SUMMARY
The discussion centers on the integrated 3-body relativistic phase space for three particles of equal mass, specifically in the context of K+ decay to pi+ pi+ pi-. The formula provided for the integrated phase space is Φ = (1/(π³ 2⁷ M²)) ∫(s₂ to s₃) [(1/s) √((s-s₁)(s-s₂)(s₃-s)(s₄-s))] ds, where M is the initial mass and s₁, s₂, s₃, and s₄ are defined in terms of the particle masses. The user expresses difficulty in performing the integral analytically and suggests numerical integration as a viable approach. Additionally, a request for a similar formula for the integrated four-body phase space is made.
PREREQUISITES
- Understanding of relativistic kinematics
- Familiarity with phase space concepts in particle physics
- Knowledge of numerical integration techniques
- Basic grasp of decay processes and branching ratios
NEXT STEPS
- Research the derivation of integrated phase space formulas for multiple particle decays
- Learn numerical integration methods applicable to complex integrals in physics
- Explore the concept of branching ratios in particle decay processes
- Investigate the integrated four-body relativistic phase space and its applications
USEFUL FOR
Particle physicists, researchers in high-energy physics, and students studying decay processes and phase space calculations will benefit from this discussion.