Quantum Wave Mechanics: Free Space Propagation and Bound States in Infinite Potential Wells

Administrative and Organizational Logistics

  • Homework Assignment Schedule:
    • The next homework assignment is released today.
    • Next Monday is a designated holiday; no lecture will take place.
    • The default submission deadline for the homework is set for Tuesday evening.
    • Potential deadline extension: The deadline may shift to Wednesday evening if necessary, but students should plan around the Tuesday submission target.
    • Homework scheduling follows a Sunday/Monday periodicity cadence.

Non-Relativistic Schrödinger Equation and Wave Mechanics Review

  • Space-Form Non-Relativistic Schrödinger Equation (Time-Independent):

    • −ℏ22md2ψ(x)dx2+V(x)ψ(x)=Eψ(x)-\frac{\hbar^2}{2m} \frac{d^2\psi(x)}{dx^2} + V(x)\psi(x) = E\psi(x)
  • Time-Dependent Wave Function Component:

    • Features a sinusoidal waveform represented in complex exponential form: ϕ(t)=e−jωt=e−jEℏt\phi(t) = e^{-j\omega t} = e^{-j\frac{E}{\hbar}t}
    • Energy EE acts as the separation constant arising from spatial and temporal separation of variables.
    • Angular frequency ω\omega connects directly to energy through E=ℏωE = \hbar\omega.
  • Probability Density Function and Fundamental Boundary Conditions:

    • The overall spatial-temporal probability density is defined as: P(x,t)=Ψ(x,t)Ψ∗(x,t)=∣Ψ(x,t)∣2P(x,t) = \Psi(x,t)\Psi^*(x,t) = |\Psi(x,t)|^2
    • Spatial probability density (time-independent): P(x)=ψ(x)ψ∗(x)=∣ψ(x)∣2P(x) = \psi(x)\psi^*(x) = |\psi(x)|^2
    • Existence / Normalization Boundary Condition: The particle must exist somewhere in the total spatial domain, requiring the spatial integral over all space to equal unity: ∫−∞∞∣ψ(x)∣2dx=1\int_{-\infty}^{\infty} |\psi(x)|^2 dx = 1
    • Continuity Conditions: The wave function ψ(x)\psi(x) and its first derivative dψ(x)dx\frac{d\psi(x)}{dx} must be continuous, finite, and single-valued across space for finite potentials V(x)V(x).
    • These physical constraints align strictly with the Heisenberg Uncertainty Principle.

Free Particle Kinematics and Traveling Wave Solutions

  • Free Space Scenario Definition:

    • Assumes an electron moving in free space without influence from atomic nuclei or periodic lattice potentials (V(x)=C=0V(x) = C = 0 everywhere).
  • Simplified Differential Equation for Free Space (V=0V = 0):

    • −ℏ22md2ψ(x)dx2=Eψ(x)-\frac{\hbar^2}{2m} \frac{d^2\psi(x)}{dx^2} = E\psi(x)
    • Rearranged standard second-order homogeneous form: d2ψ(x)dx2+2mEℏ2ψ(x)=0\frac{d^2\psi(x)}{dx^2} + \frac{2mE}{\hbar^2}\psi(x) = 0
  • Exponential Solution Form:

    • ψ(x)=Aej2mEℏ2x+Be−j2mEℏ2x\psi(x) = A e^{j \sqrt{\frac{2mE}{\hbar^2}} x} + B e^{-j \sqrt{\frac{2mE}{\hbar^2}} x}
  • Wave Number kk Definition:

    • k=2mEℏ2=2mEℏk = \sqrt{\frac{2mE}{\hbar^2}} = \frac{\sqrt{2mE}}{\hbar}
    • E=ℏ2k22mE = \frac{\hbar^2 k^2}{2m}
    • Parabolic Dispersion Relation: Energy EE is proportional to k2k^2 (E∝k2E \propto k^2), yielding a parabolic energy-wavevector curve.
  • Total Spatial-Temporal Wave Function Ψ(x,t)\Psi(x,t):

    • Ψ(x,t)=ψ(x)e−jωt=Aej(kx−ωt)+Be−j(kx+ωt)\Psi(x,t) = \psi(x) e^{-j\omega t} = A e^{j(kx - \omega t)} + B e^{-j(kx + \omega t)}
    • Component $A e^{j(kx - \omega t)}$: Represents a plane wave traveling in the positive $x−direction(-direction (+x$).
    • Component Be−j(kx+ωt)B e^{-j(kx + \omega t)}: Represents a plane wave traveling in the negative xx-direction (−x-x).
  • Momentum and De Broglie Relationships:

