Introduction to Brownian Motion

Watch a grain of pollen jitter in water under a microscope. Or track the cumulative winnings of a gambler flipping a fair coin every millisecond. Zoom out far enough — rescale time and space correctly — and both pictures converge to the same object. That object is a random, continuous, nowhere-smooth path. This convergence is not a vague analogy. It is a precise limit theorem, and the limiting object is Brownian motion. It is the central continuous-time process of probability theory. Understanding it means understanding two things at once. It is both the endpoint of the Random Walks story. And it is the starting point of stochastic calculus, diffusion theory, and mathematical finance. Brownian motion matters because it is the unique reasonable candidate for a continuous-path process. It has independent, stationary increments. By a scaling argument tied to the Normal distribution, these increments are necessarily Gaussian. It sits at a crossroads of several fields. These include physics (Einstein's 1905 explanation of molecular motion). They include pure mathematics (Wiener's 1923 construction, the first rigorous existence proof for a stochastic process on path space). They also include applications from option pricing to noise models in engineering. It also raises a genuine mathematical subtlety that a naive picture obscures. The limiting paths, while continuous, are almost surely nowhere differentiable. So "Brownian velocity" does not exist in the classical sense. The big picture is a scaling limit. Take a symmetric random walk with step size Δx\Delta x taken every Δt\Delta t seconds. As Δt→0\Delta t \to 0, only one relationship between Δx\Delta x and Δt\Delta t produces a nondegenerate limit. That relationship is Δx∝Δt\Delta x \propto \sqrt{\Delta t}. This time\sqrt{\text{time}} scaling is the same scaling that governs the Poisson process's Gaussian approximation via the Central Limit Theorem. It is the fingerprint of diffusive behavior. It distinguishes diffusion sharply from ballistic (Δx∝Δt\Delta x \propto \Delta t) motion. This article builds Brownian motion from the random walk up. We state the precise definition. We prove Donsker-type convergence intuition via the Central Limit Theorem. We establish the defining theorem (existence, Gaussian finite-dimensional distributions, path continuity). We examine the delicate nondifferentiability phenomenon. Two full worked examples round out the treatment. So does a counterexample showing why independence of increments is essential. Finally, we discuss where Brownian motion appears across mathematics and science.

Key takeaways
  • Brownian motion BtB_t is the scaling limit of a symmetric random walk when step size scales as Δt\sqrt{\Delta t}.
  • It has independent, stationary increments distributed as Bt−Bs∼N(0,t−s)B_t - B_s \sim N(0, t-s).
  • Paths are almost surely continuous but almost surely nowhere differentiable — smooth-looking, infinitely jagged.
  • The finite-dimensional distributions are jointly Gaussian with covariance Cov(Bs,Bt)=min⁡(s,t)\mathrm{Cov}(B_s,B_t) = \min(s,t).
  • Wiener's theorem guarantees a version of the process with continuous sample paths exists on a suitable probability space.
  • Key idea: rescaling a random walk by n\sqrt{n} in space and nn in time forces, via the Central Limit Theorem, a Gaussian continuous-path limit — this is Brownian motion.

Where this lives today

Brownian motion is the basic building block of stochastic calculus (Itô integrals, stochastic differential equations), which underlies modern mathematical finance: the Black–Scholes option pricing model treats log-stock-prices as drifted, scaled Brownian motion. In physics, it remains the canonical model of diffusion — heat conduction, particle transport, and the Fokker–Planck equation are its PDE counterparts. In statistics, Brownian motion (and its bridge and sheet variants) arises as the limiting process in the theory of empirical processes, underlying Kolmogorov–Smirnov goodness-of-fit tests. In engineering, white noise is formally the (distributional) derivative of Brownian motion, central to signal processing and Kalman filtering. In pure mathematics, Brownian motion connects to potential theory (harmonic functions and hitting probabilities), fractal geometry (its graph has Hausdorff dimension 3/23/2), and representation theory of Gaussian processes; it is also the prototypical example motivating the general theory of Markov processes and martingales built on the foundations of Random Walks.

Ask the tutor: How does adding drift and volatility parameters turn standard Brownian motion into the geometric Brownian motion used to model stock prices?

DefinitionStandard Brownian Motion

A stochastic process (Bt)t≥0(B_t)_{t \ge 0} defined on a probability space (Ω,F,P)(\Omega, \mathcal{F}, \mathbb{P}) is a standard (one-dimensional) Brownian motion (or Wiener process) if: 1. Initial condition: B0=0B_0 = 0 almost surely. 2. Independent increments: for all 0≤t0<t1<⋯<tn0 \le t_0 < t_1 < \cdots < t_n, the random variables

Bt1−Bt0, Bt2−Bt1, …, Btn−Btn−1B_{t_1} - B_{t_0},\ B_{t_2} - B_{t_1},\ \dots,\ B_{t_n} - B_{t_{n-1}}

are mutually independent. 3. Gaussian stationary increments: for all 0≤s<t0 \le s < t,

Bt−Bs∼N(0,t−s).B_t - B_s \sim N(0, t - s).

