Physic Labs

Particle physics

Quantum chromodynamics (QCD)

Watch a high-energy photon convert into an electron–positron pair in a nuclear field and the spiraling tracks of both particles in the detector's magnetic field. Vary photon energy and field strength to verify the threshold Eγ≥1,022E_γ\geq1{,}022 MeV and the track radius r=p/(qB)r=p/(qB) scaling inversely with B.

Research

Equipment

  • Virtual detector chamber with magnetic field and nuclear Coulomb field
  • Photon-energy slider (readout in MeV)
  • Magnetic-field slider (readout in tesla)
  • 'Change energy split' button sharing energy between the pair
  • Pause button and two opposite helical tracks on the 3D canvas

Procedure

  1. Create a pair above threshold

    Pull the photon-energy slider below 1 MeV: the readout warns 'Eγ below the 1.022 MeV threshold' and no pair forms. Raise it to tens of MeV: the photon becomes an electron and a positron — the threshold is the rest energy 2mec2≈1,0222m_ec^2\approx1{,}022 MeV of the two particles.

  2. Read track radius in the field

    At fixed energy, watch the two tracks curl in opposite senses — electron and positron carry opposite charges. Lower the field slider B: the spirals widen since the radius r=p/(qB)r=p/(qB) is inversely proportional to B; this is how detectors measure charged-particle momentum.

  3. Change the energy split and compare showers

    Press 'Change energy split' to redivide the photon energy between the particles: the less energetic one curls tighter. Push Eγ to maximum and see secondary tracks multiply — hinting at the particle shower that QCD hadronizes from quarks and gluons in a real detector.

Simulation

Experiment history

Photon pair production γ → e⁺e⁻ was predicted in late-1920s quantum electrodynamics and first seen in cloud chambers; in 1932 Carl David Anderson discovered the positron in cosmic rays using exactly the magnetic-curvature technique this simulation illustrates. Quantum chromodynamics was built in the early 1970s: Murray Gell-Mann framed 'color' charge from his quark model (1964), and in 1973 David Gross, Frank Wilczek, and David Politzer showed the strong force weakens at short distance — 'asymptotic freedom' explains why quarks never appear singly but only as hadron showers in detectors.

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