Difference between revisions of "Relativistic Differential Cross-section"
		
		
		
		
		
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| <center><math>|p_2^2| =E_2^2-m^2=\frac{(\mathbf P_1 \cdot \mathbf P_2)^2}{m^2}-m^2=\frac{(\mathbf P_1 \cdot \mathbf P_2)^2-m^4}{m^2}</math></center> | <center><math>|p_2^2| =E_2^2-m^2=\frac{(\mathbf P_1 \cdot \mathbf P_2)^2}{m^2}-m^2=\frac{(\mathbf P_1 \cdot \mathbf P_2)^2-m^4}{m^2}</math></center> | ||
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|   In the frame where one of the particles (particle 1) is at rest , the relative velocity can be expressed as |   In the frame where one of the particles (particle 1) is at rest , the relative velocity can be expressed as | ||
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| <center><math> v_2=\frac{|\vec p_2|}{E_2}</math></center> | <center><math> v_2=\frac{|\vec p_2|}{E_2}</math></center> | ||
Revision as of 01:24, 4 July 2017
Relativistic Differential Cross-section
dQ is the invariant Lorentz phase space factor
and F is the flux of incoming particles
where v is the relative velocity between the particles. 
Using the relativistic definition of energy
In the frame where one of the particles (particle 1) is at rest , the relative velocity can be expressed as
The invariant form of F is
 
In the center of mass frame