4. Continuous paths: for almost every ω∈Ω\omega \in \Omega, the map t↦Bt(ω)t \mapsto B_t(\omega) is a continuous function of tt. A process satisfying (1)–(3) but not necessarily (4) is called a version of Brownian motion; property (4) singles out the continuous version, which is the object of interest and which we will show exists.

Intuition

Picture a random walk Sn=X1+X2+⋯+XnS_n = X_1 + X_2 + \cdots + X_n where each Xi=±1X_i = \pm 1 with probability 1/21/2, independently. This is the discrete skeleton. To get a continuous-time, continuous-space limit, imagine speeding up the clock: take nn steps per unit time, and shrink each step so the total variance stays finite. Concretely, define for t≥0t \ge 0

Wn(t)=1nS⌊nt⌋.W_n(t) = \frac{1}{\sqrt{n}} S_{\lfloor nt \rfloor}.

At integer multiples of 1/n1/n, Var(Wn(t))=⌊nt⌋n→t\mathrm{Var}(W_n(t)) = \frac{\lfloor nt \rfloor}{n} \to t. The Central Limit Theorem tells us that S⌊nt⌋/nS_{\lfloor nt\rfloor}/\sqrt{n} converges in distribution to N(0,t)N(0,t): this is exactly the scaling Δx∼Δt\Delta x \sim \sqrt{\Delta t} mentioned above. Independence of the walk's increments is inherited by WnW_n's increments over disjoint time blocks, and this independence survives in the limit. What is not obvious — and is the deep content of Donsker's theorem, which we approach here at the level of finite-dimensional convergence — is that the entire path, not just single-time marginals, converges, and that the limit has continuous paths. The picture to hold in mind: at any fixed resolution the path looks like a smooth wiggly curve, but zoom into any interval and the same jaggedness reappears at every scale — a fractal-like self-similarity coming from the identity Bctc BtB_{ct} \stackrel{d}{=} \sqrt{c}\, B_t for c>0c>0. This self-similarity is why no derivative exists: the local increment over [t,t+h][t, t+h] has typical size h\sqrt{h}, so the difference quotient (Bt+h−Bt)/h\big(B_{t+h}-B_t\big)/h has typical size 1/h→∞1/\sqrt{h} \to \infty.

Figure
Random walk paths rescaled by n\sqrt{n} converge toward a continuous Brownian path
t x coarse walk, n = 8 steps finer skeleton, n = 64: approaching B(t) as n → ∞: step ~ ±1/√n every 1/n time units
TheoremExistence and Characterization of Brownian Motion (Wiener)

Let (Xi)i≥1(X_i)_{i \ge 1} be i.i.d. random variables with E[Xi]=0\mathbb{E}[X_i] = 0 and Var(Xi)=1\mathrm{Var}(X_i) = 1, and let S0=0S_0 = 0, Sn=X1+⋯+XnS_n = X_1 + \cdots + X_n. Define the rescaled process

Wn(t)=S⌊nt⌋n,t≥0.W_n(t) = \frac{S_{\lfloor nt \rfloor}}{\sqrt n}, \qquad t \ge 0.

Then:

(a) Finite-dimensional convergence. For every finite set of times 0=t0<t1<⋯<tk0 = t_0 < t_1 < \cdots < t_k, the vector

(Wn(t1),…,Wn(tk))\big(W_n(t_1), \dots, W_n(t_k)\big)

converges in distribution, as n→∞n \to \infty, to a Gaussian vector (Bt1,…,Btk)(B_{t_1}, \dots, B_{t_k}) with independent increments Btj−Btj−1∼N(0,tj−tj−1)B_{t_j}-B_{t_{j-1}} \sim N(0, t_j - t_{j-1}), mutually independent across jj.

(b) Existence of a continuous version. There exists a probability space and a stochastic process (Bt)t≥0(B_t)_{t\ge0} on it satisfying properties (1)–(4) of the definition of Brownian motion above, whose finite-dimensional distributions are exactly the Gaussian law obtained in (a). In particular such a process exists, is essentially unique in law, and can be chosen with continuous sample paths.

(c) Covariance structure. For this process, E[Bt]=0\mathbb{E}[B_t]=0 for all tt and

Cov(Bs,Bt)=min⁡(s,t),s,t≥0.\mathrm{Cov}(B_s, B_t) = \min(s,t), \qquad s,t \ge 0.
Proof

We prove (a) using the Central Limit Theorem and the Cramér–Wold device; (b) is addressed via Kolmogorov's continuity criterion together with the Normal distribution moment structure (a full measure-theoretic construction of Wiener measure via consistency/Kolmogorov extension is sketched, citing standard existence for the countable-dimensional distributions); (c) is a direct computation.

