Glossary
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An experimental topic | Quantum Mechanics is our best description of what we observe in experiments, even though we cannot observe the wavefunction.
Basis functions | Any quantum state can be expanded in a complete set of basis functions. The choice of basis set has no physical meaning.
Binding |
Born Approximation | At high energy, scattering can be treated by perturbation theory. The scattered wave depends on a matrix element which is the Fourier transform of the potential. ⟨k′|ˆV|k⟩=∫∫∫V(r) exp (−iχ.r)dτ;χ≡k′−k For elastic scattering from a central potential this becomes: dσdΩ=m2(ksinθ2)2ℏ4|∫∞0rV(r)sin(2krsinθ2)dr|2
Curvature | The kinetic energy is related to the curvature of a wave. Thus ground states tend to have smooth wavefunctions and no nodes.
Degenerate Perturbation Theory | The perturbed wavefunction is a linear combination of the unperturbed, degenerate states. Calculate eigenstates and eigenvalues from the matrix: |V11−ΔEjV12…V1NV21V22−ΔEj…V2N…………VN1VN2…VNN−ΔEj|=0 With every degeneracy there is an associated symmetry and conservation law.
Exchange | Much of the bonding comes from exchange integrals - interference between an electrons on different atoms. When two particles are indistinguishable, the wavefunction must be (anti)symmetric, so is usually a sum of two terms. Since measurable quantities (intensities, matrix element) involve the wavefunction times itself, this gives interference terms: exchange.
Expectation value | The expectation value is the predicted mean value of the result of an experiment for a system in a given quantum state. This mean value may not correspomnd to any of the quantised states of the system if it is not in an eigenstate of the operator whose expectation value is sought.
Hidden Variables | Quantum mechanics requires a collapse of a spatially extended wavefunction instantaneously. If it could be used to transport information, this “action at a distance” would be conflict with relativity, but nobody has yet done so.
Indistinguishable Particles | Quantum mechanical intensities cannot depend on labels on indistinguishable particles. Thus wavefunctions must be either symmetric (bosons) or antisymmetric (fermions) with respect to exchange of any such labels. Appropriate wavefunctions are “Slater determinants” of matrices.
Integrals | The most important property of a matrix element is whether it is zero. This determines whether something can happen or not.
Many-Fermions |
Measurement | A measurement is an interaction between the quantum system and the rest of the universe which collapses the system into an eigenstate of the quantity being measured
Partial Wave Analysis | Low energy scattering is homogeneous: we consider only s-waves.
Relativistic Quantum Mechanics | The Schrödinger equation is non-relativistic. The Klein Gordon equation, the natural generalization to E2=p2c2+m2c4, gives “free particle” solutions with negative energy and negative probability. The Dirac Equation, another generalisation, can only be solved for a four-component wavefunction, which represents spin-half and antimatter.
Scattering | Describing scattering involves solving the Schrödinger equation for an incoming plane wave and outgoing spherical wave.
The wavefunction and interference |
Time independent Perturbation Theory | For the energy, to first order, you can assume that the wavefunction is unchanged and evalulate the energy shift from the matrix element ΔE0≈⟨n0|ˆV|n0⟩≡V00 For the wavefunctions, the amount of other unperturbed wavefunction mixed in depends on the matrix element between them, and their energy difference. |ϕ0⟩=|n0⟩+∑k≠0⟨nk|ˆV|n0⟩(E0−Ek)|nk⟩≡|n0⟩+∑k≠0Vk0(E0−Ek)|nk⟩ For the energy, to second order, we consider mixing of the wavefunctions: ΔE0=0+∑i=1,∞⟨ni|ˆV|n0⟩V0i(E0−Ei)=∑i=1,∞|Vi0|2(E0−Ei)
Time-dependence | Wavefunctions oscillate in time as exp(iEt/ℏ) but intensities do not e−iEt/ℏeiEt/ℏ=1.
Time-dependent Perturbation Theory | If a system starts in state |k⟩,(cm(t)=0) the probability that it will shift to state |k⟩ in time t depends on the matrix element cm(t)=(iℏ)−1∫t0Vmk exp(iωmkt)dt For a harmonic perturbation we get a resonance when the perturbing frequency matches the energy difference between the states m and k: |cm(t)|2=V2mksin2[(ωmk−ω)t/2]ℏ2(ωmk−ω)2=4ℏ2V2mkf(t,ωmk−ω) Energy is extracted from the perturbing potential. If the transition is to a group of near-degenerate states, The transition rate depends on the square of the matrix element, and the density of states, as given by Fermi’s Golden rule: R=2πℏ[|Vmk|2g(Em)]Em=Ek
Variational Principle | A surprisingly good estimate of the ground state energy comes from minimising the expectation value of the energy for an arbitrary, normalised trial wavefunction ϕ(an). E[an]≈Minan(⟨ϕ(an)|ˆH|ϕ(an)⟩⟨ϕ(an)|ϕ(an)⟩) Excited states can also be found using trial wavefunctions orthogonal to the ground state.