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Stochastic Calculus for Finance II : Continuous-Time Models

Steven E. Shreve

Chapter 3

Brownian Motion - all with Video Answers

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Chapter Questions

03:52

Problem 1

E According to Definition 3.3.3(iii), for $0 \leq t<u$, the Brownian motion increment $W(u)-W(t)$ is independent of the $\sigma$-algebra $\mathcal{F}(t)$. Use this property and property (i) of that definition to show that, for $0 \leq t<u_1<u_2$, the increment $W\left(u_2\right)-W\left(u_1\right)$ is also independent of $\mathcal{F}(t)$.

Nick Johnson
Nick Johnson
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01:35

Problem 2

Let $W(t), t \geq 0$, be a Brownian motion, and let $\mathcal{F}(t), t \geq 0$, be a filtration for this Brownian motion. Show that $W^2(t)-t$ is a martingale. (Hint: For $0 \leq s \leq t$, write $W^2(t)$ as $(W(t)-W(s))^2+2 W(t) W(s)-W^2(s)$.)

Nick Johnson
Nick Johnson
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Problem 3

Exercise 3.3 (Normal kurtosis). The kurtosis of a random variable is defined to be the ratio of its fourth central moment to the square of its variance. For a normal random variable, the kurtosis is 3 . This fact was used to obtain (3.4.7). This exercise verifies this fact.

Let $X$ be a normal random variable with mean $\mu$, so that $X-\mu$ has mean zero. Let the variance of $X$, which is also the variance of $X-\mu$, be $\sigma^2$. In (3.2.13), we computed the moment-generating function of $X-\mu$ to be $\varphi(u)=\mathbb{E} e^{u(X-\mu)}=e^{\frac{1}{2} u^2 \sigma^2}$, where $u$ is a real variable. Differentiating this function with respect to $u$, we obtain
$$
\varphi^{\prime}(u)=\mathbb{E}\left[(X-\mu) e^{u(X-\mu)}\right]=\sigma^2 u e^{\frac{1}{2} \sigma^2 u^2}
$$
and, in particular, $\varphi^{\prime}(0)=\mathbb{E}(X-\mu)=0$. Differentiating again, we obtain
$$
\varphi^{\prime \prime}(u)=\mathbf{E}\left[(X-\mu)^2 e^{u(X-\mu)}\right]=\left(\sigma^2+\sigma^4 u^2\right) e^{\frac{1}{2} \sigma^2 u^2}
$$
and, in particular, $\varphi^{\prime \prime}(0)=\mathbf{E}\left[(X-\mu)^2\right]=\sigma^2$. Differentiate two more times and obtain the normal kurtosis formula $\mathrm{E}\left[(X-\mu)^4\right]=3 \sigma^4$.

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Problem 4

(Other variations of Brownian motion). Theorem 3.4.3 asserts that if $T$ is a positive number and we choose a partition $\Pi$ with points $0=t_0<t_1<t_2<\cdots<t_n=T$, then as the number $n$ of partition points approaches infinity and the length of the longest subinterval $\|\Pi\|$ approaches zero, the sample quadratic variation
$$
\sum_{j=0}^{n-1}\left(W\left(t_{j+1}\right)-W\left(t_j\right)\right)^2
$$
approaches $T$ for almost every path of the Brownian motion $W$. In Remark 3.4.5, we further showed that $\sum_{j=0}^{n-1}\left(W\left(t_{j+1}\right)-W\left(t_j\right)\right)\left(t_{j+1}-t_j\right)$ and $\sum_{j=0}^{n-1}\left(t_{j+1}-t_j\right)^2$ have limit zero. We summarize these facts by the multiplication rules
$$
d W(t) d W(t)=d t, \quad d W(t) d t=0, \quad d t d t=0 .
$$

