Chapter 10: Brownian motion Flashcards
graphs of Brownian motion:
jagged movements
shown examples, for graphs of different times each pic has 1/5 of next. For T unit of time on the x-axis and root(T) units of space on the y-axis.
E[|X_T|]≈ root(T) as T tends to infinity
As we scale out we see convergence to a limit, random, continuous time stochastic processes.
THM 10.2.1
Brownian motion
There is a stochastic process (Bt) such that:
- The paths of (Bt) are continuous.
- For any 0 ≤ u ≤ t, the random variable Bt −Bu is independent of σ(Bv ; v ≤ u).
- For any 0 ≤ u ≤ t, the random variable Bt −Bu has distribution N(0,t−u).
1* Bt is a random continuous funct
2* movement between time t and u is indep f what happened before
(2 points in time indep of past)
Definition 10.2.2
STANDARD Brownian motion
If B0 = 0 we say that (Bt) is a standard Brownian motion.
WE DENOTE Bt as STANDARD BM: We write (Bt) for a standard Brownian motion, and Ft = σ(Bu ; u ≤ t) for its generated(natural) filtration. We work over the filtered space (Ω,F,(Ft),P)
Bt
We write (Bt) for a standard Brownian motion, and Ft = σ(Bu ; u ≤ t) for its generated filtration. We work over the filtered space (Ω,F,(Ft),P)
Brownian motion notes:
Bt (standard)
- B_t -B_0 ~N(0,t-0) so..
- Putting u = 0 into the second property and noting that B0 = 0, we obtain that the distribution of Brownian motion at time t is Bt ∼ N(0,t).
- B_t -B_0 ~N(0,t-0)
- E[Bt] = 0 for all t
- B^n_t ∈ L^1 for all n ∈ N. (*)
if Z ∼ N(0,t) then E[Z^2] = t.
so Brownian motion…
(*)
if Z ∼ N(0,t) then E[Z^2] = t.
Hence E[B^2_t ] = var(B_t) = t
for all t
if Z ∼ N(µ,σ^2) then
E[e^Z]
(*)
if Z ∼ N(µ,σ2) then
E[e^Z] = e^{µ+(1/2)σ^2}
E[e^{B_t}]
*
E[e^{B_t}] = e^{t/2}
B_t^n ∈ L^p for all p ≥ 1
B_t^n ∈ L^p for all p ≥ 1
⇔
E[|B_t|^p] less than infinity for all t,p
Brownian motion and heat equation
Temp @ position x @ time t is u(t,x), t ∈ [0,∞) time and x ∈R space.
Suppose at t=0 temp at point x is f(x)=u(0,x)
heat equation is
∂u/∂t = ∂^2u/∂x^2
with the initial condition
u(0,x) = f(x)
If we start Brownian motion from x ∈ R, then Bt ∼ x + N(0,t) ∼ N(x,t), so we can write down its probability density function
φ_{t,x}(y) =
(1 /√2πt) exp[−(y−x)^2/2t]
LEMMA 10.3.1
A sol of the heat equation
φt,x(y) satisfies the heat equation
φ_{t,x}(y) =
(1 /√2πt) exp[−(y−x)^2/2t]
If we start Brownian motion from x ∈ R, then Bt ∼ x + N(0,t) ∼ N(x,t), so we can write down its probability density function
Proof 10.3.1
φt,x(y) satisfies the heat equation
φ_{t,x}(y) =
(1 /√2πt) exp[−(y−x)^2/2t]
Because if u(t,x) solves so does u(t,x-y)
for any value of y. Assume y=0 and need to show that
φt,x(0) =
(1 /√2πt) exp[−(x^2/2t] satisfies ∂u/∂t = ∂^2u/∂x^2. Partial differentiation: chain and product rule
∂ φ/∂ t= (-0.5/√(2πt^3))exp(-x^2/2t)+ (1/√2πt)(-x^2(-1)/2t^2)exp(-x^2/2t)
1 √2π x2 2t5/2 − 1 t3/2exp−x2 2t and ∂φ ∂x = (1/√2πt)(−2x/2t) exp(−x2^/2t).
= −x/√2πt^3 exp(−x2^/2t).
so as
∂2φ/∂x2
= −1 √2πt3 exp−x2 2t+ −x √2πt3 −2x 2t
exp(−x2^/2t).
=
(1/√2π)[( x^2/2t^{5/2}) −
1/t^{3/2}] exp(−x2^/2t).
Hence, ∂φ/∂t = ∂^2φ/∂x^2 .
Lemma 10.3.2
We can use Lemma 10.3.1 to give a physical explanation of the connection between Brownian motion and heat diffusion. We define
w(t,x) = E_x[f(B_t)
That is, to get w(t,x), we start a particle at location x, let it perform Brownian motion for time t, and then take the expected value of f(Bt).
w(t,x)
w(t,x) = E_x[f(B_t)
satisfies
heat equation
∂u/∂t = ∂^2u/∂x^2
and the initial condition
u(0,x) = f(x)
PROOF
Lemma 10.3.2
w(t,x) = E_x[f(B_t)
satisfies
heat equation
∂u/∂t = ∂^2u/∂x^2
and the initial condition
u(0,x) = f(x)
w(t,x)= E_x[f(B_t)] = integral from -infinity to infinity of [ f(y)φ_{t,x}(y)].dy
*by looking in reverse to see how much heat there was initially
E_x[f(B_t)
start BM at x and consider packets of heat moving with BM
- f represents initial cond: how muh heat initially u(0,x)=f(x)
- B_t is heat varying ranf back in time
- E_x approx average heat effect over lots of heat packets
Consequently u=u
PROOF:
B_0=x, So w(0,x)= E_x[f(B_0) = E_x[f(x)] = f(x) and hence initial cond satisfied
integral from -∞ to ∞ of [f(y) (∂/∂t)(φt,x(y))]dy integral from -∞ to ∞ of [f(y) (∂^2/∂x^2)(φt,x(y))]dy = (∂^2/∂x^2) integral from -∞ to ∞ of f(y)φ_{t,x}(y)dy = ∂^2w/∂x^2