Physic Labs

Quantum mechanics

Spin and the Pauli exclusion principle

Explore spin-1/2: a pure state is a point on the Bloch sphere, yet a Stern–Gerlach measurement yields only two outcomes with Born probability P(+)=cos⁡2(θ/2)P(+)=\cos^2(\theta/2). Set polar angle θ, azimuth φ, and the angle between preparation and measurement axes to verify the beam split.

Undergraduate

Equipment

  • Virtual Bloch sphere with a red state vector precessing in a field
  • Sliders for polar angle θ, azimuth φ, time t
  • Stern–Gerlach beam-splitting simulation with two spots
  • Slider for the angle between preparation and measurement axes; particle count

Procedure

  1. Read probabilities on the Bloch sphere

    In figure 1 set θ = 0: the vector points to the north pole and the readout gives P(+z) = 100%. Raise θ to 90° (equator) for P(+) = P(−) = 50%, and θ = 180° for P(−z) = 100% — matching P(+)=cos⁡2(θ/2)P(+)=\cos^2(\theta/2).

  2. Analyze the Stern–Gerlach split

    In figure 2, set the axis angle to 0 and raise the particle count: all particles land in one spot. Set 90°: two equally bright spots. Read the 'Born prediction' line and compare the theoretical P(+) with the counted split.

  3. Change precession time and conclude

    Raise the time slider t: the vector precesses around the field and ⟨σ⟩ rotates continuously, yet outcomes remain only ±ℏ/2 — the two-level nature of spin-1/2. Predict P(+) at θ = 60° and check with P=cos⁡2(30°)=0,75P=\cos^2(30°)=0{,}75.

Simulation

Experiment history

In 1922 Otto Stern and Walther Gerlach fired a beam of silver atoms through an inhomogeneous magnetic field and saw it split into two — quantization of magnetic-moment orientation, later understood as the electron's spin ±1/2. George Uhlenbeck and Samuel Goudsmit proposed spin in 1925 to explain fine spectral structure. Wolfgang Pauli that same year stated the exclusion principle: no two fermions in an atom share the same set of quantum numbers — explaining the periodic table and later derived from the antisymmetry of many-body wavefunctions (the spin–statistics theorem of Fierz and Pauli, 1939–40). Pauli received the 1945 Nobel Prize.

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