Part (a): finite-dimensional convergence. Fix times 0=t0<t1<⋯<tk0 = t_0 < t_1 < \cdots < t_k. Write the increments of the rescaled walk as

Δj(n):=Wn(tj)−Wn(tj−1)=S⌊ntj⌋−S⌊ntj−1⌋n,j=1,…,k.\Delta_j^{(n)} := W_n(t_j) - W_n(t_{j-1}) = \frac{S_{\lfloor nt_j\rfloor} - S_{\lfloor n t_{j-1}\rfloor}}{\sqrt n}, \qquad j=1,\dots,k.

Because SmS_m is a sum of i.i.d. increments XiX_i, and ⌊ntj−1⌋<⌊ntj⌋\lfloor nt_{j-1}\rfloor < \lfloor nt_j \rfloor (eventually, since tj−1<tjt_{j-1}<t_j), the blocks

X⌊ntj−1⌋+1+⋯+X⌊ntj⌋X_{\lfloor nt_{j-1}\rfloor+1} + \cdots + X_{\lfloor n t_j\rfloor}

for j=1,…,kj = 1,\dots,k are sums over disjoint index ranges of i.i.d. variables, hence Δ1(n),…,Δk(n)\Delta_1^{(n)}, \dots, \Delta_k^{(n)} are independent random variables for each nn. Let mj(n)=⌊ntj⌋−⌊ntj−1⌋m_j^{(n)} = \lfloor n t_j\rfloor - \lfloor n t_{j-1}\rfloor, the number of summands in block jj. Since ⌊ntj⌋/n→tj\lfloor nt_j\rfloor/n \to t_j and ⌊ntj−1⌋/n→tj−1\lfloor nt_{j-1}\rfloor/n \to t_{j-1}, we get mj(n)/n→tj−tj−1=:δj>0m_j^{(n)}/n \to t_j - t_{j-1} =: \delta_j > 0. Each Δj(n)\Delta_j^{(n)} is 1n\frac{1}{\sqrt n} times a sum of mj(n)m_j^{(n)} i.i.d. mean-zero, unit-variance variables. Rewrite

Δj(n)=mj(n)n⋅1mj(n)∑i=1mj(n)X⌊ntj−1⌋+i.\Delta_j^{(n)} = \sqrt{\frac{m_j^{(n)}}{n}} \cdot \frac{1}{\sqrt{m_j^{(n)}}}\sum_{i=1}^{m_j^{(n)}} X_{\lfloor nt_{j-1}\rfloor + i}.

By the classical Central Limit Theorem (finite variance suffices; Lindeberg–Lévy form), the inner normalized sum converges in distribution to N(0,1)N(0,1) as mj(n)→∞m_j^{(n)} \to \infty. Since mj(n)/n→δj\sqrt{m_j^{(n)}/n} \to \sqrt{\delta_j}, Slutsky's theorem gives

Δj(n)→dN(0,δj)as n→∞,\Delta_j^{(n)} \xrightarrow{d} N(0, \delta_j) \quad \text{as } n \to \infty,

for each fixed jj. To upgrade this to joint convergence of the independent vector (Δ1(n),…,Δk(n))(\Delta_1^{(n)},\dots,\Delta_k^{(n)}), note that for independent random variables convergence in distribution of each marginal to a limit implies joint convergence to the product law: for any bounded continuous f1,…,fkf_1,\dots,f_k,

E[∏j=1kfj(Δj(n))]=∏j=1kE[fj(Δj(n))]⟶∏j=1kE[fj(Zj)]\mathbb{E}\Big[\prod_{j=1}^k f_j(\Delta_j^{(n)})\Big] = \prod_{j=1}^k \mathbb{E}[f_j(\Delta_j^{(n)})] \longrightarrow \prod_{j=1}^k \mathbb{E}[f_j(Z_j)]

where Zj∼N(0,δj)Z_j \sim N(0,\delta_j) independent, using independence at each finite nn and marginal convergence in distribution (which implies convergence of E[fj(⋅)]\mathbb{E}[f_j(\cdot)] for bounded continuous fjf_j). This is exactly convergence in distribution of the joint vector to the product measure, i.e. to independent Gaussians Z1,…,ZkZ_1,\dots,Z_k with Zj∼N(0,tj−tj−1)Z_j \sim N(0, t_j - t_{j-1}). Finally, set Btj:=Z1+⋯+ZjB_{t_j} := Z_1 + \cdots + Z_j. The continuous mapping theorem (applied to the linear, hence continuous, map (Δ1,…,Δk)↦(Δ1,Δ1+Δ2,…,Δ1+⋯+Δk)(\Delta_1,\dots,\Delta_k)\mapsto (\Delta_1, \Delta_1+\Delta_2,\dots,\Delta_1+\cdots+\Delta_k)) gives

(Wn(t1),…,Wn(tk))=(∑i≤1Δi(n),…,∑i≤kΔi(n))→d(Bt1,…,Btk),\big(W_n(t_1),\dots,W_n(t_k)\big) = \Big(\sum_{i\le 1}\Delta_i^{(n)}, \dots, \sum_{i \le k}\Delta_i^{(n)}\Big) \xrightarrow{d} (B_{t_1},\dots,B_{t_k}),

and by construction Btj−Btj−1=Zj∼N(0,tj−tj−1)B_{t_j}-B_{t_{j-1}} = Z_j \sim N(0,t_j-t_{j-1}) with these increments mutually independent. This proves (a).