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Problem 5

(Black-Scholes-Merton formula). Let the interest rate $r$ and the volatility $\sigma>0$ be constant. Let
$$
S(t)=S(0) e^{\left(r-\frac{1}{2} \sigma^2\right) t+\sigma W(t)}
$$
be a geometric Brownian motion with mean rate of return $r$, where the initial stock price $S(0)$ is positive. Let $K$ be a positive constant. Show that, for $T>0$,
$$
\mathbb{E}\left[e^{-r T}(S(T)-K)^{+}\right]=S(0) N\left(d_{+}(T, S(0))\right)-K e^{-r T} N\left(d_{-}(T, S(0))\right),
$$
where
$$
d_{ \pm}(T, S(0))=\frac{1}{\sigma \sqrt{T}}\left[\log \frac{S(0)}{K}+\left(r \pm \frac{\sigma^2}{2}\right) T\right],
$$
and $N$ is the cumulative standard normal distribution function
$$
N(y)=\frac{1}{\sqrt{2 \pi}} \int_{-\infty}^y e^{-\frac{1}{2} z^2} d z=\frac{1}{\sqrt{2 \pi}} \int_{-y}^{\infty} e^{-\frac{1}{2} z^2} d z .
$$

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Problem 6

Let $W(t)$ be a Brownian motion and let $\mathcal{F}(t), t \geq 0$, be an associated filtration.
3.10 Exercises
119
(i) For $\mu \in \mathbb{R}$, consider the Brownian motion with drift $\mu$ :
$$
X(t)=\mu t+W(t) .
$$

Show that for any Borel-measurable function $f(y)$, and for any $0 \leq s<t$, the function
$$
g(x)=\frac{1}{\sqrt{2 \pi(t-s)}} \int_{-\infty}^{\infty} f(y) \exp \left\{-\frac{(y-x-\mu(t-s))^2}{2(t-s)}\right\} d y
$$
satisfies $\mathbb{E}[f(X(t)) \mid \mathcal{F}(s)]=g(X(s))$, and hence $X$ has the Markov property. We may rewrite $g(x)$ as $g(x)=\int_{-\infty}^{\infty} f(y) p(\tau, x, y) d y$, where $\tau=t-s$ and
$$
p(\tau, x, y)=\frac{1}{\sqrt{2 \pi \tau}} \exp \left\{-\frac{(y-x-\mu \tau)^2}{2 \tau}\right\}
$$
is the transition density for Brownian motion with drift $\mu$.
(ii) For $\nu \in \mathbb{R}$ and $\sigma>0$, consider the geometric Brownian motion
$$
S(t)=S(0) e^{\sigma W(t)+\nu t} .
$$

Set $\tau=t-s$ and
$$
p(\tau, x, y)=\frac{1}{\sigma y \sqrt{2 \pi \tau}} \exp \left\{-\frac{\left(\log \frac{y}{x}-\nu \tau\right)^2}{2 \sigma^2 \tau}\right\} .
$$

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Problem 7

Exercise 3.7. Theorem 3.6.2 provides the Laplace transform of the density of the first passage time for Brownian motion. This problem derives the analogous formula for Brownian motions with drift. Let $W$ be a Brownian motion. Fix $m>0$ and $\mu \in \mathbb{R}$. For $0 \leq t<\infty$, define
$$
\begin{aligned}
X(t) & =\mu t+W(t), \\
\tau_m & =\min \{t \geq 0 ; X(t)=m\} .
\end{aligned}
$$

As usual, we set $\tau_m=\infty$ if $X(t)$ never reaches the level $m$. Let $\sigma$ be a positive number and set
$$
Z(t)=\exp \left\{\sigma X(t)-\left(\sigma \mu+\frac{1}{2} \sigma^2\right) t\right\} .
$$
(i) Show that $Z(t), t \geq 0$, is a martingale.
(ii) Use (i) to conclude that
$$
\mathbb{E}\left[\exp \left\{\sigma X\left(t \wedge \tau_m\right)-\left(\sigma \mu+\frac{1}{2} \sigma^2\right)\left(t \wedge \tau_m\right)\right\}\right]=1, \quad t \geq 0 .
$$
120
3 Brownian Motion
(iii) Now suppose $\mu \geq 0$. Show that, for $\sigma>0$,
$$
\mathbf{E}\left[\exp \left\{\sigma m-\left(\sigma \mu+\frac{1}{2} \sigma^2\right) \tau_m\right\} \mathbf{I}_{\left\{\tau_m<\infty\right\}}\right]=1 .
$$