    • Momentum magnitude: p=ℏkp = \hbar k
    • De Broglie wavelength: \lambda = \frac{h}{p} = \frac{2\pi\hbar}{p} = \frac{2\pi}{k}
    • Wave number in terms of wavelength: k=2πλk = \frac{2\pi}{\lambda}
  • Unidirectional Motion (+x+x Direction Only, B=0B = 0):

    • Wave function: Ψ(x,t)=Aej(kx−ωt)\Psi(x,t) = A e^{j(kx - \omega t)}
    • Probability Density Evaluation:
    • ∣Ψ(x,t)∣2=Ψ(x,t)Ψ<em>(x,t)=(Aej(kx−ωt))(A</em>e−j(kx−ωt))=∣A∣2|\Psi(x,t)|^2 = \Psi(x,t)\Psi^<em>(x,t) = \left(A e^{j(kx - \omega t)}\right) \left(A^</em> e^{-j(kx - \omega t)}\right) = |A|^2
    • Implication: The spatial dependence completely cancels out, making the probability density ∣A∣2|A|^2 a constant across all positions xx.
    • Heisenberg Uncertainty Relation: Having an exact, single wave vector kk implies precise momentum (p=ℏkp = \hbar k, so Δp=0\Delta p = 0). Consequently, the spatial position uncertainty becomes infinite (Δx→∞\Delta x \rightarrow \infty), meaning the electron can be found anywhere in space with equal probability.
    • Localization: To construct a spatially localized electron (wave packet), one must combine a superposition of wave functions possessing a range of distinct kk values.

Bound Electrons: Infinite Potential Well Formulation

  • Physical Motivation:

    • Electrons in solid-state devices, crystals, and semiconductors are rarely free; they are confined by localized potential wells V(x)V(x).
  • One-Dimensional Infinite Potential Well System Geometry:

    • Region 0≤x≤a0 \le x \le a (Inside Well): V(x)=0V(x) = 0, width of well is aa.
    • Region x<0x < 0 and x>ax > a (Barriers): V(x)=V0→∞V(x) = V_0 \rightarrow \infty.
  • Wave Function Behavior at Infinite Barriers (V→∞V \rightarrow \infty):

    • For any finite energy EE, the potential energy inside the barrier is infinitely larger than EE.
    • Wave function value outside the well: ψ(x)=0\psi(x) = 0 for x<0x < 0 and x>ax > a.
    • Boundary values: ψ(0)=0\psi(0) = 0 and ψ(a)=0\psi(a) = 0.
    • Exception to Derivative Continuity: The first derivative dψ(x)dx\frac{d\psi(x)}{dx} is not continuous at the boundaries x=0x = 0 and x=ax = a due to the non-physical infinite potential step V→∞V \rightarrow \infty.
  • Internal Differential Equation (0≤x≤a0 \le x \le a):

    • d2ψ(x)dx2+k2ψ(x)=0\frac{d^2\psi(x)}{dx^2} + k^2\psi(x) = 0, where k=2mEℏ2k = \sqrt{\frac{2mE}{\hbar^2}}
  • Trigonometric Solution Form:

    • ψ(x)=A1cos⁡(kx)+A2sin⁡(kx)\psi(x) = A_1 \cos(kx) + A_2 \sin(kx)
  • Application of Boundary Conditions:

    • Boundary at x=0x = 0:
    • ψ(0)=A1cos⁡(0)+A2sin⁡(0)=A1(1)+A2(0)=A1=0\psi(0) = A_1 \cos(0) + A_2 \sin(0) = A_1 (1) + A_2 (0) = A_1 = 0
    • Since ψ(0)=0\psi(0) = 0, A1A_1 must equal zero, eliminating the cosine term entirely.
    • Remaining wave function: ψ(x)=A2sin⁡(kx)\psi(x) = A_2 \sin(kx)
    • Boundary at x=ax = a:
    • ψ(a)=A2sin⁡(ka)=0\psi(a) = A_2 \sin(ka) = 0
    • To avoid trivial solutions (A2=0A_2 = 0, which implies no particle exists), we require sin⁡(ka)=0\sin(ka) = 0.
    • Constraint equation: ka=nπka = n\pi, where nn is an integer.
    • Quantized wave vector values: kn=nπak_n = \frac{n\pi}{a} for n=1,2,3,…n = 1, 2, 3, \dots
    • Note on quantum numbers: nn must be a positive integer (n∈Z+n \in \mathbb{Z}^+). Negative integers yield redundant states, and n=0n = 0 results in ψ(x)=0\psi(x) = 0 everywhere.
  • Normalization Determination of Coefficient A2A_2:

