From matrix element to hadronic cross section

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SUMMARY

The discussion focuses on calculating the hadronic cross section from a matrix element in a 2->3 scattering process involving quarks. The matrix element is derived from five Feynman diagrams and is expressed in terms of scalar products of four-momenta. Key formulas include the differential cross section dσ and the phase space factor dΦ, with specific equations provided for both two and three outgoing particles. The most comprehensive resource cited is S.J. Chang's book on Quantum Field Theory, which elaborates on these calculations in detail.

PREREQUISITES
  • Understanding of Feynman diagrams and their role in particle physics
  • Familiarity with Quantum Field Theory (QFT) concepts
  • Knowledge of relativistic kinematics and four-momenta
  • Experience with phase space integrals in scattering processes
NEXT STEPS
  • Study the derivation of the hadronic cross section in Quantum Field Theory
  • Learn about phase space integrals for multiple particle final states
  • Review S.J. Chang's book on QFT for detailed explanations of scattering theory
  • Examine relevant papers on 2->3 scattering processes for practical examples
USEFUL FOR

Particle physicists, theoretical physicists, and researchers working on scattering processes and hadronic cross sections will benefit from this discussion.

ayseo
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Hello,

currently I work on 2->3 scattering process. So there exist five external momenta and in my case 5 different Feynman diagrams, for which I have already calculated the full matrix element.
The matrix element is a function of various scalar products of the four-momenta. This scattering contains quarks. My next aim is to calculate the hadronic cross section from the matrix element.

Can someone explain me how can I do this?
 
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ayseo, I think this topic is mentioned in almost every treatment of scattering theory, and 99 percent of those treatments are way too brief to be of any use. The most complete discussion I've found is in a book on QFT by S.J. Chang, which devotes ten pages to it.

You need to put a factor in front due to the initial flux, and a factor in back due to the final phase space. The general result for a collision of two particles a and b is

dσ = (2ωab vab)-1|ℳ|2

where dΦ is the phase space factor,

dΦ = (2π)4 δ4(∑ki - P) Π (d3ki/((2π)3i)

ℳ of course is the relativistically invariant amplitude calculated from the Feynman diagram. 1/2ωa is a boson kinematical factor ("wavefunction normalization"), one for each particle both incoming and outgoing. For fermions use M/E instead.

vab = |va - vb| is the relative velocity of a and b. ωi, ki are the energy/momenta of the individual outgoing particles, while E, P are the total energy/momentum.

Bad enough already, but the real ugly part comes when you go to integrate out the four δ-functions and express the (redundant) ki's in terms of the desired experimental parameters. Quoting Chang, for two outgoing particles,

dΦ = k131/(16π2 (E k12 - ω1 P·k1))

For three outgoing particles, (take a deep breath!)

dΦ = k12k22 dk112/((2π)51 [k22(E - ω1) - ω2 k2·(P - k1)])
 
there's an older paper that sets up a lot of these phase space integrals, and I believe a production process with 2->3 is done in the appendix of :

http://prola.aps.org/abstract/PR/v185/i5/p1865_1
and some more in
http://prd.aps.org/abstract/PRD/v2/i9/p1902_1
 

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