beyond the black-scholes-merton modelpjhdent/introefcollegeiii.pdfoverview 1 limitations of the...

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Limitations of the Black-Scholes model Stochastic volatility models Fractional Brownian motion models Concluding remarks Beyond the Black-Scholes-Merton model Harry van Zanten (TU/e) Econophysics Lecture Leiden, November 5, 2009 Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

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Page 1: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

Beyond the Black-Scholes-Merton model

Harry van Zanten (TU/e)

Econophysics LectureLeiden, November 5, 2009

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

Page 2: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

Overview

1 Limitations of the Black-Scholes model

2 Stochastic volatility models

3 Fractional Brownian motion models

4 Concluding remarks

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

Page 3: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

Limitations of the Black-Scholes model

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

Page 4: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

Black-Scholes model

Good news: it is a nice, well-behaved model

simple, mathematically tractable

no arbitrage, completeness

explicit expressions for the basic options

explicit hedging strategies

can use PDE techniques for pricing

can use stochastic analysis tools

Bad news: it does not model what we actually see!...

volatility smile

statistical analysis

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

Page 5: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

Black-Scholes model

Good news: it is a nice, well-behaved model

simple, mathematically tractable

no arbitrage, completeness

explicit expressions for the basic options

explicit hedging strategies

can use PDE techniques for pricing

can use stochastic analysis tools

Bad news: it does not model what we actually see!...

volatility smile

statistical analysis

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

Page 6: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

Assumptions in the Black-Scholes model

Asset prices modeled by a geometric Brownian motion:

St = S0eµt+σWt ,

where

µ : drift, σ : volatility, W : Brownian motion.

Recall:

W0 = 0,

Wt −Ws is independent of (Wu : u ≤ s) for all t ≥ s,

Wt −Ws ∼ N(0, t − s),

t 7→Wt continuous.

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

Page 7: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

Geometric Brownian motion

0 200 400 600 800 1000

010

2030

4050

60

Figure: Typical sample path of a geometric Brownian motion

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

Page 8: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

Returns in the Black-Scholes-Merton model

For t ≥ s, let

Rs,t =St − Ss

Ss

be the return over the time interval [s, t].

In the BSM-model:

Rs,t = eµ(t−s)+σ(Wt−Ws) − 1 ≈ µ(t − s) + σ(Wt −Ws).

Hence:

returns over disjoint time intervals are independent,

returns are (approximately) normally distributed.

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

Page 9: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

Returns in the Black-Scholes-Merton model

Q: is this what we see in actual asset price data?

A: that depends...

It turns out that the time-scale at which you look plays a crucialrole!

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

Page 10: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

Returns in the Black-Scholes-Merton model

Q: is this what we see in actual asset price data?

A: that depends...

It turns out that the time-scale at which you look plays a crucialrole!

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

Page 11: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

Returns in the Black-Scholes-Merton model

Q: is this what we see in actual asset price data?

A: that depends...

It turns out that the time-scale at which you look plays a crucialrole!

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

Page 12: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

A look at some real asset price data

Data:

Daily AEX index data

Minute-by-minute Philips stockprice data

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

Page 13: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

AEX data

0 50 100 150 200 250

340

360

380

400

daily AEX index

0 50 100 150 200 250

-0.02

-0.01

0.00

0.01

0.02

daily AEX returns

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

Page 14: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

AEX data analysis

-3 -2 -1 0 1 2 3

-0.02

0.00

0.02

Normal Q-Q Plot

Theoretical Quantiles

Sam

ple

Qua

ntile

s

Histogram of r

r

Frequency

-0.02 -0.01 0.00 0.01 0.02

010

2030

0 5 10 15 20

0.0

0.4

0.8

Lag

ACF

Autocorrelations r

0 5 10 15 20

0.0

0.4

0.8

Lag

ACF

Autocorrelations r*r

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

Page 15: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

Philips data

0 100 200 300 400 500

438.2

438.4

438.6

438.8

439.0

439.2

439.4

minute by minute Philips stock

0 100 200 300 400 500

-5e-04

0e+00

5e-04

1e-03

minute by minute Philips returns

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

Page 16: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

Philips data analysis

-3 -2 -1 0 1 2 3

-5e-04

5e-04

Normal Q-Q Plot

Theoretical Quantiles

Sam

ple

Qua

ntile

s

Histogram of r

r

Frequency

-5e-04 0e+00 5e-04 1e-03

050

100

200

0 5 10 15 20 25

0.0

0.4

0.8

Lag

ACF

Autocorrelations r

0 5 10 15 20 25

0.0

0.4

0.8

Lag

ACF

Autocorrelations r*r

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

Page 17: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

Typical features of asset price data

heavy-tailed returns

squared returns are positively correlated

long-range dependence in returns

variable volatility

volatility clustering

...

