Index
Chapter 4 · Item 4.1
Bound and unbound states: chapter roadmap
Discrete spectra, continuum states and the logic of one-dimensional models
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Guided reading

Chapter 4 turns the general rules of wave mechanics into a systematic problem-solving method. The potential divides space into regions; the time-independent Schrödinger equation determines the local form of the wave function; boundary and normalizability conditions select the physically allowed solutions.

Two energy regimes

A bound state is spatially localized and normalizable. Its wave function decays where the energy lies below the asymptotic potential, and its allowed energies form a discrete set.

An unbound state extends to infinity. It represents propagation or scattering and belongs to a continuous energy spectrum.

\[\int_{-\infty}^{\infty}|\psi(x)|^2\,dx=1\quad\text{(bound state)}\]
Time-independent Schrödinger equation (TISE)

Every model begins with

\[-\frac{\hbar^2}{2m}\frac{d^2\psi}{dx^2}+V(x)\psi=E\psi\]

The sign of \(E-V\) controls the local behavior: oscillatory when \(E>V\), exponential when \(E<V\). This observation anticipates confinement, penetration and tunneling.

Five models, one strategy
ModelCentral idea
Harmonic oscillatorSmooth confinement and equally spaced energies
Finite wellBoundary matching and transcendental quantization
Attractive well, \(E>0\)Reflection, transmission and resonances
Delta wellDerivative jump at a singular potential
Rectangular barrierEvanescent waves and tunneling
A reusable solve sequence
  • Sketch \(V(x)\), mark the energy, and divide space into regions.
  • Write the correct local solution in each region.
  • Discard divergent terms and impose continuity conditions.
  • Use normalization for bound states or probability current for scattering states.
  • Check dimensions, limiting cases and physical interpretation.
From energy comparison to solution type

Begin locally. In a region where the potential is constant, the TISE can be written as

\[\psi''+k^2\psi=0,\qquad k^2=\frac{2m(E-V)}{\hbar^2}\]

For \(E>V\), \(k\) is real and the independent solutions oscillate. For \(E<V\), write \(k=i\kappa\); the solutions are exponential:

\[\psi(x)=Ae^{\kappa x}+Be^{-\kappa x}\]

For a bound state, the exponentially growing branch is discarded at each infinity. For scattering, the oscillatory branches are assigned directions and interpreted through current.

Bound-state energies and scattering states

For a bound state, solve in every region and ask whether a globally continuous, differentiable and normalizable wave function exists. This occurs only for isolated energies, giving a discrete spectrum. For an unbound state, the incident energy is continuous; matching fixes the reflected and transmitted amplitudes.

Local form → global physics

Quantization and scattering are not separate rules. Both follow from joining local solutions into one acceptable global wave function. For a bound state, the matching conditions select isolated energies. For a scattering state, they determine amplitude ratios and therefore \(R\) and \(T\).

Exercise-ready boundary

This page is designed to support short guided exercises on: Bound and unbound states: chapter roadmap.

  • Use from this page: the definitions, physical setup, highlighted equations and conceptual links needed to start a first calculation or explanation.
  • Keep in the book: complete derivations, extended historical discussion, worked solutions and the full textbook narrative remain in the original chapter and linked book resources.
  • Good exercise balance: ask the student to identify assumptions, apply one relation, and interpret the result physically, without requiring material not introduced on this page.
Practice anchors

Use these anchors to design compact exercises. The exercise should be answerable from this page plus standard algebra, while longer derivations, full worked examples and broader context should point back to the original book.

  • Focus: Bound and unbound states: chapter roadmap.
  • Conceptual check: state what the main result says physically before using it algebraically.
  • Equation: \[-\frac{\hbar^2}{2m}\frac{d^2\psi}{dx^2}+V(x)\psi=E\psi\]
  • Boundary: use this page for setup and first-step reasoning; cite the book for longer derivations, complete experimental history or solved-problem detail.
  • Typical task: derive, interpret, or apply the relation above to a simple case without introducing topics outside this page.
Source note: Original auxiliary summary for this book-app, based on Chapter 4 of Mario Reis, Quantum Mechanics, Elsevier, 2026. Book text and figures are copyright © 2026 Elsevier Inc.; consult the original book for the complete presentation, derivations and exercises.