Part (b): existence of a continuous version. The family of finite-dimensional Gaussian laws constructed in part (a), indexed over all finite subsets of [0,∞)[0,\infty), is consistent: the law of (Bt1,…,Btk)(B_{t_1},\dots,B_{t_k}) marginalizes correctly to the law of any sub-collection, since marginals of jointly Gaussian vectors are Gaussian with the matching covariance (a direct check from the explicit covariance formula derived in part (c) below, which depends only on the pair of times, not on which other times are included). By the Kolmogorov extension theorem, there exists a probability space (Ω,F,P)(\Omega,\mathcal F,\mathbb P) and a process (Bt)t≥0(B_t)_{t \ge 0} on it — a priori only defined on the product σ\sigma-algebra of R[0,∞)\mathbb R^{[0,\infty)} — whose finite-dimensional distributions match those constructed in (a). This process automatically satisfies properties (1)–(3) of the definition, since these are statements about finite-dimensional laws. It remains to produce a version with almost-surely continuous paths (property (4)); the process handed to us by the extension theorem lives on a non-separable path space and need not have this regularity built in. We invoke Kolmogorov's continuity criterion: if a process (Xt)t∈[0,T](X_t)_{t\in[0,T]} satisfies, for some constants α,β,C>0\alpha,\beta,C>0 and all s,ts,t,

E[∣Xt−Xs∣α]≤C ∣t−s∣1+β,\mathbb{E}\big[|X_t - X_s|^\alpha\big] \le C\,|t-s|^{1+\beta},

then XX admits a modification with (locally) Hölder-continuous paths of any order less than β/α\beta/\alpha; in particular a continuous modification exists. We check this moment bound for BB using the fourth moment of the normal law: since Bt−Bs∼N(0,t−s)B_t - B_s \sim N(0, t-s) for s<ts<t (from the increment structure in (a)), and a mean-zero Gaussian Z∼N(0,σ2)Z\sim N(0,\sigma^2) has E[Z4]=3σ4\mathbb{E}[Z^4] = 3\sigma^4, we obtain

E[(Bt−Bs)4]=3(t−s)2.\mathbb{E}\big[(B_t-B_s)^4\big] = 3(t-s)^2.

Taking α=4\alpha = 4 and C=3C=3, this is exactly C∣t−s∣1+βC|t-s|^{1+\beta} with β=1\beta = 1. Kolmogorov's criterion then guarantees a modification of BB with sample paths Hölder continuous of every order γ<β/α=1/4\gamma < \beta/\alpha = 1/4, and in particular continuous. Two versions of a process that agree in finite-dimensional distributions and where one is continuous can be identified (up to a null set) as the desired continuous process; we relabel this continuous modification (Bt)t≥0(B_t)_{t\ge 0}. It still satisfies (1)–(3), since modification does not change finite-dimensional distributions, and now also satisfies (4). This establishes existence of standard Brownian motion as defined. (Uniqueness in law is immediate: any two processes satisfying (1)–(3) have, by definition, the same finite-dimensional Gaussian distributions with independent increments; since a Gaussian process is fully determined in law by its mean and covariance function, and both mean 00 and covariance min⁡(s,t)\min(s,t) are forced by (1)–(3) as we now show in (c), the law of the whole process — as a measure on continuous path space via (4) — is uniquely determined.)

Part (c): covariance structure. Since B0=0B_0 = 0 and Bt−B0∼N(0,t)B_t - B_0 \sim N(0,t), we have E[Bt]=0\mathbb{E}[B_t] = 0 for all t≥0t \ge 0. For 0≤s≤t0 \le s \le t, write Bt=Bs+(Bt−Bs)B_t = B_s + (B_t - B_s), where BsB_s and Bt−BsB_t - B_s are independent by the independent-increments property (using the partition 0<s<t0<s<t in property (2)). Then

Cov(Bs,Bt)=Cov(Bs,Bs)+Cov(Bs,Bt−Bs)=Var(Bs)+0=s,\mathrm{Cov}(B_s, B_t) = \mathrm{Cov}(B_s, B_s) + \mathrm{Cov}(B_s, B_t - B_s) = \mathrm{Var}(B_s) + 0 = s,

using independence to kill the cross term and Var(Bs)=s\mathrm{Var}(B_s) = s from property (3) applied with the interval [0,s][0,s]. By symmetry in s,ts,t, for general s,t≥0s,t\ge 0,

Cov(Bs,Bt)=min⁡(s,t).\mathrm{Cov}(B_s,B_t) = \min(s,t).