Can we find sensible models that capture these features?

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

Page 18: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

Typical features of asset price data

heavy-tailed returns

squared returns are positively correlated

long-range dependence in returns

variable volatility

volatility clustering

...

Can we find sensible models that capture these features?

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

Page 19: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

Issues surrounding model building for asset prices

What do we want?

Model should reflect observed statistical properties

Model should make sense economically

Model should allow pricing/hedging

Would like to have a “microscopic”, “physical” justification

This turns out to be a lot to ask for...

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

Page 20: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

Issues surrounding model building for asset prices

What do we want?

Model should reflect observed statistical properties

Model should make sense economically

Model should allow pricing/hedging

Would like to have a “microscopic”, “physical” justification

This turns out to be a lot to ask for...

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

Page 21: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

Issues surrounding model building for asset prices

What do we want?

Model should reflect observed statistical properties

Model should make sense economically

Model should allow pricing/hedging

Would like to have a “microscopic”, “physical” justification

This turns out to be a lot to ask for...

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

Page 22: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

Issues surrounding model building for asset prices

What do we want?

Model should reflect observed statistical properties

Model should make sense economically

Model should allow pricing/hedging

Would like to have a “microscopic”, “physical” justification

This turns out to be a lot to ask for...

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

Page 23: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

Issues surrounding model building for asset prices

What do we want?

Model should reflect observed statistical properties

Model should make sense economically

Model should allow pricing/hedging

Would like to have a “microscopic”, “physical” justification

This turns out to be a lot to ask for...

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

Page 24: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

Issues surrounding model building for asset prices

What do we want?

Model should reflect observed statistical properties

Model should make sense economically

Model should allow pricing/hedging

Would like to have a “microscopic”, “physical” justification

This turns out to be a lot to ask for...

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

Page 25: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

Some attempts to construct better models

Stochastic volatility models

Idea: replace the constant volatility σ by a stochastic process.

Non-Brownian motion models

Idea: replace the Brownian motion by a different process drivingthe stock-price fluctuations.

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

Page 26: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

Stochastic volatility models

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

Page 27: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

Stochastic volatility

In the Black-Scholes-Merton model, the log-price processXt = log St satisfies

dXt = µ dt + σ dWt .

A stochastic volatility model postulates that

dXt = µt dt + σt dWt ,

for (σt : t ≥ 0) a stochastic process.

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

Page 28: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

Why stochastic volatility?

statistical properties: in general much better

economic properties: incompleteness!

pricing/hedging: involved/not always possible

“microscopic”, “physical” justification: perhaps reasonable?

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

Page 29: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

Examples of stochastic volatility models

Heston:

dσ2t = α(θ − σ2

t ) dt + τ√σ2

t dBt .

GARCH-type:

dσ2t = α(θ − σ2

t ) dt + τσ2t dBt .

3/2 model:

dσ2t = α(θ − σ2

t ) dt + τ(σ2t )3/2 dBt .

...

Which one should we use?

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

Page 30: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

Nonparametric estimation of stochastic volatility models

Idea: use nonparametric estimator to choose the statistically mostreasonable parametric model.

hand picture in Figure 3. Based on computations of the mean and varianceof the estimate, with h = 0.7, we have also fitted a normal density by handand compared it to the kernel deconvolution estimator. The result is givenas the right hand picture in Figure 3. The resemblance is remarkable.

500 1000 1500 2000 2500

100

200

300

400

500

600

500 1000 1500 2000 2500

5.5

6

6.5

Figure 1: AEX. Left: daily closing values. Right: log of the daily closingvalues.fig:10

500 1000 1500 2000 2500

-0.06

-0.04

-0.02

0.02

0.04

500 1000 1500 2000 2500

-25

-20

-15

-10

Figure 2: AEX. Left: the values of Xt, i.e. the centered daily log returns.Right: log(X2

t ) .fig:11

The kernel used to compute the estimates is a kernel from Wand (1998),with ! = 3 and A = 8,

w(x) =48x(x2 ! 15) cos x! 144(2x2 ! 5) sin x

"x7. (12) simkernel

It has characteristic function

#w(t) = (1! t2)3, |t| " 1. (13) simchar

The bandwidths are chosen by hand. The estimates have been computedby fast Fourier transforms using the Mathematica 4.2 package.

8

-25 -20 -15 -10 -5

0.025

0.05

0.075

0.1

0.125

0.15

0.175

-25 -20 -15 -10 -5

0.025

0.05

0.075

0.1

0.125

0.15

0.175

Figure 3: AEX. Left: The estimate of the density of log(!2t ) with h = 0.7.

