Time Series vs SDEs Diffusions Consider the AR(1) process. It is a - - PowerPoint PPT Presentation

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Time Series vs SDEs Diffusions Consider the AR(1) process. It is a - - PowerPoint PPT Presentation

Financial econometrics based on stochastic differential equations and the sde package S.M. Iacus (University of Milan) Rennes, useR! 2009, July 8th - 10th 1 / 17 Time Series vs SDEs Diffusions Consider the AR(1) process. It is a discrete-time


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Financial econometrics based on stochastic differential equations and the sde package

S.M. Iacus (University of Milan)

Rennes, useR! 2009, July 8th - 10th

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Time Series vs SDEs

Diffusions Exact likelihood Pseudo-likelihood Simulated likelihood method Hermite expansion

2 / 17

Consider the AR(1) process. It is a discrete-time random process, defined as

Xt = θXt−1 + ǫt, X0 = x0, ǫt :

i.i.d. random variables (noise)

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Time Series vs SDEs

Diffusions Exact likelihood Pseudo-likelihood Simulated likelihood method Hermite expansion

2 / 17

Consider the AR(1) process. It is a discrete-time random process, defined as

Xt = θXt−1 + ǫt, X0 = x0, ǫt :

i.i.d. random variables (noise) Its continuous-time counter part (the Ornstein-Uhlenbeck process), written in differential form, looks like

dXt = −θXtdt + dWt, X0 = x0, Wt :

the Wiener process (noise)

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SLIDE 4

Time Series vs SDEs

Diffusions Exact likelihood Pseudo-likelihood Simulated likelihood method Hermite expansion

2 / 17

Consider the AR(1) process. It is a discrete-time random process, defined as

Xt = θXt−1 + ǫt, X0 = x0, ǫt :

i.i.d. random variables (noise) Its continuous-time counter part (the Ornstein-Uhlenbeck process), written in differential form, looks like

dXt = −θXtdt + dWt, X0 = x0, Wt :

the Wiener process (noise) A stochastic differential equation models a dynamical system with feedback by adding continuous time shocks

dXt = b(Xt)dt + σ(Xt)dWt

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Time Series vs SDEs

Diffusions Exact likelihood Pseudo-likelihood Simulated likelihood method Hermite expansion

3 / 17

In continuous time models: time between Xt and Xt+∆t matters ! The length

  • f ∆t is crucial as well.
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Time Series vs SDEs

Diffusions Exact likelihood Pseudo-likelihood Simulated likelihood method Hermite expansion

3 / 17

In continuous time models: time between Xt and Xt+∆t matters ! The length

  • f ∆t is crucial as well.

In time-series models: nothing happens (probabilistically) between Xt and

Xt−1

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Time Series vs SDEs

Diffusions Exact likelihood Pseudo-likelihood Simulated likelihood method Hermite expansion

3 / 17

In continuous time models: time between Xt and Xt+∆t matters ! The length

  • f ∆t is crucial as well.

In time-series models: nothing happens (probabilistically) between Xt and

Xt−1

Why this matters? An example: according to McCrorie & Chambers (2006, J. of Econ.) and others, “spurious Granger causality [tested with VAR models] is

  • nly a consequence of the intervals in which economic data are generated

being finer than the econometrician’s sampling interval.” Conclusions: assume a continuous time model (SDE). Discretize that, build a VAR from the discretized SDE and the spurious Granger causality vanishes!

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Time Series vs SDEs

Diffusions Exact likelihood Pseudo-likelihood Simulated likelihood method Hermite expansion

3 / 17

In continuous time models: time between Xt and Xt+∆t matters ! The length

  • f ∆t is crucial as well.

In time-series models: nothing happens (probabilistically) between Xt and

Xt−1

Why this matters? An example: according to McCrorie & Chambers (2006, J. of Econ.) and others, “spurious Granger causality [tested with VAR models] is

  • nly a consequence of the intervals in which economic data are generated

being finer than the econometrician’s sampling interval.” Conclusions: assume a continuous time model (SDE). Discretize that, build a VAR from the discretized SDE and the spurious Granger causality vanishes! Rephrasing: why using a binomial distribution if your underlying model is a Gaussian?

