SUMMARY
The discussion clarifies the differences in angular distributions between Bhabha scattering and muon pair production. Bhabha scattering, represented as e+ e- → e+ e-, involves an additional Feynman diagram allowing for both scattering and pair annihilation/production. In contrast, muon pair production, e+ e- → μ+ μ-, occurs solely through pair annihilation. The scattering amplitudes are defined as Mμ = (u2 + t2)/s2 and Mel = (s2 + u2)/t2 + 2u2/(ts) + Mμ, with cross-sections proportional to the squares of these amplitudes.
PREREQUISITES
- Understanding of Feynman diagrams
- Knowledge of Mandelstam variables (s, t, u)
- Familiarity with high-energy particle physics
- Basic algebra for calculating scattering amplitudes
NEXT STEPS
- Study Feynman diagrams in detail
- Learn about Mandelstam variables and their applications
- Research the principles of high-energy particle collisions
- Explore the algebraic methods for calculating cross-sections in particle physics
USEFUL FOR
Physicists, students of particle physics, and researchers interested in the differences between Bhabha scattering and muon pair production.