An analytical perturbative solution to the Merton–Garman model using symmetries

AuthorNathaniel Wiesendanger Shaw,Xavier Calmet
Published date01 January 2020
Date01 January 2020
DOIhttp://doi.org/10.1002/fut.22061
© 2019 The Authors. The Journal of Futures Markets published by Wiley Periodicals, Inc.
J Futures Markets. 2020;40:322. wileyonlinelibrary.com/journal/fut
|
3
Received: 30 May 2019
|
Accepted: 2 September 2019
DOI: 10.1002/fut.22061
RESEARCH ARTICLE
An analytical perturbative solution to the MertonGarman
model using symmetries
Xavier Calmet
1
|
Nathaniel Wiesendanger Shaw
1,2
1
School of Mathematical and Physical
Sciences, University of Sussex, Brighton,
United Kingdom
2
Business School, University of Sussex,
Falmer, Brighton, United Kingdom
Correspondence
Xavier Calmet, School of Mathematical
and Physical Sciences, University of
Sussex, Brighton BN1 9QH, United
Kingdom.
Email: x.calmet@sussex.ac.uk
Funding information
Science and Technology Facilities
Council, Grant/Award Number: ST/
P000819/1
Abstract
In this paper, we introduce an analytical perturbative solution to the
MertonGarman model. It is obtained by doing perturbation theory around
the exact analytical solution of a model which possesses a twodimensional
Galilean symmetry. We compare our perturbative solution of the MertonGar-
man model to Monte Carlo simulations and find that our solutions perform
surprisingly well for a wide range of parameters. We also show how to use
symmetries to build option pricing models. Our results demonstrate that the
concept of symmetry is important in mathematical finance.
KEYWORDS
MertonGarman model, option pricing model, perturbation theory
JEL CLASSIFICATION
C02; G10
1
|
INTRODUCTION
Calculating the price of an option is an important challenge in mathematical finance. The first attempts in that direction are
attributed to Louis Bachelier who during in his Doctoral thesis, Théorie de la spéculation, published in 1900, considered a
mathematical model of Brownian motion and its use for valuing options. This study provided the foundations for the
BlackScholes model (Black & Scholes, 1973). However, although the BlackScholes model was a breakthrough in the field, it
is widely accepted that it has limitations. In particular, the volatility is treated as a constant which is not very realistic.
Since the seminal works of Black and Scholes (1973) and Merton (1973), more sophisticated models with a
timedependent volatility have been proposed. For example, the affine Heston model (see Heston, 1993), which
assumes a timedependent volatility, with a stochastic process involving the squareroot of the stochastic
volatility, and a leverage effect, has been implemented in a large number of empirical studies (Andersen,
Benzoni, & Lund, 2002; Bakshi, Cao, & Chen, 1997; Bates, 2000, 2006; Chernov, Gallant, Ghysels, & Tauchen,
2003; Eraker, 2004; Huang & Wu, 2004; Pan, 2002, to name a few). Such models have however limitations and are
often modified artificially by combining them with models of jumps in returns and/or in volatility (such as
Benzoni, 2002; Jones, 2003). As a consequence, there is a substantial strand of literature devoted to nonaffine
volatility models, which note that the popular squareroot stochastic volatility model is not very realistic (see,
e.g., AïtSahalia & Kimmel, 2007; Chourdakis & Dotsis, 2011; Christoffersen, Jacobs, & Mimouni, 2010; Duan &
Yeh, 2010; Eraker, Johannes, & Polson, 2003; Kaeck & Alexander, 2012, to name a few). However, the issue with
such models is a general lack of closed form characteristic function, which makes pricing much more
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This is an open access article under the terms of the Creative Commons Attribution License, which permits use, distribution and reproduction in any medium, provided
the original work is properly cited.
challenging. As stated in Chourdakis and Dotsis (2011) when regarding the place of nonaffine models and the
debate of their tractability against affine models: Does analytically tractability come at the cost of empirical
misspecification?It is a useful endeavor to study the nonaffine model as we propose in this paper, if an
analytical solution for the option pricing formula can be found.