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A few examples of SDEs

Diffusions Exact likelihood Pseudo-likelihood Simulated likelihood method Hermite expansion

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gBm : dXt = µXtdt + σXtdWt CIR : dXt = (θ1 + θ2Xt)dt + θ3

√XtdWt

CKLS : dXt = (θ1 + θ2Xt)dt + θ3Xθ4

t dWt

nonlinear mean reversion (A¨

ıt-Sahalia)

dXt = (α−1X−1

t

+ α0 + α1Xt + α2X2

t )dt + β1Xρ t dWt

double Well potential (bimodal behaviour, highly nonlinear)

dXt = (Xt − X3

t )dt + dWt

Jacobi diffusion (political polarization):

dXt = −θ

  • Xt − 1

2

  • dt +
  • θXt(1 − Xt)dWt

radial Ornstein-Uhlenbeck : dXt = (θX−1

t

− Xt)dt + dWt

hyperbolic diffusion : dXt = σ2

2

  • β − γ

Xt

δ2+(Xt−µ)2

  • dt + σdWt
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Diffusion processes solutions to SDEs

Diffusions Exact likelihood Pseudo-likelihood Simulated likelihood method Hermite expansion

5 / 17

From the statistical point of view, we are interested in the parametric family of diffusion process solutions of the SDE

dXt = b(Xt, θ)dt + σ(Xt, θ)dWt, X0 = x0, t ∈ [0, T] θ = (α, β) ∈ Θα × Θβ = Θ, where Θα ⊂ Rp and Θβ ⊂ Rq.

Observations always come in discrete time form at some times ti = i∆n,

i = 0, 1, 2, ..., n, where ∆n is the length of the steps. We denote the

  • bservations by Xn := {Xi = Xti}0≤i≤n.
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Diffusion processes solutions to SDEs

Diffusions Exact likelihood Pseudo-likelihood Simulated likelihood method Hermite expansion

5 / 17

From the statistical point of view, we are interested in the parametric family of diffusion process solutions of the SDE

dXt = b(Xt, θ)dt + σ(Xt, θ)dWt, X0 = x0, t ∈ [0, T] θ = (α, β) ∈ Θα × Θβ = Θ, where Θα ⊂ Rp and Θβ ⊂ Rq.

Observations always come in discrete time form at some times ti = i∆n,

i = 0, 1, 2, ..., n, where ∆n is the length of the steps. We denote the

  • bservations by Xn := {Xi = Xti}0≤i≤n.

Different sampling schemes, different statistical procedures:

  • 1. Large sample asymptotics: ∆ fixed, T = n∆ → ∞ as n → ∞
  • 2. High frequency: T = n∆n fixed, ∆n → 0 as n → ∞
  • 3. Rapidly increasing design: T = n∆ → ∞, ∆n → 0 as n → ∞ under

the additional condition n∆k

n → 0 for k > 1

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Likelihood in discrete time

Diffusions Exact likelihood Pseudo-likelihood Simulated likelihood method Hermite expansion

6 / 17

By Markov property of diffusion processes, the likelihood has this form

Ln(θ) =

n

  • i=1

pθ (∆, Xi|Xi−1)pθ(X0)

Problem: the transition density pθ (∆, Xi|Xi−1) is often not available! Only for OU, CIR and gBm

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Likelihood in discrete time

Diffusions Exact likelihood Pseudo-likelihood Simulated likelihood method Hermite expansion

6 / 17

By Markov property of diffusion processes, the likelihood has this form

Ln(θ) =

n

  • i=1

pθ (∆, Xi|Xi−1)pθ(X0)

Problem: the transition density pθ (∆, Xi|Xi−1) is often not available! Only for OU, CIR and gBm Solutions:

discretization of the SDE (Euler, Milstein, Ozaki, etc) simulation method hermite polynomial expansion partial differential equations

  • ther approximations of the transition density
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Local Gaussian Approximation. Euler Scheme.

7 / 17

By Euler discretization of the SDE : dXt = b(Xt, θ)dt + σ(Xt, θ)dWt

Xt+∆t − Xt = b(Xt, θ)∆t + σ(Xt, θ)(Wt+∆t − Wt),

we get an approximate transition density which is Gaussian. This is widely seen in applied

  • contexts. But is this approximation good or not? In general no!

For example, for gBm, the true transition density is a log-normal and the Euler schemes provides

  • nly a Gaussian approximation!

It is possible to prove that estimators are not even consistent for non negligible ∆.

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Euler, ∆ and bias

Diffusions Exact likelihood Pseudo-likelihood Simulated likelihood method Hermite expansion

8 / 17

Consider OU model

dXt = (θ1 − θ2Xt)dt + θ3dWt, X0 = x0

Both true and Euler approximation are Gaussian respectively with mean and variance

m(∆, x) = xe−θ2∆ + θ1 θ2

  • 1 − e−θ2∆

, v(∆, x) = θ2

3

  • 1 − e−2θ2∆

2θ2 ,

and (Euler)

mEuler(∆, x) = x(1 − θ2∆) + θ1∆ , vEuler(∆, x) = θ2

3∆ ,

Only under high-frequency setting, i.e. ∆ → 0, the approximation is acceptable.

