Quantum Theory Flashcards

1
Q

Give 5 problems which are unresolved without quantum theory

A
  1. Photoelectric effect
  2. Discrete emission/absorption spectra
  3. Double slit experiment
  4. De-Broglie’s matter-wave properties
  5. Compton scattering
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2
Q

Give the de Broglie relations

A

E = ℏω, p = ℏk, where E is the energy of a free particle, p is the momentum associated with a wave of angular frequency ω and k is the wave vector.

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3
Q

State Schrodinger’s Equation

A

iℏ(∂Ψ/∂t) = −ℏ^2(∇^2)Ψ/2m + VΨ

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4
Q

State the Stationary State Schrodinger Equation

A

−ℏ^2(∇^2)ψ/2m + Vψ = Eψ, where Ψ(x,t) = ψ(x)e^(−iEt/ℏ)

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5
Q

For a particle with potential 0 inside the interval (0,a) and infinite potential outside, give the permitted energies of the particle.

A

E = En = (nπℏ)^2/2ma^2.

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6
Q

Define the ground state

A

When the possible energies of a system are discrete and bounded below, the wavefunction with the lowest possible energy is called the ground state.

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7
Q

For a particle with potential 0 inside the interval (0,a)x(0,b)x(0,c) and infinite potential outside, give the permitted energies of the particle.

A

E = E_(n1,n2,n3) = (πℏ)^2/2m[(n1/a)^2+(n2/b)^2+(n3/c)^2]

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8
Q

Define degeneracy

A

The degeneracy of an energy level E of a system is the dimension of the solution space to the stationary state Schrödinger equation with energy E (though by convention, if this is one, it is said to be non-degenerate).

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9
Q

Give the probability postulate

A

The function ρ(x, t) ≡ |Ψ(x, t)|^2 is a probability density function for the position of the particle, where Ψ(x, t) is the particle’s wave function.

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10
Q

Define a normalisable wave function

A

A wave function Ψ is normalisable if 0 < triple integral over R3 of |Ψ(x, t)|^2 < ∞ for all t.

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11
Q

Define a normalised wave function

A

A wave function Ψ is normalised if triple integral over R3 of |Ψ(x, t)|^2 =1 for all t.

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12
Q

Define the correspondence principle

A

The tendency for quantum results to approach classical results for large quantum numbers.

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13
Q

Define the expectation of a position function

A

The expectation value of a function of position f(x) is given by the triple integral over R3 of f(x)|Ψ(x, t)|^2

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14
Q

Define the probability current of a wave function.

A

j(x,t) = iℏ/2m[Ψ(x,t){(∇Ψ)(x,t)}* − {Ψ(x,t)}*(∇Ψ)(x,t)].

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15
Q

Give the conditions of a wave function

A
  1. Wave functions must be continuous, single-valued functions. This condition ensures that the probability density is single-valued and has no discontinuities.
  2. Wave functions must be normalizable.
  3. ∇Ψ must be continuous everywhere, except where there is an infinite discontinuity in the potential V. This is necessary since a finite discontinuity in ∇Ψ implies an infinite discontinuity in ΔΨ, and thus from the Schrodinger equation an infinite discontinuity in V.
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16
Q

Define the potential of the one-dimensional harmonic oscillator

A

The one-dimensional harmonic oscillator potential for angular frequency ω is V(x) = 1/2m(ωx)^2.

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17
Q

Define an even parity state

A

In one dimension a stationary state wave function satisfying ψ(−x) = ψ(x) is said to describe even parity state.

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18
Q

Define an odd parity state

A

In one dimension a stationary state wave function satisfying ψ(−x) = -ψ(x) is said to describe odd parity state.

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19
Q

State the allowed energies of a one-dimensional harmonic oscillator

A

The energies of the one-dimensional quantum harmonic oscillator of angular frequency ω are E = En = (n + ½)ℏω.

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20
Q

Define the complex inner product of a wave function

A

Let ϕ and ψ be wavefunctions. Then we define the complex inner product ⟨ϕ|ψ⟩ as the integral from -∞ to ∞ of ϕbar(x)ψ(x).

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21
Q

Define a Hilbert space

A

A complete complex inner product space is called a Hilbert space.

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22
Q

State the Hilbert space postulate

A

The states of a quantum system are elements of a Hilbert space.

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23
Q

Define adjointness

A

If A is a linear operator acting on a complex inner product space, then the adjoint A∗ of A satisfies ⟨A∗ϕ|ψ⟩ = ⟨ϕ|Aψ⟩, for all ϕ, ψ ∈ H.

24
Q

Define self-adjointness

A

A linear operator A is self-adjoint if A∗ = A.

25
Q

State the observables postulate

A

The observables of a quantum system are given by self-adjoint linear operators on the space of states.

26
Q

Define the position operator

A

The position operator X in three dimensions has components Xi that are defined on wave functions ψ ∈ H via (Xiψ)(x) = xiψ(x). In vector form, Xψ = xψ.

27
Q

Define the momentum operator

A

The momentum operator P has components Pi that are defined on differentiable wave functions ψ by (Piψ)(x) = −iℏ∂ψ/∂(xi)(x). In vector form, Pψ = −iℏ∇ψ.

