Quantum Theory Flashcards
Give 5 problems which are unresolved without quantum theory
- Photoelectric effect
- Discrete emission/absorption spectra
- Double slit experiment
- De-Broglie’s matter-wave properties
- Compton scattering
Give the de Broglie relations
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.
State Schrodinger’s Equation
iℏ(∂Ψ/∂t) = −ℏ^2(∇^2)Ψ/2m + VΨ
State the Stationary State Schrodinger Equation
−ℏ^2(∇^2)ψ/2m + Vψ = Eψ, where Ψ(x,t) = ψ(x)e^(−iEt/ℏ)
For a particle with potential 0 inside the interval (0,a) and infinite potential outside, give the permitted energies of the particle.
E = En = (nπℏ)^2/2ma^2.
Define the ground state
When the possible energies of a system are discrete and bounded below, the wavefunction with the lowest possible energy is called the ground state.
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.
E = E_(n1,n2,n3) = (πℏ)^2/2m[(n1/a)^2+(n2/b)^2+(n3/c)^2]
Define degeneracy
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).
Give the probability postulate
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.
Define a normalisable wave function
A wave function Ψ is normalisable if 0 < triple integral over R3 of |Ψ(x, t)|^2 < ∞ for all t.
Define a normalised wave function
A wave function Ψ is normalised if triple integral over R3 of |Ψ(x, t)|^2 =1 for all t.
Define the correspondence principle
The tendency for quantum results to approach classical results for large quantum numbers.
Define the expectation of a position function
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
Define the probability current of a wave function.
j(x,t) = iℏ/2m[Ψ(x,t){(∇Ψ)(x,t)}* − {Ψ(x,t)}*(∇Ψ)(x,t)].
Give the conditions of a wave function
- Wave functions must be continuous, single-valued functions. This condition ensures that the probability density is single-valued and has no discontinuities.
- Wave functions must be normalizable.
- ∇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.
Define the potential of the one-dimensional harmonic oscillator
The one-dimensional harmonic oscillator potential for angular frequency ω is V(x) = 1/2m(ωx)^2.
Define an even parity state
In one dimension a stationary state wave function satisfying ψ(−x) = ψ(x) is said to describe even parity state.
Define an odd parity state
In one dimension a stationary state wave function satisfying ψ(−x) = -ψ(x) is said to describe odd parity state.
State the allowed energies of a one-dimensional harmonic oscillator
The energies of the one-dimensional quantum harmonic oscillator of angular frequency ω are E = En = (n + ½)ℏω.
Define the complex inner product of a wave function
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).
Define a Hilbert space
A complete complex inner product space is called a Hilbert space.
State the Hilbert space postulate
The states of a quantum system are elements of a Hilbert space.