Probability Theory and Statistics required for random wave motion analysis

Summary of Contents

  • 1.Probability spaces.
  • 2. Random variables
  • 3. Lebesgue integral w.r.t. a measure and w.r.t. a probability measure
  • 4. Cornerstone theorems of Lebesgue’s theory of integration: Monotone convergence. Fatou’s lemma and dominated convergence.
  • 5. Moments of a random variable, mean, variance, skewness and higher moments.
  • 6. The direct product of a finite number of measures and Fubini’s theorem on change in the order of integration.
  • 7. Karl Pearson’s correlation coefficient.
  • 8. Absolute continuity of measures, the Radon-Nikodym theorem and probability distributions and densities.
  • 9. Conditional expectation and conditional probability.
  • 10. Quantum probability space: Events, observables and states in a quantum probability space.
  • 11. Joint probability distribution of classical random variables.
  • 12. Heisenberg’s uncertainty principle for non-commuting observables and the impossibility of defining joint probabilities for non-commuting observables in the quantum theory.
  • 13. Positive definitivity of the joint characteristic function of classical random variables.
  • 14. Bochner’s theorem in classical probability.
  • 15. Non-positive definitivity of joint characteristic functions of non-commuting observables in the quantum theory.
  • 16. The inequalities of John Bell and the consequent impossibility of constructing a hidden variable theory for quantum mechanics.
  • 17. Classical stochastic processes: Brownian motion, Poisson process and more generally Levy processes.
  • 18.Ito’s formula for Brownian motion and Poisson processes.
  • 19. Quantum Brownian motion and quantum Poisson processes: Noncom-mutative generalizations of classical BM and classical PP.
  • 20. Realizing classical stochastic processes using families of operators in Boson Fock space in a coherent state.
  • 21. Bernoulli random variables in classical and quantum probability.
  • 22. Stochastic differential equations driven by Brownian motion: Existence and Uniqueness.
  • 23. Stochastic differential equations driven by Levy processes.
  • 24. The generalized Ito-Doleans Dade-Meyer differential rule for discontinuous Martingales.
  • 25. Girsanov’s formula for the change of drift in an sde.
  • 26. Quantum stochastic differential equations in the sense of Hudson and Parthasarathy; Existence and Uniqueness of solutions.
  • 27. Some practical applications of quantum probability.

[a] Computation of scattering cross sections.

[b] The wave function of our universe: Wheeler-Dewitt-Hartle-Hawking’s theory. The Hartle-Hawking theory of the probability distribution of the radius of our universe with a scalar field coupling.

[c] Computation of tunneling probabilities of a quantum particle through a potential barrier with applications to tunneling diode.

[d] Probability of induced transitions in a laser; The interaction of Light with atoms-The Glauber-Sudarshan theory.

[e] Energy bands in a semiconductor-the theory based on Bloch wave functions; Specialization to the Kronig-Penney model.

[f] Modeling quantum systems coupled to a noisy bath—The Hudson-Parthasarathy equation and its solution using Maasen’s kernel approach and using the functional form of the Glauber-Sudarshan representation.

Probability spaces and measure theoretic theorems on probability spaces

A triplet (Q, J-, P) where U is called the sample space of the experiment, P is the a-field of events and P is a probability measure.

  • 2. Random variables
  • 3. Lebesgue integral w.r.t. a measure and w.r.t. a probability measure
  • 4. Cornerstone theorems of Lebesgue’s theory of integration: Monotone convergence, Fatou’s lemma and dominated convergence.
  • 5. Moments of a random variable, mean, variance, skewness and higher mo-ments.
  • 6. The direct product of a finite number of measures and Fubini’s theorem on change in the order of integration.
  • 7. Karl Pearson’s correlation coefficient.
  • 8. Absolute continuity of measures, the Radon-Nikodym theorem and probability distributions and densities.
  • 9. Conditional expectation and conditional probability.

Basic facts about quantum probability

  • 10. Quantum probability space: Events, observables and states in a quantum probability space.
  • 11. Joint probability distribution of classical random variables.
  • 12. Heisenberg’s uncertainty principle for non-commuting observables and the impossibility of defining joint probabilities for non-commuting observables in the quantum theory.
  • 13. Positive definitivity of the joint characteristic function of classical random variables.
  • 14. Bochner’s theorem in classical probability.
  • 15. Non-positive definitivity of joint characteristic functions of non-commuting observables in the quantum theory.
  • 16. The inequalities of John Bell and the consequent impossibility of constructing a hidden variable theory for quantum mechanics.

Given three random variables Xi, X2, ^3, each assuming values ±1 only, we observe that

X3(X!-X2) < l-XiX2

Taking expectations gives

E(X!X3) - E(X2X3) < 1 - E(%!X2)

Interchanging Xi and X2 gives

E(X2X3) - E(XrX3) < 1 - E(X1X2)

Thus,

lEpQXa) - E(X2X3)I < 1 - E(XjX2)

This is called Bell’s inequality for Bernoulli random variables. It is violated in certain cases for quantum Bernoulli random variables. For example, consider 1,2,3 ie, the Pauli spin matrices. These matrices have eigenvalues ±1 but do not commute. Choose unit directions ni,n2,n3 and consider the observables

Xk = (nie, a) = ntiCTi + nfc22 + nfc3<73, k = 1, 2,3

Then,

XkXm = (nk,nm) +i(a,hk x nm)

Now, we can choose the state

P = (W2

Then,

Tr(p<7fc) = 0, k = 1,2,3

and we have

Tr{pXkXm) = (hk, hm), k, m = 1, 2,3

Let Okm be the angle between hk and nm. Then to verify Bell’s inequality, for the quantum observables Xi, X%, X3, we require that

|cos(0i3) - COS(6*23)| < 1 - cos(0i2)

for all points on the unit sphere. Now, suppose we choose n3 as the north pole and |#i — O21 < e. Then by an appropriate choice of e, Bell’s inequality will be violated.

 
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