Use this fact to show $\mathbb{P}\left\{\tau_m<\infty\right\}=1$ and to obtain the Laplace transform
$$
\mathbb{E} e^{-\alpha \tau_m}=e^{m \mu-m \sqrt{2 \alpha+\mu^2}} \text { for all } \alpha>0 .
$$
(iv) Show that if $\mu>0$, then $\mathbb{E} \tau_m<\infty$. Obtain a formula for $\mathbb{E} \tau_m$. (Hint: Differentiate the formula in (iii) with respect to $\alpha$.)
(v) Now suppose $\mu<0$. Show that, for $\sigma>-2 \mu$,
$$
\mathbb{E}\left[\exp \left\{\sigma m-\left(\sigma \mu+\frac{1}{2} \sigma^2\right) \tau_m\right\} \mathbb{I}_{\left\{\tau_m<\infty\right\}}\right]=1 .
$$

Use this fact to show that $\mathbb{P}\left\{\tau_m<\infty\right\}=e^{-2 x|\mu|}$, which is strictly less than one, and to obtain the Laplace transform
$$
\mathbf{E} e^{-\alpha \tau_m}=e^{m \mu-m \sqrt{2 \alpha+\mu^2}} \text { for all } \alpha>0 \text {. }
$$

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Problem 8

Exercise 3.8. Inis problem presents the convergence or the distribution of stock prices in a sequence of binomial models to the distribution of geometric Brownian motion. In contrast to the analysis of Subsection 3.2.7, here we allow the interest rate to be different from zero.

Let $\sigma>0$ and $r \geq 0$ be given. For each positive integer $n$, we consider a binomial model taking $n$ steps per unit time. In this model, the interest rate per period is $\frac{r}{n}$, the up factor is $u_n=e^{\sigma / \sqrt{n}}$, and the down factor is $d_n=e^{-\sigma / \sqrt{n}}$. The risk-neutral probabilities are then
$$
\tilde{p}_n=\frac{\frac{r}{n}+1-e^{-\sigma / \sqrt{n}}}{e^{\sigma / \sqrt{n}}-e^{-\sigma / \sqrt{n}}}, \quad \tilde{q}_n=\frac{e^{\sigma / \sqrt{n}}-\frac{r}{n}-1}{e^{\sigma / \sqrt{n}}-e^{-\sigma / \sqrt{n}}} .
$$

Let $t$ be an arbitrary positive rational number, and for each positive integer $n$ for which $n t$ is an integer, define
$$
M_{n t, n}=\sum_{k=1}^{n t} X_{k, n}
$$
where $X_{1, n}, \ldots, X_{n, n}$ are independent, identically distributed random variables with
$$
\widetilde{\mathbb{P}}\left\{X_{k, n}=1\right\}=\tilde{p}_n, \quad \widetilde{\mathbb{P}}\left\{X_{k, n}=-1\right\}=\tilde{q}_n, k=1, \ldots, n .
$$

The stock price at time $t$ in this binomial model, which is the result of $n t$ steps from the initial time, is given by (see (3.2.15) for a similar equation)
3.10 Exercises
121
$$
\begin{aligned}
S_n(t) & =S(0) u_n^{\frac{1}{2}\left(n t+M_{n t, n}\right)} d_n^{\frac{1}{2}\left(n t-M_{n t, n}\right)} \\
& =S(0) \exp \left\{\frac{\sigma}{2 \sqrt{n}}\left(n t+M_{n T, n}\right)\right\} \exp \left\{-\frac{\sigma}{2 \sqrt{n}}\left(n t-M_{n t, n}\right)\right\} \\
& =S(0) \exp \left\{\frac{\sigma}{\sqrt{n}} M_{n t, n}\right\} .
\end{aligned}
$$