Right: The normal fit to the log(!2t ). The dashed line is the normal density

and the solid line the kernel estimate.fig:13

This is actually the same example as in our paper Van Es et al. (2005)on volatility density estimation for discrete time models. The estimator (7)presented here is, as a function of the sampled data, exactly the same asthe one for the discrete time models. The di!erence lies in the choice ofunderlying model. In the present paper the model is a discretely sampledcontinuous time process, while in Van Es et al. (2005) it is a discrete timeprocess. For the latter type of models the discretization step in the beginningof this section is not necessary since these models satisfy an exact convolutionstructure.

4 Wavelet deconvolution

Starting point is again the simplified model (5). Contrary to the previ-ous section, we are now interested in estimating the accumulated squaredvolatility over an interval of length ". We assume having observations of Sat times k" to our disposal, but now with " fixed (low frequency observa-tions). The transformed increments log(Si!!S(i!1)!)2 are then distributedas Yi = Xi + "i, where

Xi = log! i!

(i!1)!!2

u du, "i = log Z2i ,

and Zi is an i.i.d. sequence of standard Gaussian random variables, indepen-dent of !. The sequence Xi is stationary and we assume that its marginaldensity f exists, i.e. f is the density of

log! !

0!2

u du.

Of course, estimating f is equivalent with estimating the density of theaggregated squared volatility

" !0 !2

u du.

9

Figure: AEX data and estimator of the density of log σ2t .

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

Page 31: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

“Physical” justification

Reasonable that volatility has its own dynamics, partly independentof the dynamics of individual stocks (“temperature” of themarket).

Volatility clustering and switching between “calm” and “excited”periods may be explained e.g. by a double well potential.

Figure: Potential V

SDE for volatility:

dσ2t = V ′(σ2

t ) dt + τ(σ2(Xt)) dBt ,

where B is a second Brownian motion.

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

Page 32: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

Completeness of the Black-Scholes market

The Black-Scholes market is complete: every “reasonable”contingent claim can be perfectly hedged by a self-financingportfolio consisting of stocks and bonds.

Intuitive reason: there are as many independent risky assets assources of randomness. Or: by trading the stock the randomnesscaused by the Brownian motion can be “neutralized”. In otherwords: there are enough risky assets to “hedge away” therandomness.

Technical reason: there is a unique martingale measure.

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

Page 33: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

Incompleteness of stochastic volatility models

In SV-models typically more sources of randomness than riskyassets.

As a result, not every derivative can be perfectly hedged in a SVmodel: incompleteness.

Some consequences:

have to resort to e.g. super hedging or quantile hedging,

for non-attainable derivatives, there is a whole interval ofpossible no-arbitrage prices,

need additional considerations to choose a specific price (e.g.utility considerations).

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

Page 34: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

Statistical soundness vs. completeness

Roughly speaking:

Models having the desirable property of completeness are typicallynot realistic from the statistical point of view.

Statistically sound models are typically incomplete and hence giverise to more involved pricing procedures.

No widespread consensus...

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

Page 35: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

Statistical soundness vs. completeness

Roughly speaking:

Models having the desirable property of completeness are typicallynot realistic from the statistical point of view.

Statistically sound models are typically incomplete and hence giverise to more involved pricing procedures.

No widespread consensus...

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

Page 36: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

Fractional Brownian motion models

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

Page 37: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

Where does the Brownian motion come from?

Donsker (’52):

Z1,Z2, . . . , i.i.d. EZi = 0, VarZi = 1.

X(n)t =

1√n

[nt]∑

i=1

Zi , t ∈ [0, 1].

Theorem.

X (n) ⇒ Brownian motion

in D[0, 1].

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

Page 38: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

Donsker’s theorem visualized

2 4 6 8 10

12

34

5

0 20 40 60 80 100

-10

-6-2

0 200 400 600 800

010

30

0 2000 6000 10000

-100

050

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

Page 39: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

What if there is a memory in the system?

Davydov (’70), Taqqu (’75):

Z1,Z2, . . . , stationary, . . . , EZi = 0, Var(Z1 + · · ·+ Zn) ∼ n2H ,H ∈ (0, 1), . . .

X(n)t =

1√Var(Z1 + · · ·+ Zn)

[nt]∑

i=1

Zi , t ∈ [0, 1].

Theorem.

X (n) ⇒ fractional Brownian motion

in D[0, 1].

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

Page 40: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

Fractional Brownian motion

Fractional Brownian motion (fBm):

Gaussian process W H = (W Ht : t ≥ 0), centered,

EW Hs W H

t =1

2(t2H + s2H − |t − s|2H),

with H ∈ (0, 1) the Hurst index.