This completes the proof of (c) and of the theorem. ■\blacksquare

∎
CorollaryNowhere differentiability

Almost surely, the path t↦Btt \mapsto B_t of standard Brownian motion is nowhere differentiable on [0,∞)[0,\infty).

(Stated here as the signature qualitative feature of the process; the full proof is a substantial result of Paley–Wiener–Zygmund type and is beyond the scope of this introductory treatment, but the heuristic is immediate from scaling: since Bt−Bs∼N(0,∣t−s∣)B_t - B_s \sim N(0,|t-s|), we have E[(Bt−Bs)2]=∣t−s∣\mathbb E[(B_t-B_s)^2] = |t-s|, so a typical increment over a tiny interval of length hh has size of order h\sqrt h, not order hh. A genuine derivative at ss would require (Bs+h−Bs)/h→(B_{s+h}-B_s)/h \to some finite limit, but the typical size of this ratio is h/h=1/h→∞\sqrt h / h = 1/\sqrt h \to \infty as h→0h\to 0. This scaling obstruction, made rigorous via a Borel–Cantelli argument over dyadic increments, is what forces nondifferentiability at every point simultaneously.)

Worked examples

Example 1: A joint-probability computation with asymmetric, non-round times. Let (Bt)(B_t) be standard Brownian motion. Compute P(B2>1,B5>4)\mathbb{P}(B_2 > 1, B_5 > 4). Solution. Use the independent increments structure. Write B5=B2+(B5−B2)B_5 = B_2 + (B_5 - B_2), where B2∼N(0,2)B_2 \sim N(0,2) and B5−B2∼N(0,3)B_5 - B_2 \sim N(0,3) are independent (by property (2)–(3) of the definition, using the partition 0<2<50<2<5). Let X=B2X = B_2 and Y=B5−B2Y = B_5 - B_2, so X∼N(0,2)X \sim N(0,2), Y∼N(0,3)Y\sim N(0,3) independent, and we want

P(X>1, X+Y>4).\mathbb{P}(X > 1,\ X + Y > 4).

Condition on X=xX = x: given X=xX=x, the event becomes Y>4−xY > 4-x, and since Y∼N(0,3)Y \sim N(0,3) independent of XX,

P(X>1,X+Y>4)=∫1∞ϕ2(x) P(Y>4−x) dx=∫1∞ϕ2(x)[1−Φ ⁣(4−x3)]dx,\mathbb{P}(X>1, X+Y>4) = \int_1^\infty \phi_2(x)\, \mathbb{P}(Y > 4-x)\, dx = \int_1^\infty \phi_2(x)\left[1-\Phi\!\left(\frac{4-x}{\sqrt3}\right)\right]dx,

where ϕ2\phi_2 is the N(0,2)N(0,2) density and Φ\Phi the standard normal CDF. This integral does not have an elementary closed form, but it can be evaluated numerically or expressed via the bivariate normal CDF, since (X,X+Y)(X,X+Y) is a bivariate Gaussian vector with

Var(X)=2,Var(X+Y)=Var(B5)=5,Cov(X,X+Y)=Cov(B2,B5)=min⁡(2,5)=2,\mathrm{Var}(X) = 2,\quad \mathrm{Var}(X+Y) = \mathrm{Var}(B_5) = 5, \quad \mathrm{Cov}(X,X+Y) = \mathrm{Cov}(B_2,B_5) = \min(2,5) = 2,

matching part (c) of the theorem directly — a useful cross-check. The correlation is

ρ=225=210≈0.6325.\rho = \frac{2}{\sqrt{2}\sqrt{5}} = \frac{2}{\sqrt{10}} \approx 0.6325.

Standardizing, Z1=X/2Z_1 = X/\sqrt2, Z2=(X+Y)/5Z_2 = (X+Y)/\sqrt5 are standard normals with correlation ρ≈0.6325\rho \approx 0.6325, and we want

P(Z1>12, Z2>45)=P(Z1>0.7071, Z2>1.7889).\mathbb{P}\Big(Z_1 > \tfrac{1}{\sqrt2},\ Z_2 > \tfrac{4}{\sqrt5}\Big) = \mathbb{P}(Z_1 > 0.7071,\ Z_2 > 1.7889).

Using the standard bivariate normal survival function L(h,k;ρ)=P(Z1>h,Z2>k)L(h,k;\rho) = \mathbb{P}(Z_1>h, Z_2>k) with h=0.7071h=0.7071, k=1.7889k=1.7889, ρ=0.6325\rho = 0.6325, numerical evaluation (e.g. via the bivariate normal integral tables or software) gives

P(B2>1,B5>4)≈0.0206.\mathbb{P}(B_2>1, B_5>4) \approx 0.0206.

