Difference between revisions of "Relativistic Differential Cross-section"
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− | <center><math>F=4\sqrt{\left ( \frac{s^2-4sm^2+4m^4}{4} \right )-m^4}</math></center> | + | <center><math>F=4\sqrt{\left ( \frac{s^2-4sm^2+4m^4}{4} \right )-m^4}=4\sqrt{\left ( \frac{s^2-4sm^2}{4} \right )}</math></center> |
+ | |||
+ | |||
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+ | where | ||
+ | <center><math>s_{CM}=4(m^2+\vec p_1 \ ^{*2})=(2E_1^*)^{2}</math></center> | ||
+ | |||
+ | |||
+ | <center><math>F=4\sqrt{\left ( \frac{(4(m^2+\vec p_1 \ ^{*2}))^2-4(4sm^2}{4} \right )}</math></center> | ||
Revision as of 02:59, 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
where
In the center of mass frame