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Simulated likelihood method

Diffusions Exact likelihood Pseudo-likelihood Simulated likelihood method Hermite expansion

9 / 17

Let pθ(∆, y|x) be the true transition density of Xt+∆ at point y given

Xt = x. Consider a δ << ∆, for example δ = ∆/N for N large enough,

and then use the Chapman-Kolmogorov equation as follows:

pθ(∆, y|x) =

  • pθ(δ, y|z)pθ(∆ − δ, z|x)dz = Ez{pθ(δ, y|z)|∆ − δ} ,

It means that pθ(∆, y|x) is seen as the expected value over all possible transitions of the process from time t + (∆ − δ) to t + ∆, taking into account that the process was in x at time t. So we need simulations!

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What about N? We need many simulations

10 / 17

Example: approximation for the CIR model

0.00 0.05 0.10 0.15 0.20 5 10 15 20 25 x conditional density exact N=2 N=5 N=10

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What about N? We need many simulations

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Example: approximation for the CIR model

0.00 0.05 0.10 0.15 0.20 5 10 15 20 25 x conditional density exact N=2 N=5 N=10

We need many simulations (N) for each time points (Xti, Xti+∆). But not all simulation schemes are stable for all models

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Numerical instability. Up|Down ∆ = 0.1|0.25

11 / 17

A¨ ıt-Sahalia process dXt = (5 − 11Xt + 6X2

t − X3 t )dt + dWt,

X0 = 5

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Numerical instability. Up|Down ∆ = 0.1|0.25

11 / 17

A¨ ıt-Sahalia process dXt = (5 − 11Xt + 6X2

t − X3 t )dt + dWt,

X0 = 5

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A¨ ıt-Sahalia’s approximation

Diffusions Exact likelihood Pseudo-likelihood Simulated likelihood method Hermite expansion

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True likelihood (continuous line), Euler approximation (dashed line), A¨ ıt-Sahalia approximation (dotted line). Where is the dotted line? Coincides with the continuous line! Model dXt = βXtdt + dWt

−3 −2 −1 1 2 3 26.0 26.5 27.0 27.5 β log−likelihood

no need to have ∆ small, but (was) very difficult to implement!

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The sde package

13 / 17

The sde package implements A¨ ıt-Sahalia method. It also implements the following methods

local Gaussian (dcEuler), Elerian (dcElerian), Ozaki (dcOzaki) and Shoji-Ozaki

(dcShoji) approximations

Simulated Likelihood Method (dcSim), Kessler’s (dcKessler) and A¨

ıt-Sahalia (HPloglik) approximations all of them can be passed to the mle function in R or used to build appropriate likelihood functions.

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The sde package

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The sde package also implements many simulation schemes, including: Euler, Milstein, Milstein2, Elerian, Ozaki, Ozaki-Shoji, Exact Simulation Scheme, Simulation from conditional distribution, Predictor-Correction scheme, etc via the unique sde.sim function

sde.sim(t0 = 0, T = 1, X0 = 1, N = 100, delta, drift, sigma, drift.x, sigma.x, drift.xx, sigma.xx, drift.t, method = c("euler", "milstein", "KPS", "milstein2", "cdist","ozaki","shoji","EA"), alpha = 0.5, eta = 0.5, pred.corr = T, rcdist = NULL, theta = NULL, model = c("CIR", "VAS", "OU", "BS"), k1, k2, phi, max.psi = 1000, rh, A, M=1)

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The sde.sim function

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For the OU process, dXt = −5Xtdt + 3.5dWt, it is as easy as

> d <- expression(-5 * x) > s <- expression(3.5) > sde.sim(X0=10,drift=d, sigma=s) -> X > str(X) Time-Series [1:101] from 0 to 1: 10 9.32 8.79 8.89 8.48 ...

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The sde.sim function

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For the CIR model dXt = (6 − 3Xt)dt + 2√XtdWt

d <- expression( 6-3*x ) s <- expression( 2*sqrt(x) ) sde.sim(X0=10,drift=d, sigma=s) -> X

  • r, via model name

sde.sim(X0=10, theta=c(6, 3, 2), model="CIR") -> X

  • r, via exact conditional distribution rcCIR (also implemented in sde)

sde.sim(X0=10, theta=c(6, 3, 2), rcdist=rcCIR, method="cdist") -> X

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Also in the sde package

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The package also implements other estimation procedures

estimating functions (linear, quadratic, martingale) GMM (but be careful, not really what you want to use with SDE!) approximate AIC statistics for model selection (sdeAIC) φ-divergence test statistics for parametric hypotheses testing (not in the book) change point (cpoint) analysis; both parametric and nonparametric non parametric estimation of drift (ksdrift) and diffusion (ksdiff) coefficients Markov Operator distance (MOdist) for clustering of SDE paths

The companion book: Simulation and Inference for Stochastic Differential Equations, with R Examples, Springer (2008).