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The general definition of the cross section is given by (e. g. [H+02])
 |
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(1.5) |
where denotes the n-particle phase space of the final-state particles,
stands for the symmetry factor of the final state and
represents the flux factor of the particles and . This flux factor can be expressed in the center of mass system by
with the CM-momentum of the particles and .
In [Leh03]1.2 it was shown that one can express the cross section for the production of unstable particles and in the final state by
 |
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(1.6) |
with and denoting the CM momenta of the and the -system. Here one needs to assume that the Matrix element is only dependend on . The spectral functions depend only in the medium, which explicitly breaks Lorentz-invariance, on the four-momenta of the particles. Considering the vacuum-case they will only depend on the squares
.
For a three-particle final state one gets a more complicated result due to a rising number of degrees of freedom in the final state
Here denote the CM-momenta of the particles c and d. The CM-momentum of is given by total momentum conservation
Subsections
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Oliver Buss
2005-03-16
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