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Course 6Book 6D: Diffusions, Finance and ComputationChapter 1
Brownian Motion
Construction, scaling, quadratic variation, the Markov property, the reflection principle and harmonic measure.
Read with Taylor II, chapter 11, §11.1 (the Wiener measure), §11.3–11.5 (path properties, the Markov property and exit times); Øksendal, Stochastic Differential Equations, chapter 2; and Jost, Partial Differential Equations, section 8.3 (Brownian motion and the heat semigroup). Mörters and Peres, Brownian Motion (Cambridge, 2010), is the modern reference, and its chapter 1 contains the Lévy construction used here. This chapter proves the Lévy–Ciesielski construction, the quadratic variation theorem, the reflection principle (from the strong Markov property, stated), Kakutani's solution of the Dirichlet problem (harmonicity), and the recurrence and transience criteria.
Book 6A met Brownian motion as the random path whose position at time is distributed by the heat kernel (6A.3 The Heat Equation on ℝⁿ). This book takes the random path seriously. A Brownian path is continuous but nowhere differentiable; it has finite quadratic variation, , which is the fact that makes stochastic calculus different from ordinary calculus; and averaging functions over Brownian paths solves the heat equation, the Laplace equation and, with Feynman and Kac, every linear parabolic equation with a potential. Those averages are also prices: the value of a financial contract is an expectation over random paths, and the equations of mathematical finance are heat equations in disguise (6D.6 Black–Scholes).
We construct Brownian motion from a sequence of independent Gaussians, prove its basic path properties, and use it to solve the Dirichlet problem. The probability needed is modest: Gaussian random variables, independence, expectation as a Lebesgue integral on a probability space (3A.4 Measures, Probability and Weights), and the Borel–Cantelli lemma. Where a proof needs heavier machinery (the strong Markov property, the existence of continuous versions in general), we state it.
A convention. Probabilists normalise Brownian motion so that has variance ; its generator is , and solves . The heat equation of Books 6A–6C corresponds to (6A.3 The Heat Equation on ℝⁿ). We use the probabilists' convention throughout Book 6D.
By the end of this chapter you will be able to:
- explain the random walk scaling and define Brownian motion as a Gaussian process with covariance ;
- construct Brownian motion on from Haar and Schauder functions, and prove that the series converges uniformly almost surely;
- prove that quadratic variation converges to in , and deduce that paths have infinite length;
- use the reflection principle to find the law of the running maximum and of hitting times;
- prove that is harmonic, compute exit probabilities, and decide recurrence and transience by dimension.
Speculation before physics
Five years before Einstein's paper on Brownian motion, Louis Bachelier defended a doctoral thesis in Paris, Théorie de la spéculation (1900), under Henri Poincaré. Bachelier modelled the price of French government bonds traded on the Paris Bourse as a random process whose increments over disjoint time intervals are independent, with variance proportional to elapsed time: a Brownian motion (with drift zero, in his model). He derived the heat equation for the probability density of the price, computed the law of the maximum by an argument equivalent to the reflection principle of this chapter, priced options, and compared his formulas with market data.
The thesis was received politely and then largely forgotten, until Paul Samuelson and others rediscovered it in the 1950s. Two corrections were needed before it became modern finance: prices cannot go negative, so the model is applied to the logarithm of a price (geometric Brownian motion, 6D.3 Stochastic Differential Equations and Feynman–Kac); and the price of an option must not depend on investors' attitudes to risk, which led to the replication argument of Black, Scholes and Merton in 1973 (6D.6 Black–Scholes). But the core mathematical object, a continuous random path with independent Gaussian increments, is Bachelier's, and it is the object of this chapter.
Random walks and the definition
Toss a fair coin every seconds and step . After time the position is , with a sum of independent steps. Then and , and by the central limit theorem converges in distribution to . The step size , the square root of the time step, is forced: smaller steps give a limit that does not move, larger ones a limit that explodes. This diffusive scaling, space like the square root of time, is the scaling of the heat equation. Increments over disjoint time intervals use disjoint sets of coin tosses, so they are independent. Monroe Donsker proved in 1951 that the whole random path converges in distribution, as a random continuous function, to the following object.