    • ∫0a∣ψ(x)∣2dx=∫0aA22sin⁡2(nπxa)dx=1\int_{0}^{a} |\psi(x)|^2 dx = \int_{0}^{a} A_2^2 \sin^2\left(\frac{n\pi x}{a}\right) dx = 1
    • Using trigonometric identity sin⁡2(θ)=1−cos⁡(2θ)2\sin^2(\theta) = \frac{1 - \cos(2\theta)}{2}:
    • A22∫0a1−cos⁡(2nπxa)2dx=A22(a2)=1A_2^2 \int_{0}^{a} \frac{1 - \cos\left(\frac{2n\pi x}{a}\right)}{2} dx = A_2^2 \left(\frac{a}{2}\right) = 1
    • A2=2aA_2 = \sqrt{\frac{2}{a}}
  • Normalized Spatial Wave Function for State nn:

    • ψn(x)=2asin⁡(nπxa)\psi_n(x) = \sqrt{\frac{2}{a}} \sin\left(\frac{n\pi x}{a}\right)

Energy Quantization, Standing Waves, and Physical Interpretations

  • Quantized Energy Levels Derivation:

    • Equating kn=nπak_n = \frac{n\pi}{a} with kn=2mEnℏ2k_n = \sqrt{\frac{2mE_n}{\hbar^2}}:
    • kn2=n2π2a2=2mEnℏ2k_n^2 = \frac{n^2 \pi^2}{a^2} = \frac{2mE_n}{\hbar^2}
    • En=n2π2ℏ22ma2E_n = \frac{n^2 \pi^2 \hbar^2}{2m a^2}
    • Substitution with Planck's constant (h=2πℏh = 2\pi\hbar):
    • En=n2h28ma2E_n = \frac{n^2 h^2}{8m a^2}
  • Physical Differences Between Free and Bound States:

    • Free Electrons: Form continuous traveling waves ej(kx−ωt)e^{j(kx - \omega t)}.
    • Bound Electrons: Form localized standing waves sin⁡(nπxa)\sin\left(\frac{n\pi x}{a}\right).
    • Instrument Analogy: Equivalent to acoustic standing waves on guitar strings or inside woodwind instruments (clarients), where fixed physical boundaries restrict resonance to specific harmonic modes/frequencies.
  • Ground State and Zero-Point Energy:

    • Lowest allowed quantum energy state occurs at n=1n = 1:
    • E1=π2ℏ22ma2>0E_1 = \frac{\pi^2 \hbar^2}{2m a^2} > 0
    • Key Principle: Ground state energy E1E_1 cannot be zero ($E_1 eq 0$) even though $V(x) = 0$ inside the well. A confined quantum particle cannot possess zero kinetic energy without violating spatial uncertainty constraints.
  • Spatial Probability Density Distribution Characteristics ∣ψn(x)∣2|\psi_n(x)|^2:

    • Ground State (n=1n = 1):
    • Features a single symmetric probability peak located directly in the center (x=a2x = \frac{a}{2}).
    • Probability decays smoothly towards zero at the hard boundary walls x=0x = 0 and x=ax = a.
    • Second State (n=2n = 2):
    • Displays two symmetric probability peaks separated by an internal node (zero probability) at x=a2x = \frac{a}{2}.
    • Third State (n=3n = 3):
    • Displays three probability peaks separated by two internal nodes.
    • High Quantum Numbers (n→∞n \rightarrow \infty) and Classical Correspondence:
    • As nn increases, spatial probability oscillations become exceedingly dense.
    • Averaging over macroscopic spatial intervals smooths the rapid oscillations into an effectively constant spatial line (P≈1aP \approx \frac{1}{a}).
    • Demonstrates the Correspondence Principle: At high quantum numbers (n≫1n \gg 1), quantum mechanical predictions merge smoothly with classical macroscopic physics, where a classical bouncing particle has uniform spatial probability throughout a box.