For λ=0.1 and ⟨n∣V∣n⟩=3 eV, find the first-order energy shift.
Answer and explanation
0.3 eV
Multiply the matrix element by λ.
Subjects
Choose questions individually, practise online, or create a worksheet with matching answers. Counts include generated variants, not only authored originals.
0.3 eV
Multiply the matrix element by λ.
⟨n∣V∣n⟩
The diagonal expectation in the unperturbed state is the first-order coefficient.
4.8 eV
Add the correction to the unperturbed value.
Diagonalize the perturbation restricted to that subspace
The appropriate combinations resolve first-order splitting.
State-mixing corrections involve energy-gap denominators. A small gap can make the ratio large despite a small numerator.
Credit relative scales rather than coupling size alone.
3 eV
The weighted diagonal mean is 2/2+4/2.
Write H=H0+λV and expand observables or states about a solvable reference problem. Small λ is useful only relative to relevant spectral scales.
Advanced universityWrite H=H0+λV and expand observables or states about a solvable reference problem. Small λ is useful only relative to relevant spectral scales.
Advanced universityScattering models compare incoming and outgoing waves far from a localized interaction. Boundary conditions identify which waves are physically incident.
Advanced universityScattering models compare incoming and outgoing waves far from a localized interaction. Boundary conditions identify which waves are physically incident.
Advanced universityFor a normalized trial state in the Hamiltonian domain, the expectation of a Hamiltonian bounded below is at least its ground energy.
Advanced universityFor a normalized trial state in the Hamiltonian domain, the expectation of a Hamiltonian bounded below is at least its ground energy.
Advanced universityConnect rotation, oscillations, central forces and continuous wave models.
Work with Gauss laws, electrical field models, thermodynamic laws and electromagnetic waves.
Compare relativistic measurement with quantum states, the Schrödinger equation and uncertainty.
Use Lagrangian and Hamiltonian methods, then interpret canonical ensembles.
Explore perturbation theory, scattering, variational quantum estimates and a conceptual bridge to general relativity.