A (standard, one-dimensional) Brownian motion is a family of random variables on a probability space such that
- ;
- for , the increments are independent;
- for ;
- for every , the path is continuous.
A Brownian motion in is with independent one-dimensional Brownian motions as components. Brownian motion started at is , and we write , for its probabilities and expectations.
Properties 1–3 say exactly that is a Gaussian process (every finite collection is jointly Gaussian) with mean zero and covariance
(Exercise 1.8). Property 4 is the real content: it is not implied by 1–3 (one can modify each on a null set depending on and destroy continuity) and needs a construction.
The Lévy–Ciesielski construction
On use the Haar functions: , and for and ,
They form an orthonormal basis of (orthonormality is a direct check; completeness holds because their span contains the indicator of every dyadic interval, and these span a dense subspace; 4A.5 Hilbert Spaces and Lax–Milgram). Their integrals are the Schauder functions
tents supported on with height ; for fixed the tents have disjoint supports.
Let and (, ) be independent random variables. Then almost surely the series
converges uniformly on , and its sum is a Brownian motion on .
Proof. A Gaussian tail bound. For and , .
Uniform convergence. Let . By the union bound and the tail estimate with (), , which is summable. By the Borel–Cantelli lemma, almost surely for all beyond some . Since the tents at level have disjoint supports and height ,
which is summable in . So the series converges uniformly, almost surely, and its sum is continuous (a uniform limit of continuous functions, 2B.5 Uniform Convergence and Arzelà–Ascoli). On the null set where it fails, set .
The covariance. For fixed , the partial sums are Gaussian, and they converge in as well (the terms are orthogonal in with summable variances, as the next display shows), so is jointly Gaussian with mean zero, and by independence of the 's
because . By Parseval's identity for the orthonormal basis , this is . The same argument applies to any finite collection , which is therefore a mean-zero Gaussian vector with covariance . By Exercise 1.8, properties 1–3 hold, and 4 was proved above.
To get Brownian motion on , take independent copies on and glue them: for . The construction is also an algorithm: the level- terms refine the path at the dyadic points of spacing by adding independent Gaussian bumps at the midpoints, which is how Brownian paths are drawn on a computer (the "Brownian bridge" or midpoint displacement method).
Invariances. Each of the following is again a Brownian motion (Exercise 1.9): ; for fixed (and it is independent of , the Markov property); the rescaled path for (Brownian scaling); and the time-inverted path (extended by at ). Scaling says Brownian motion looks the same at every scale, statistically: zooming in by a factor in time and in space gives the same picture. It is a random fractal.
Quadratic variation
For a partition of with mesh , the quadratic variation of the path along is .
. So in as , and almost surely along any sequence of partitions with .
Proof. Write , independent with . Then , a sum of independent mean-zero terms, so its variance is the sum of the variances: (the fourth moment of is ). And . For almost sure convergence, Chebyshev's inequality gives , summable, and Borel–Cantelli applies.
For a function , . Brownian paths are therefore nothing like functions: increments over a time are of size , not , and their squares add up to something finite and deterministic. In shorthand, , which is the rule behind Itô's formula (6D.2 Martingales and the Itô Integral).
Almost surely, the path has infinite total variation on every interval with .
Proof. Take dyadic partitions of (rational suffice, then every interval contains one), along which almost surely. If the total variation were finite, then , because by uniform continuity of the path. Contradiction.
In particular Brownian paths are not differentiable on any interval (a function differentiable everywhere on an interval with bounded derivative has finite variation). Much more is true: Raymond Paley, Norbert Wiener and Antoni Zygmund proved in 1933 that almost every Brownian path is differentiable at no point (statement). Infinite variation is also why the integral cannot be defined path by path as a Riemann–Stieltjes integral, and why Itô had to define it as an limit.
The reflection principle
For let , the first time the path reaches , and the running maximum. Then .
The tool is the strong Markov property (statement): if is a stopping time (whether is decided by the path up to time ; 6D.2 Martingales and the Itô Integral) with almost surely, then is a Brownian motion independent of the path up to time . For deterministic this is the Markov property; for hitting times it is a theorem (Øksendal, section 7.2; Mörters and Peres, section 2.1).