The key structural point — independent of the numeric integration — is that this problem reduces entirely to Gaussian bivariate machinery because Brownian motion's finite-dimensional distributions are jointly Gaussian with the explicit covariance min⁡(s,t)\min(s,t): no path-integral or process-level reasoning beyond that is needed for finite-time-point questions.

Example 2: Verifying the scaling/self-similarity property with concrete numbers. Show that if (Bt)t≥0(B_t)_{t\ge0} is standard Brownian motion and c=4c = 4, then B~t:=12B4t\widetilde B_t := \tfrac{1}{2} B_{4t} is again a standard Brownian motion, and use this to compute P(B12−B4>6)\mathbb{P}(B_{12} - B_4 > 6) two ways: directly, and via the rescaled process. Solution. First, the general scaling claim: for c>0c>0, define B~t=c−1/2Bct\widetilde B_t = c^{-1/2} B_{ct}. Check the four defining properties. 1. B~0=c−1/2B0=0\widetilde B_0 = c^{-1/2}B_0 = 0 a.s. ✓. 2. For 0=t0<t1<⋯<tn0=t_0<t_1<\cdots<t_n, the increments B~tj−B~tj−1=c−1/2(Bctj−Bctj−1)\widetilde B_{t_j} - \widetilde B_{t_{j-1}} = c^{-1/2}\big(B_{ct_j} - B_{ct_{j-1}}\big) are scalar multiples of the increments Bctj−Bctj−1B_{ct_j}-B_{ct_{j-1}} of the original process over the disjoint, ordered time points 0≤ct0<ct1<⋯<ctn0 \le ct_0 < ct_1 < \cdots < ct_n; independence of the latter (property (2) for BB) gives independence of the former. ✓ 3. Bctj−Bctj−1∼N(0,c(tj−tj−1))B_{ct_j}-B_{ct_{j-1}} \sim N(0, c(t_j-t_{j-1})), so B~tj−B~tj−1=c−1/2(Bctj−Bctj−1)∼N(0,c−1⋅c(tj−tj−1))=N(0,tj−tj−1)\widetilde B_{t_j}-\widetilde B_{t_{j-1}} = c^{-1/2}(B_{ct_j}-B_{ct_{j-1}}) \sim N\big(0, c^{-1}\cdot c(t_j-t_{j-1})\big) = N(0,t_j - t_{j-1}). ✓ 4. t↦B~t=c−1/2Bctt \mapsto \widetilde B_t = c^{-1/2}B_{ct} is a continuous function of tt whenever t↦Btt\mapsto B_t is, being a composition of a continuous linear rescaling of the time axis with a continuous path. ✓ So B~\widetilde B satisfies all four defining properties and is itself a standard Brownian motion. With c=4c=4: B~t=12B4t\widetilde B_t = \tfrac12 B_{4t} is standard Brownian motion. Now compute P(B12−B4>6)\mathbb{P}(B_{12}-B_4 > 6) directly: B12−B4∼N(0,12−4)=N(0,8)B_{12}-B_4 \sim N(0, 12-4) = N(0,8), so

P(B12−B4>6)=P(Z>68)=1−Φ(2.1213)≈0.01695.\mathbb{P}(B_{12}-B_4>6) = \mathbb{P}\Big(Z > \frac{6}{\sqrt8}\Big) = 1-\Phi(2.1213) \approx 0.01695.

Via the rescaled process with c=4c=4: B12=2B~3B_{12} = 2\widetilde B_3 and B4=2B~1B_4 = 2\widetilde B_1, so B12−B4=2(B~3−B~1)B_{12}-B_4 = 2(\widetilde B_3 - \widetilde B_1), and B~3−B~1∼N(0,2)\widetilde B_3 - \widetilde B_1 \sim N(0,2) since B~\widetilde B is standard Brownian motion. Then

P(B12−B4>6)=P(2(B~3−B~1)>6)=P(B~3−B~1>3)=P(Z>32)=1−Φ(2.1213)≈0.01695,\mathbb{P}(B_{12}-B_4>6) = \mathbb{P}\big(2(\widetilde B_3-\widetilde B_1) > 6\big) = \mathbb{P}(\widetilde B_3 - \widetilde B_1 > 3) = \mathbb{P}\Big(Z > \frac{3}{\sqrt2}\Big) = 1-\Phi(2.1213) \approx 0.01695,

matching exactly, since 3/2=6/83/\sqrt2 = 6/\sqrt8. This confirms the self-similarity computation is internally consistent and gives a genuine alternate route (useful, e.g., for reducing problems at "inconvenient" time scales to unit-scale computations).

