Relativistically invariant 2-body phase space integral

In summary, The conversation discusses the use of a function, represented as ##\lambda^{\frac{1}{2}}##, in the calculation of a relativistically invariant 2-body phase space integral. The function is shorthand for ##\sqrt{\lambda (x,y,z)}## and can be found in various textbooks and lecture notes on relativistic particle kinematics. The Källén function is a commonly used reference for this function, while the Review of Particle Physics provides a comprehensive overview of kinematics in relativistic scattering problems.
  • #1
George Wu
6
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TL;DR Summary
I encounter a function that I don‘t know in the calculation of Relativistically invariant 2-body phase space integral
I encounter a function that I don‘t know in the calculation of Relativistically invariant 2-body phase space integral:
1684333571500.png

in this equation, ##s##is the square of total energy of the system in the center-of-mass frame(I think)
I don't know what the function ##\lambda^{\frac{1}{2}}## is.
There are more equations involving this function:
P$3{FTJ%2Z0E4A%)9[BD%[C.png

I just want to know if anyone knows which textbook these equations come from, or what the function ##\lambda^{\frac{1}{2}}## is.
 
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  • #2
Do you have any reference for those 2 screenshots? A book, some lecture notes we could have access to. Otherwise, I can't recall any special function in mathematics with that notation.
 

FAQ: Relativistically invariant 2-body phase space integral

What is a relativistically invariant 2-body phase space integral?

A relativistically invariant 2-body phase space integral is a mathematical expression used in particle physics to describe the distribution of momenta and energies of two particles in the final state of a relativistic collision or decay process. It ensures that the calculations respect the principles of special relativity.

Why is relativistic invariance important in phase space integrals?

Relativistic invariance is crucial because it ensures that the physical laws and calculations remain consistent and accurate regardless of the observer's frame of reference. This is a fundamental requirement in high-energy physics where particles often move at speeds close to the speed of light.

How is the 2-body phase space integral calculated?

The 2-body phase space integral is calculated by integrating over the allowed momentum and energy configurations of the two final-state particles. This involves using delta functions to enforce energy and momentum conservation and integrating over the invariant mass and angles of the final particles.

What are the applications of the 2-body phase space integral in particle physics?

The 2-body phase space integral is used in various applications including the calculation of decay rates, cross-sections for scattering processes, and in the analysis of particle collisions. It helps in predicting the outcomes and distributions of particles resulting from high-energy interactions.

What challenges are associated with computing the relativistically invariant 2-body phase space integral?

Challenges include the complexity of ensuring relativistic invariance, handling singularities that may arise in the integrals, and dealing with the high-dimensional integrals that require sophisticated numerical methods. Accurate computations often necessitate advanced techniques in mathematical physics and computational algorithms.

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