For and ,
Proof. Since ,
with (because by continuity). By the strong Markov property is a Brownian motion independent of , and so is . Hence, conditionally on , is , positive or negative with probability each (and zero with probability ). So
Thus . The last equality is the symmetry of .
The name describes the proof: every path that reaches before time and ends below corresponds, by reflecting its part after in the line , to a path that ends above , and reflection preserves probabilities. Bachelier used this argument in 1900. Consequences (Exercise 1.10): is finite almost surely (Brownian motion reaches every level), but ; and has density .
A down-and-out barrier option becomes worthless if the underlying price ever falls to a barrier. In a model where the log-price is (no drift), the probability that it stays above the barrier up to time is
with the standard normal distribution function. With per square-root year, year and a barrier below in log terms (), this is : about one chance in three of being knocked out. Pricing barrier options in the Black–Scholes model uses the same reflection, combined with a change of measure that removes the drift (6D.6 Black–Scholes).
Harmonic measure and the Dirichlet problem
Let be a bounded domain and the exit time, finite almost surely (Exercise 1.11). For a continuous function on , define
the expected value of at the point where Brownian motion started at first leaves . The law of under is the harmonic measure of seen from .
The function is harmonic in . At every boundary point that is regular for the Dirichlet problem (in the sense of 6B.6 Perron’s Method and Barriers), as . In particular, if every boundary point is regular (for example, if satisfies an exterior cone condition), is the solution of the Dirichlet problem in , on .
Proof. We prove harmonicity; the boundary behaviour is in Mörters and Peres, section 3.1. Fix and a ball , and let be the exit time from , so . By the strong Markov property at , after time the path is a Brownian motion started at , independent of the past, and it exits at the same place as the original path (it has not left yet). So
Brownian motion started at is invariant in law under rotations about (its density is radial), so the exit point is uniformly distributed on the sphere . Hence
for every small : has the mean value property. It is also bounded and measurable, and continuous (by the same identity, averaged over , it is a convolution with a smooth bump, as in the proof of Weyl's lemma in 6A.2 Harmonic Functions). A continuous function with the mean value property is harmonic (6A.2 Harmonic Functions).
So harmonic measure is the answer to the question "where does a random walker leave the room?", and the Dirichlet problem is a gambling problem: if you receive when the walk exits at , the fair price of the game started at is . Shizuo Kakutani found this connection in 1944. In one dimension, harmonic functions are linear, and the exit problem from is gambler's ruin: (Exercise 1.12).
Recurrence and transience
Apply the same idea to the annulus in and the event that the walk reaches the inner sphere before the outer one. The probability is harmonic in , equal to on and on , and the boundary is smooth, so is the radial harmonic function with these values (6A.2 Harmonic Functions):
Now let (the walk reaches the outer sphere in finite time almost surely, and makes this ever later). In two dimensions : Brownian motion in the plane comes back arbitrarily close to every point, infinitely often (neighbourhood recurrence). In three or more dimensions : with positive probability the walk never comes back to the ball, and in fact almost surely (transience). George Pólya had proved the same dichotomy for random walks on the integer lattice in 1921. The dividing line is the dimension at which the Newtonian potential stops being a logarithm: recurrence is a statement about the fundamental solution of the Laplacian.
The quadratic variation theorem is the foundation of Itô calculus (6D.2 Martingales and the Itô Integral), and Kakutani's theorem becomes the Feynman–Kac formula for parabolic equations with potentials (6D.3 Stochastic Differential Equations and Feynman–Kac). On a Riemannian manifold, Brownian motion is the diffusion whose generator is times the Laplace–Beltrami operator, and its transition density is the heat kernel of 9B.7 The Heat Equation on a Manifold; S. R. S. Varadhan proved in 1967 that as , so short-time Brownian motion "knows" the Riemannian distance (Exercise 1.15). Perelman's reduced distance (12A.5 Reduced Distance and Reduced Volume) is the analogue for the backward heat equation along a Ricci flow, and the reduced volume is, heuristically, the volume of space as seen by Brownian motion in space-time.