Awellknown example of such models is the MertonGarman model (Garman, 1976; Merton, 1973) which is indeed a
more realistic model as it allows for a timedependent volatility and it is not restricted to an affine model for the volatility.
However, solving nonaffine models is time consuming, as it involves numerical methods. Thus, many practitioners are still
using the BlackScholes formula to obtain a fast, albeit not necessarily very reliable, price quote for an option.
The aim of our study is twofold. We will derive an analytical approximative solution to the partial differential
equation describing the MertonGarman model, which enables one fast calculation of option prices. This requires us to
identify a symmetricversion of the model, which can easily be solved analytically. One can then reintroduce the
symmetry breaking terms of the original MertonGarman differential equation and do perturbation theory around the
symmetric solution thereby obtaining an approximative but analytical solution to the original MertonGarman
differential equation. We then propose a new approach to model building in option pricing based on the concept of
symmetry groups and representation theory. This concept has been extremely successful in modern physics. It is at the
origin of all successful models in physics, for example, in particle physics, cosmology, or solidstate physics. We note
that perturbation theory has been used in option pricing models (Aguilar, 2017; Baaquie, 1997; Baaquie, Coriano, &
Srikant, 2003; Blazhyevskyi & Yanishevsky, 2011; Kleinert & Korbel, 2016; Utama & Purqon, 2016) but here we
organize perturbation theory around a very specific solution, namely that of the symmetrical model which we will
introduce in this paper.
This paper is organized as follows. In Section 2, we derive the partial differential equation, which describes the
MertonGarman model. In Section 3, we explain how to reduce the original MertonGarman model to a simple,
symmetrical, model. We present an exact analytical solution to the symmetrical model. We then restore the original
MertonGarman model by reintroducing the symmetry breaking terms and provide an analytical perturbative solution to
the MertonGarman model. In Section 4, we compare our solutions to different numerical solutions found in the literature.
In Section 5, we propose a new approach to model building in mathematical finance. Finally, we conclude in Section 6.
2
|
THE MERTONGARMAN MODEL
In the MertonGarman model, the price of an option is dependent on the time t, the price of the underlying S, and the
volatility V. Both Sand Vare taken to be timedependent functions, and thus the MertonGarman model has the
potential to provide a more accurate calculation of an option price than, for example, the BlackScholes model.
We start from the stochastic differential equations (SDEs) for the price of the underlying Sand for the volatility V:
d
S rSdt V SdW=+
,
S
(1)
d
Vκθ Vdt ξVdW=()+ ,
αV
(2)
which resembles a stochastic, mean reverting, volatility regime. Here,
ξ
is the standard deviation of the volatility and
κ
is the speed of mean reversion to the longrun variance θ. The interest rate ris assumed to be constant. The model
described by Equations (1) and (2) covers many wellknown stochastic volatility models, for instance, setting
α
=
1
and
1/2 recovers the Hull and White (see Hull & White, 1987) and Heston models, respectively. However, we do not
constrain ourselves to either of these worlds. Here,
α
can take arbitrary values. We will denote the correlation between
the two Brownian motions
WS
and
V
by
ρ
.
We shall first consider a call option, but our results can be extended to a put option in a straightforward manner. Our
first step is to find the associated partial differential equation, which describes this model. We do so by applying the
FeynmanKac formula (see, e.g., Hull, 1997), which states that the price of a call option, as defined by the model
dynamics in Equations (1) and (2), is given by
∑∑
∂∂
C
tμtx C
xρσ txσtx C
xx rC+(,)+
1
2(, ) (, ) =0
,
i
iiij
ij ij
ij
=1 , =1
2
(3)
4
|
CALMET AND WIESENDANGER SHAW

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