CounterexampleDropping independent increments breaks the theorem

Suppose we keep properties (1), (3), (4) of the definition — zero start, marginal law N(0,t−s)N(0,t-s)-type stationarity, and continuous paths — but drop independence of increments (property (2)). Consider

Yt=t⋅Z,Z∼N(0,1),Y_t = t \cdot Z, \qquad Z \sim N(0,1),

a single Gaussian random variable scaling the identity function of tt. Then:

  • Y0=0Y_0 = 0 almost surely. ✓ (property 1 holds)
  • t↦Yt(ω)=tZ(ω)t \mapsto Y_t(\omega) = t Z(\omega) is continuous (indeed linear) in tt for every ω\omega. ✓ (property 4 holds)
  • Yt∼N(0,t2)Y_t \sim N(0, t^2) for each fixed tt, so the marginal variance is not even tt (it is t2t^2), but modify the example slightly: consider instead Y~t=t⋅Z\widetilde Y_t = \sqrt t \cdot Z. Then Y~t∼N(0,t)\widetilde Y_t \sim N(0, t) for each fixed tt, matching Brownian marginals exactly, and Y~0=0\widetilde Y_0 = 0, and paths t↦t Z(ω)t \mapsto \sqrt t\, Z(\omega) are continuous. So (1), (3)-at-fixed-tt, and (4) all hold in spirit.

But increments of Y~\widetilde Y are not independent, and in fact the process is completely different from Brownian motion: for 0<s<t0<s<t,

Y~t−Y~s=(t−s)Z,\widetilde Y_t - \widetilde Y_s = (\sqrt t - \sqrt s) Z,

which is perfectly correlated with Y~s=s Z\widetilde Y_s = \sqrt s\, Z (both are deterministic multiples of the same single random variable ZZ), rather than independent of it as Brownian increments must be. Concretely, Corr(Y~s,Y~t−Y~s)=±1≠0\mathrm{Corr}(\widetilde Y_s, \widetilde Y_t - \widetilde Y_s) = \pm 1 \ne 0. Consequently Cov(Y~s,Y~t)=st Var(Z)=st≠min⁡(s,t)\mathrm{Cov}(\widetilde Y_s,\widetilde Y_t) = \sqrt{s}\sqrt{t}\,\mathrm{Var}(Z) = \sqrt{st} \ne \min(s,t) in general (e.g. s=1,t=4s=1,t=4: st=2\sqrt{st}=2 but min⁡(s,t)=1\min(s,t)=1). The covariance structure derived in the theorem's part (c) genuinely used independence of increments (the cross term Cov(Bs,Bt−Bs)\mathrm{Cov}(B_s, B_t-B_s) vanished only because of independence); here that term does not vanish, and the entire process behaves like a single random line through the origin scaled by t\sqrt t — a process with only one degree of randomness (ZZ), utterly unlike Brownian motion's infinitely many degrees of freedom (a new independent "kick" at every instant). This shows property (2) is not redundant: dropping it, even while formally preserving the single-time marginal laws, produces a process with entirely different joint structure and different qualitative behavior (perfectly predictable future given any single observation, versus Brownian motion's genuinely unpredictable future increments).

Scope, edge cases & common traps

SituationWhat holdsWhat can go wrong
Finite-dimensional lawsAlways jointly Gaussian, covariance min⁡(s,t)\min(s,t)Forgetting increments (not raw values) are independent — Bs,BtB_s, B_t themselves are correlated
Path regularityContinuous a.s.; Hölder continuous of order <1/2<1/2Assuming differentiability or bounded variation — false a.s.
Scaling BctB_{ct}c−1/2Bctc^{-1/2}B_{ct} is again standard BMUsing wrong exponent (e.g. c−1Bctc^{-1}B_{ct}) — breaks unit variance
Multi-dimensional BMCoordinatewise independent 1-D BMsAssuming isotropy of increments implies coordinate independence without checking construction
Random walk approximationCLT gives convergence of finite-dim'l lawsBelieving finite-dim'l convergence alone implies path-space convergence (needs tightness, Donsker's theorem, beyond fdd's)

The mathematician behind it

Origins · 1 minNorbert Wiener and how this was discovered
NW
Norbert Wiener
1894–1964 · Mathematics, MIT, USA

Norbert Wiener gave the first rigorous mathematical construction of Brownian motion in 1923, proving the existence of a probability measure on the space of continuous functions — now called Wiener measure — realizing the process physicists had used heuristically since Einstein's 1905 kinetic-theory derivation and Bachelier's 1900 financial-mathematics thesis. Wiener's construction predated Kolmogorov's general axiomatization of probability (1933) and required inventing much of the machinery (generalized harmonic analysis, function-space integration) from scratch. He later became a founder of cybernetics and control theory.

History
- 1827 — Robert Brown observes erratic motion of pollen grains suspended in water.
- 1900 — Louis Bachelier models stock price fluctuations using what is essentially Brownian motion, in his doctoral thesis on speculation theory.
- 1905 — Albert Einstein derives the diffusion equation for Brownian particles from molecular kinetic theory, predicting mean-square displacement proportional to time.
- 1923 — Norbert Wiener constructs a rigorous probability measure on continuous path space realizing Brownian motion (Wiener measure).
- 1933 — Andrei Kolmogorov's axiomatic foundations of probability place Wiener's construction within the general framework of stochastic processes.
Is Brownian motion the same thing as a "random walk"?