History
Robert Brown observed the motion of pollen particles in 1827. Louis Bachelier (1900), Albert Einstein (1905) and Marian Smoluchowski (1906) gave the first theories, and Jean Perrin's experiments (1908–09) confirmed Einstein's (6A.3 The Heat Equation on ℝⁿ). Norbert Wiener constructed Brownian motion as a measure on continuous paths in 1923, which is why it is also called the Wiener process. Paul Lévy developed the theory of its paths in the 1930s and 1940s, including the midpoint construction, and Zbigniew Ciesielski gave the Haar-function form in 1961. Paley, Wiener and Zygmund proved nowhere differentiability in 1933, Kakutani connected Brownian motion to the Dirichlet problem in 1944, and Donsker proved the invariance principle in 1951.
Brownian motion is the continuous Gaussian process with , independent increments and ; equivalently, covariance with continuous paths. It is the scaling limit of random walks and is built explicitly as with Schauder functions, converging uniformly almost surely. It is invariant under sign change, restarting, scaling and time inversion. Quadratic variation , so paths have infinite length and are nowhere differentiable: . By reflection, . Exit distributions solve the Dirichlet problem ( is harmonic), and comparison with radial harmonic functions shows Brownian motion is recurrent in dimensions and and transient in dimensions and higher. 6D.2 Martingales and the Itô Integral builds the calculus of Brownian motion: martingales, the Itô integral and Itô's formula.
Exercises
Let be a mean-zero Gaussian process with . Show that , that for , and that increments over disjoint intervals are independent. (Jointly Gaussian variables are independent iff they are uncorrelated.)
Solution
, so almost surely. . For , . All increments are jointly Gaussian (linear combinations of a Gaussian vector), so pairwise uncorrelated increments are independent; the same computation applies to any finite family.
Using Exercise 1.8, show that and are Brownian motions, and that (with ) has the right covariance. (Continuity of at follows from the strong law of large numbers, ; you may assume it.)
Solution
All three are mean-zero Gaussian processes with continuous paths (for ). . . .
(a) From , show that has density and that almost surely. (b) Show . (c) With , compute .
Solution
(a) . As , . (b) as , not integrable. (c) .
Let . Show that for some independent of , using the fact that from any point of , the first coordinate of Brownian motion moves by more than in one unit of time with probability , and the Markov property at integer times. Conclude that almost surely and .
Solution
Let . If , the path cannot have stayed in during . These increments are independent, so . Then and .
(a) For one-dimensional Brownian motion started at , show that . (b) A gambler's capital moves like Brownian motion; starting with , they stop on reaching or . What is the probability of reaching ? (c) In Exercise 1.13 you will see that . What is the expected duration here?
Solution
(a) is harmonic on , i.e. linear, with , (all boundary points are regular in one dimension). (b) . (c) units of time.
Brownian motion has generator , and in 6D.3 Stochastic Differential Equations and Feynman–Kac we will prove that solves in , on . (a) Verify that solves this on the ball . (b) In one dimension on , find the solution and check it against Exercise 1.12. (c) How long does Brownian motion started at the centre of the unit ball in take to leave it, on average?
Solution
(a) , so , and on . (b) with gives . (c) .
For Brownian motion in started at distance from the origin, what is the probability that it ever enters the unit ball? In , started at distance , what is the probability of reaching the unit disc before the circle of radius ?
Solution
In , . In , .
The transition density of Brownian motion in is . (a) Show that as . (b) The heat kernel of is ; show that it is , and that its exponent is Perelman's reduced distance in flat space, (6C.9 Hamilton–Jacobi Equations and Viscosity Solutions, 12A.5 Reduced Distance and Reduced Volume). On a Riemannian manifold, Varadhan's theorem says : the heat kernel encodes the distance, which is why Perelman could define a distance-like quantity () whose exponential behaves like a heat kernel.
Solution
(a) , since . (b) , with exponent .
Free resources for this chapter
Chosen for what this chapter covers, and all free to read. Links checked Oct 20, 2026.
- Reference Wiener processWikipediaConstruction and path properties of Brownian motion.
- Reference Reflection principle (Wiener process)WikipediaThe law of the running maximum.
- Reference Louis BachelierWikipediaBachelier's 1900 theory of speculation.
- Notes Lecture 5: Stochastic Processes IMIT OpenCourseWare 18.S096 Topics in Mathematics with Applications in Finance (Fall 2013)Random walks, Markov chains and martingales in discrete time.
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