-variation

Parametric Inference

High freq. Low freq. Quasi MLE Diff, Jumps, fBM Adaptive Bayes MCMC Change point

Model selection

Akaike’s LASSO- type Hypotheses Testing

Option pricing

Asymptotic expansion Monte Carlo

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SLIDE 30

The model specification

30 / 33

We consider here the three main classes of SDE’s which can be easily specified. All multidimensional and eventually parametric models.

Diffusions dXt = a(t, Xt)dt + b(t, Xt)dWt

Fractional Gaussian Noise, with H the Hurst parameter dXt = a(t, Xt)dt + b(t, Xt)dW H

t

Diffusions with jumps, L´ evy dXt = a(Xt)dt + b(Xt)dWt +

  • |z|>1

c(Xt−, z)µ(dt, dz) +

  • 0<|z|≤1

c(Xt−, z){µ(dt, dz) − ν(dz)dt}

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SLIDE 31

Fractional Gaussian Noise

31 / 33

dXt = −2Xtdt + dW H

t

> samp <- setSampling(Terminal=100, n=10000) > mod <- setModel(drift="-2*x", diffusion="1",hurst=0.7) > ou <- setYuima(model=mod, sampling=samp) > fou <- simulate(ou, xinit=1)

20 40 60 80 100

  • 1.5
  • 0.5

0.5 1.0 1.5 t x

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SLIDE 32

Estimation

32 / 33

The parameters H and σ can be estimates via the function qgv (quadratic generalized variations)

> qgv(fou)

and the parameter λ using the least squares estimator lse

> lse(fou,frac=TRUE)

For more informations and software see

http://R-Forge.R-Project.org/projects/yuima

THANKS

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SLIDE 33

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