Difference between revisions of "Relativistic Differential Cross-section"
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<center><math>s \equiv 2m^{2}+2 \mathbf P_1^* \mathbf P_2^* \rightarrow \mathbf P_1^* \mathbf P_2^* = \frac{s-2m^2}{2}</math></center> | <center><math>s \equiv 2m^{2}+2 \mathbf P_1^* \mathbf P_2^* \rightarrow \mathbf P_1^* \mathbf P_2^* = \frac{s-2m^2}{2}</math></center> | ||
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+ | <center><math>F=4\sqrt{( \frac{s-2m^2}{2})^2-m^4}</math></center> | ||
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Revision as of 02:53, 4 July 2017
Relativistic Differential Cross-section
dQ is the invariant Lorentz phase space factor
and F is the flux of incoming particles
where is the relative velocity between the particles in the frame where particle 1 is at rest
Using the relativistic definition of energy
Letting be the energy of particle 2 wiith respect to particle 1, the relativistic energy equation can be rewritten such that
where similarly
is defined as the momentum of particle 2 with respect to particle 1.
The relative velocity can be expressed as
The invariant form of F is
In the center of mass frame