Kolmogorov (’40), Mandelbrot & Van Ness (’68)

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

Page 41: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

Fractional Brownian motion properties

Basic properties:

- H = 1/2: ordinary Brownian motion,- stationary increments,- H-self similar: for all a > 0, (a−HW H

at : t ≥ 0) has the same lawas W H ,- sample paths are “H-smooth”,- for H > 1/2, long range dependence:∑

E(W Hn −W H

n−1)W H1 =∞,

- for H 6= 1/2: not Markov, not a (semi)martingale.- E(W H

t −W Hs )2 = |t − s|2H : for H > 1/2 the process is

superdiffusive, for H < 1/2 it is subdiffusive.

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

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Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

Fractional Brownian motion paths

0.0 0.2 0.4 0.6 0.8 1.0

-2.5

-2.0

-1.5

-1.0

-0.5

0.0

0.0 0.2 0.4 0.6 0.8 1.0

0.0

0.1

0.2

0.3

0.4

0.5

Figure: H = 0.3, H = 0.8

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

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Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

Fractional Black-Scholes model

Model for asset prices:

St = S0eµt+σW H

t ,

where

µ : drift, σ : volatility, W H : fractional Brownian motion.

Idea: Gaussianity plausible on appropriate time scales, fBm allowsfor more realistic dependence structure.

Data analysis studies: typically H ≈ 0.6.

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

Page 44: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

Properties of the fBm model

Good news:

Statistical fit better than for BS model.

Microscopic explanation as scaling limit.

Bad news:

Can not use stochastic calculus or PDE tools.

The model allows for arbitrage!

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

Page 45: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

Properties of the fBm model

Good news:

Statistical fit better than for BS model.

Microscopic explanation as scaling limit.

Bad news:

Can not use stochastic calculus or PDE tools.

The model allows for arbitrage!

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

Page 46: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

Making sense of fBm models

Arbitrage opportunities arise in the usual setup:

No transaction costs,

Large class of continuous-time trading strategies allowed.

Possible ways to remove arbitrage opportunities:

Reduce the set of allowed trading strategies (e.g. only finitelymany trading times).

Introduce transaction costs (e.g. proportional to volumestraded).

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

Page 47: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

Making sense of fBm models

Arbitrage opportunities arise in the usual setup:

No transaction costs,

Large class of continuous-time trading strategies allowed.

Possible ways to remove arbitrage opportunities:

Reduce the set of allowed trading strategies (e.g. only finitelymany trading times).

Introduce transaction costs (e.g. proportional to volumestraded).

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

Page 48: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

Models with transaction costs

Recent developments:

After introducing transaction costs, BM can be replaced by anycontinuous process X with conditional full support:

P(

sups∈[t,T ]

|Xs − Xt − f (s)| < ε |Xs : s ≤ t)> 0

for all 0 < t < T , continuous f : [t,T ]→ R with f (0) = 0, andε > 0.

This leads to an arbitrage-free model.

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

Page 49: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

Models with transaction costs

Let X be a Gaussian process with stationary increments andspectral measure µ(dλ) = f (λ) dλ.

Theorem.

If ∫ ∞

1

log f (λ)

λ2dλ > −∞,

then X has conditional full support.

Example: for the fBm with Hurst index H, f (λ) = cH |λ|1−2H .Hence, the fBm has CFS.

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

Page 50: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

Models with transaction costs

For these models with general, non-semimartingale price processes:

How about hedging?

How about pricing?

Matters are currently unresolved. . .

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

Page 51: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

Models with transaction costs

For these models with general, non-semimartingale price processes:

How about hedging?

How about pricing?

Matters are currently unresolved. . .

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

Page 52: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

Concluding remarks

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

Page 53: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

The Black-Scholes-Merton model does not properly describeall aspects of real asset price data.

Stochastic volatility or fBm models typically do better.

Stochastic volatility: incompleteness, how to choose derivativeprices?

Fractional Brownian motion: arbitrage, how to deal with it?

The debate is ongoing. . .

THANKS FOR YOUR ATTENTION!

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model

Page 54: Beyond the Black-Scholes-Merton modelpjhdent/introefcollegeIII.pdfOverview 1 Limitations of the Black-Scholes model 2 Stochastic volatility models 3 Fractional Brownian motion models

Limitations of the Black-Scholes modelStochastic volatility models

Fractional Brownian motion modelsConcluding remarks

The Black-Scholes-Merton model does not properly describeall aspects of real asset price data.

Stochastic volatility or fBm models typically do better.

Stochastic volatility: incompleteness, how to choose derivativeprices?

Fractional Brownian motion: arbitrage, how to deal with it?

The debate is ongoing. . .

THANKS FOR YOUR ATTENTION!

Harry van Zanten (TU/e) Beyond the Black-Scholes-Merton model