This problem shows that as $n \rightarrow \infty$, the distribution of the sequence of random variables $\frac{\sigma}{\sqrt{n}} M_{n t, n}$ appearing in the exponent above converges to the normal distribution with mean $\left(r-\frac{1}{2} \sigma^2\right) t$ and variance $\sigma^2 t$. Therefore, the limiting distribution of $S_n(t)$ is the same as the distribution of the geometric Brownian motion $S(0) \exp \left\{\sigma W(t)+\left(r-\frac{1}{2} \sigma\right) t\right\}$ at time $t$.
(i) Show that the moment-generating function $\varphi_n(u)$ of $\frac{1}{\sqrt{n}} M_{n t, n}$ is given by
$$
\varphi_n(u)=\left[e^{\frac{u}{\sqrt{n}}}\left(\frac{\frac{r}{n}+1-e^{-\sigma / \sqrt{n}}}{e^{\sigma / \sqrt{n}}-e^{-\sigma / \sqrt{n}}}\right)-e^{-\frac{u}{\sqrt{n}}}\left(\frac{\frac{r}{n}+1-e^{\sigma / \sqrt{n}}}{e^{\sigma / \sqrt{n}}-e^{-\sigma / \sqrt{n}}}\right)\right]^{n t} .
$$
(ii) We want to compute
$$
\lim _{n \rightarrow \infty} \varphi_n(u)=\lim _{x \downarrow 0} \varphi_{\frac{1}{x^2}}(u),
$$
where we have made the change of variable $x=\frac{1}{\sqrt{n}}$. To do this, we will compute $\log \varphi_{\frac{1}{x^2}}(u)$ and then take the limit as $x \downarrow 0$. Show that

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07:47

Problem 9

(Laplace transform of first passage density). The solution to this problem is long and technical. It is included for the sake of completeness, but the reader may safely skip it.
Let $m>0$ be given, and define
$$
f(t, m)=\frac{m}{t \sqrt{2 \pi t}} \exp \left\{-\frac{m^2}{2 t}\right\} .
$$

According to (3.7.3) in Theorem 3.7.1, $f(t, m)$ is the density in the variable $t$ of the first passage time $\tau_m=\min \{t \geq 0 ; W(t)=m\}$, where $W$ is a Brownian motion without drift. Let
$$
g(\alpha, m)=\int_0^{\infty} e^{-\alpha t} f(t, m) d t, \quad \alpha>0,
$$
be the Laplace transform of the density $f(t, m)$. This problem verifies that $g(\alpha, m)=e^{-m \sqrt{2 \alpha}}$, which is the formula derived in Theorem 3.6.2.
(i) For $k \geq 1$, define
$$
a_k(m)=\frac{1}{\sqrt{2 \pi}} \int_0^{\infty} t^{-k / 2} \exp \left\{-\alpha t-\frac{m^2}{2 t}\right\} d t,
$$
so $g(\alpha, m)=m a_3(m)$. Show that
$$
\begin{aligned}
g_m(\alpha, m) & =a_3(m)-m^2 a_5(m), \\
g_{m m}(\alpha, m) & =-3 m a_5(m)+m^3 a_7(m) .
\end{aligned}
$$
(ii) Use integration by parts to show that
$$
a_5(m)=-\frac{2 \alpha}{3} a_3(m)+\frac{m^2}{3} a_7(m) .
$$
(iii) Use (i) and (ii) to show that $g$ satisfies the second-order ordinary differential equation
$$
g_{m m}(\alpha, m)=2 \alpha g(\alpha, m) .
$$
(iv) The general solution to a second-order ordinary differential equation of the form
$$
a y^{\prime \prime}(m)+b y^{\prime}(m)+c y(m)=0
$$
is
$$
y(m)=A_1 e^{\lambda_1 m}+A_2 e^{\lambda_2 m},
$$
where $\lambda_1$ and $\lambda_2$ are roots of the characteristic equation

Sam Low
Sam Low
Numerade Educator