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Group problem solutions

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Title: Group problem solutions


1
Group problem solutions
  • (a)
  • (b)

2
  • 2. In order to be reversible we need
  • or equivalently
  • Now divide by h and let h go to 0.
  • 3. Assuming (as in Holgate, Math. Gazette, 1967)
    that the intensity of amalgamation is
    proportional to the number of herds (perhaps it
    should be proportional to the number of pairs of
    herds) and the intensity of splitting a herd of
    size xi is proportional to xi-1, the overall
    intensity of splitting will be the sum of these.
    Hence the G-matrix has

3
  • so the equations for the stationary distribution
    are (using Holgates model)
  • whence the stationary distribution is
    1Bin(K-1,???????).

4
Browns motion
  • Richard Brown (1773-1858)
  • Scottish botanist
  • First systematic description of Australian fauna
  • Named the cell nucleus
  • Observed irregular pollen motion in liquid (first
    described by Ingenhousz in 1784)

5
Observed motion
6
Interpretation
  • The basic unit of living matter (molecule)
  • Same motion with dust particles (or carbon on
    oil)
  • Ongoing motion in closed box forever
  • Explained by fluctuating temperature due to
    heating by incident light electrical forces
    temperature difference in the liquid.
  • Delsaux (1877) impact of molecules of liquid on
    immersed particleslots of small bumps

7
Einsteins contribution
  • 1905 Annus mirabilis
  • Photoelectric effect
  • Special relativity
  • Emc2
  • On the Motion Required by the Molecular Kinetic
    Theory of Heat of Small Particles
    Suspended in a Stationary Liquid

8
Some physics
  • Two forces act on suspended particles
  • osmotic pressure (tendency towards equal
    concentration)
  • diffusion (particles hit by heat-induced movement
    of liquid molecules)
  • If q(x) is the density of particles per unit
    volume, the osmotic force is
  • (R gas constant, T abs temp, N Avogadros
    number)
  • This force causes flux

9
More physics
  • The flux due to diffusion with diffusion
    coefficient D is
  • These two fluxes must be equal in equilibrium, so
  • If we know D and r we can compute N (which was
    not known in 1905).

10
Einsteins stochastic model
  • Over a short time period ?, a particle is
    displaced by a random quantity Y. It should have
    mean 0 in equilibrium. Assume for simplicity
    with probability 1/2 each. Let x be a point. Only
    particles in (x-y,x) can pass x from left to
    right in a time interval ?.
  • Only half of those particles will in fact move
    from left to right, i.e. about particles.
  • Similarly, about particles move from
    right to left.

11
  • Net flux is then
  • and the quantity diffusing in unit time is
  • so Dy2/2?.
  • The displacement over unit time will be the sum
    of 1/? iid (why?) random variables, so has
    variance ?2Var(Y)/?.
  • Since Var(Y)y2 we have D?2/2.
  • Perrin used this to estimate Avogadros number.
    Nobel prize in physics, 1926.

12
The distribution of Brownian motion
  • A particle starting at the origin jumps Y units
    in time ?. The pgf of Y is
  • In time t, the particle takes t/??independent
    steps. The total displacement has pgf
  • with mean 0 and variance ty2/?.
  • In order to have the variance converge to ?2t we
    need y??1/2. Then

13
An excursion
  • Let XN(???2). Then

14
  • Let se?. This yields the moment generating
    function. We get
  • Exponentiating back we get the mgf for a
    N(0,?2t)-random variable.
  • One can use this type of limit to calculate the
    forward equation for the process, which turns out
    to be the heat equation.

15
A general definition
  • A Brownian motion process is a stochastic process
    having
  • Independent increments
  • Stationary increments
  • Continuity for any ???

16
Some Brownian motion process paths
17
Properties of Brownian motion process
  • X(t)N(?t,?2t)
  • Continuous paths
  • Finite squared variation
  • Not bounded variation
  • Not differentiable paths
  • Derivative of location is velocity, so for small
    time intervals this is not defined (not a very
    accurate model!)
  • Is it Markov?

18
More realistic assumption
  • Stationarity is the probability counterpart to
    conservation of momentum (mass x velocity)
  • Instead of independent increments of location, we
    could consider independent increments of momentum
  • Velocity change in particle would be twice the
    speed of the molecule times the ratio of molecule
    to particle mass

19
The Ornstein-Uhlenbeck approach
  • Let U(t) be the velocity of a particle.
    Langevins equation says
  • where K(t) is a stochastic process with mean
    zero and very quickly decreasing covariance
    (collisions from independent molecules)
  • Divide through by m to get ??/m and
    K(t)K(t)/m. Multiply by exp(?t), so

20
A formal solution
  • The integral makes sense if K(t) is continuous,
    but it probably is not.
  • Write formally K(t)dB(t)/dt to get
  • The problem is now to make sense of the
    stochastic integral on the rhs (492). The result
    is the Ornstein-Uhlenbeck process.

21
Properties of the O-U process
  • It is the only stationary Gaussian Markov process
    in continuous time and space.

22
The displacement
  • is another Gaussian process with mean X(0) and
    variance
  • For large t this behaves like a constant times t,
    as Einstein found, but for small t this behaves
    like t2. It has a derivative (velocity). Why?
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