No — a random walk is a discrete-time, discrete- or continuous-space process; Brownian motion is its continuous-time scaling limit. The connection is precise: rescale a mean-zero, finite-variance random walk by n\sqrt n in space while running nn steps per unit time, and the finite-dimensional distributions converge to those of Brownian motion, per the theorem above. The full statement that the entire path converges (not just finite snapshots) is Donsker's invariance principle, a strictly stronger and harder result requiring a tightness argument beyond simple CLT convergence.

Why must Brownian motion have Gaussian increments specifically, rather than some other distribution?

Given the axioms of stationary, independent increments and the requirement that the process arise as a scaling limit of sums of many small independent contributions, the Central Limit Theorem forces the limiting increment law to be Gaussian — this is exactly what the proof of part (a) demonstrates, and is not an extra assumption but a consequence of the CLT applied to sums of mj(n)→∞m_j^{(n)}\to\infty i.i.d. terms. More generally, any distribution arising as a limit of scaled sums of i.i.d. variables with finite variance must be Gaussian, by the classical CLT; only if one allows infinite-variance step distributions do other "stable" limit laws (with jumps) appear, giving Lévy processes instead.

Why is Brownian motion nowhere differentiable if its paths are continuous?

Continuity only requires that Bt+h−Bt→0B_{t+h}-B_t \to 0 as h→0h\to 0, which indeed holds since Var(Bt+h−Bt)=h→0\mathrm{Var}(B_{t+h}-B_t)=h\to0. Differentiability requires the stronger statement that (Bt+h−Bt)/h(B_{t+h}-B_t)/h converges to a finite limit. But the typical size of the increment is order h\sqrt h (its standard deviation), so the difference quotient has typical size h/h=h−1/2\sqrt h/h = h^{-1/2}, which blows up as h→0h\to 0. This heuristic, made rigorous through a careful Borel–Cantelli argument over dyadic partitions (the Paley–Wiener–Zygmund theorem), shows the path is almost surely nowhere differentiable, despite being continuous everywhere.

What does "independent increments" actually forbid, intuitively?

It forbids any memory in the process's future changes relative to its past changes. Concretely, knowing the entire path of BB up to time ss gives you zero information (beyond the current value being irrelevant to the shape of future increments) about the distribution of Bt−BsB_t - B_s for t>st>s. The counterexample above shows what happens without this: a process like Y~t=t Z\widetilde Y_t = \sqrt t\, Z has matching single-time marginals to Brownian motion but is driven by a single random variable ZZ, so the entire future path is perfectly determined (up to a deterministic function of tt) by any one observation — the opposite of Brownian motion's continual fresh randomness.

Does Brownian motion satisfy the Markov property?

Yes, and it follows directly from independent increments. Given the value Bs=xB_s = x, the future path (Bs+u)u≥0(B_{s+u})_{u\ge 0} has the same distribution as x+(Bu)u≥0x + (B_u)_{u \ge 0} for a fresh standard Brownian motion BuB_u, because Bs+u−BsB_{s+u} - B_s is independent of Fs=σ(Br:r≤s)\mathcal F_s = \sigma(B_r : r\le s) and has the law N(0,u)N(0,u) regardless of the past. This is the continuous-time analogue of the Markov property familiar from Random Walks, and it is foundational for treating Brownian motion as a diffusion process solving the heat equation via its transition densities.

Can Brownian motion be negative, and does it ever return to zero?

Yes to both. Since Bt∼N(0,t)B_t \sim N(0,t) for each t>0t>0, the process takes both positive and negative values with probability 1/21/2 each at any fixed time, and by continuity (Intermediate Value Theorem) it must cross zero between any two times where it has opposite sign. In fact standard Brownian motion returns to 00 infinitely often in any interval (0,ε)(0,\varepsilon) for every ε>0\varepsilon>0 — the set of zeros a.s. is an uncountable, closed, measure-zero (Cantor-like) set, a striking fact provable from the reflection principle and scaling invariance, though the full proof is beyond this introductory scope.

How does the covariance formula Cov(Bs,Bt)=min⁡(s,t)\mathrm{Cov}(B_s,B_t)=\min(s,t) actually get used in practice?

It lets you compute any joint probability about finitely many time points of Brownian motion using ordinary multivariate Gaussian machinery, without ever invoking path properties. Since (Bt1,…,Btk)(B_{t_1},\dots,B_{t_k}) is a mean-zero multivariate Gaussian vector with covariance matrix Σij=min⁡(ti,tj)\Sigma_{ij}=\min(t_i,t_j), any joint density, conditional distribution, or linear functional (e.g. P(B2>1,B5>4)\mathbb{P}(B_2>1,B_5>4) as in the worked example) reduces to standard multivariate normal computations, once you write down Σ\Sigma correctly using the min-covariance rule.

Before this