28
Q

Define the Hamiltonian operator

A

The Hamiltonian operator for a particle of mass m moving in a potential V is H = |P|^2/2m + V(X).

29
Q

Give the Hamiltonian version of the Schrodinger equation

A

The Schrodinger equation for time-dependent states ψ(t) is iℏ∂ψ(t)/∂t = Hψ(t), with stationary state ψ(t) = ψe^(−iEt/ℏ) of energy E satisfies Hψ = Eψ.

30
Q

Define an eigenstate

A

Given an observable A, then a state ψ ∈ H satisfying Aψ = αψ for some constant α ∈ C, is called an eigenstate of A, with eigenvalue α.

31
Q

Define a spectrum

A

The spectrum of an observable A is the set of all eigenvalues of A.

32
Q

State the Dirac span postulate

A

An observable A in quantum theory is required to have a complete set of eigenstates. That is, there is a set of orthonormal eigenstates {ψn} of A, such that any ψ ∈ H can be written as a linear combination of ψn.

33
Q

State the quantum measurement postulate

A

The possible outcomes of a measurement of an observable A are given by the eigenvalues {αn} of A. If the system is in a normalized quantum state ψ, then the probability of obtaining the value αn in a measurement, for a non-degenerate eigenvalue αn, is Pψ(obtaining αn) = |⟨ψn|ψ⟩|2.

34
Q

State the collapse of the wave function postulate

A

If one measures the observable A and obtains the non-degenerate eigenvalue αn, then immediately after the measurement the quantum state of the system is the eigenstate ψn ∈ H with Aψn = αnψn.

35
Q

Define the expectation of an operator

A

The expectation value of an operator A in a normalized quantum state ψ is Eψ(A) ≡ ⟨ψ|Aψ⟩.

36
Q

Define the identity operator

A

The identity operator 1 satisfies 1ψ = ψ, for all ψ ∈ H

37
Q

Define a non-negative operator

A

An operator A is said to be non-negative if ⟨ψ|Aψ⟩ ≥ 0, for all ψ ∈ H.

38
Q

Define the dispersion of an operator

A

The dispersion of an observable A in a normalized quantum state ψ is ∆ψ(A) ≡ sqrt(Eψ((A − Eψ(A)1)^2) = sqrt(Eψ(A^2) − (Eψ(A))^2).

39
Q

Define the commutator of two operators

A

The commutator of two operators A and B is [A, B] ≡ AB − BA.

40
Q

Give the canonical commutations

A

[Xi , Pj] = iℏδij1
[Xi, Xj] = 0 = [Pi , Pj].

41
Q

Give Leibniz’s rule of commutations

A

[A, BC] = B[A, C] + [A, B]C

42
Q

Give Jacobi’s identity of commutations

A

[A, [B, C]] + [B, [C, A]] + [C, [A, B]] = 0.

43
Q

State Heisenberg’s uncertainty principle

A

For normalized ψ we have ∆ψ(X)∆ψ(P) ≥ 1/2ℏ and equality holds if and only if ψ(x) = exp[(x − µ)^2/2s0ℏ + γ], for some negative constant s0, and complex constants µ, γ ∈ C.

44
Q

Define a minimum uncertainty state

A

A wave function ψ such that ∆ψ(X)∆ψ(P) = 1/2ℏ.

45
Q

Define the raising/lowering operators

A

a± = (∓iP + mωX)/sqrt(2mωℏ)

46
Q

Define the number operator

A

N = (a+)(a-)

47
Q

Define the orbital angular momentum operator

A

The angular momentum operator L = (X2P3 − X3P2, X3P1 − X1P3, X1P2 − X2P1).

48
Q

Define the Levi-Cevita alternating symbol

A

The Levi-Civita alternating symbol ϵijk, defined by ϵijk = +1 if ijk is an even permutation of 123, −1 if ijk is an odd permutation of 123 and 0 otherwise.

49
Q

Define the angular momentum operator

A

Any self-adjoint vector operator J, with components Ji, i = 1, 2, 3, satisfying [Ji , Jj ] = iℏ times the sum by k of ϵijkJk.is called an angular momentum operator.

50
Q

Define total angular momentum

A

The total angular momentum is defined by J^2 = (J1)^2 + (J2)^2 + (J3)^2.

51
Q

Define the raising and lowering operators of angular momentum

A

J± = J1 ± iJ2.

52
Q

Give the Pauli matrices

A

The 2x2 matrices σ1 = (0 1), (1 0), σ2 = (0 −i) (i 0), σ3 = (1 0) (0 −1).

53
Q

Give the spin representation of angular momentum

A

Ji = ℏσi/2, where σi are the Pauli matrices are the matrix representation of spin.

54
Q

Give Coulemb’s potential

A

V(r) = e1e2/(4πrϵ0)

55
Q

Give the Laplacian in spherical coordinates

A

∇^2 = (1/r^2)d/dr[(r^2)d/dr] + (1/(r^2)sinθ)d/dθ[(sinθ)d/dθ] + (1/(r^2)sin^2(θ))d2/dϕ^2

56
Q

Give the Bohr radius

A

The Bohr radius is a = 4πϵ0ℏ^2/me^2.