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| <center><math>\frac{s-4m^2}{4}= \vec p \ ^{*2})</math></center> | | <center><math>\frac{s-4m^2}{4}= \vec p \ ^{*2}</math></center> |
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| | <center><math>\frac{s(s-4m^2)}{4s}= \vec p \ ^{*2}</math></center> |
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| | <center><math>t=-2 p \ ^{*2}(1-cos\ \theta)=\frac{-2s(s-4m^2)}{4s}(1-cos\ \theta)</math></center> |
Revision as of 01:50, 14 June 2017
[math]\displaystyle{ \textbf{\underline{Navigation}} }[/math]
[math]\displaystyle{ \vartriangleleft }[/math]
[math]\displaystyle{ \triangle }[/math]
[math]\displaystyle{ \vartriangleright }[/math]
Limits based on Mandelstam Variables
Since the Mandelstam variables are the scalar product of 4-momenta, which are invariants, they are invariants as well. The sum of these invariant variables must also be invariant as well. Find the sum of the 3 Mandelstam variables when the two particles have equal mass in the center of mass frame gives:
[math]\displaystyle{ s+t+u=(4(m^2+ p \ ^{*2}))+(-2 p \ ^{*2}(1-cos\ \theta))+(-2 p \ ^{*2}(1+cos\ \theta)) }[/math]
[math]\displaystyle{ s+t+u \equiv 4m^2 }[/math]
Since
[math]\displaystyle{ s \equiv 4(m^2+\vec p \ ^{*2}) }[/math]
This implies
[math]\displaystyle{ s \ge 4m^2 }[/math]
In turn, this implies
[math]\displaystyle{ t \le 0 \qquad u \le 0 }[/math]
At the condition both t and u are equal to zero, we find
[math]\displaystyle{ t = 0 \qquad u = 0 }[/math]
[math]\displaystyle{ -2 p \ ^{*2}(1-cos\ \theta) = 0 \qquad -2 p \ ^{*2}(1+cos\ \theta) = 0 }[/math]
[math]\displaystyle{ (-2 p \ ^{*2}+2 p \ ^{*2}cos\ \theta) = 0 \qquad (-2 p \ ^{*2}-2 p \ ^{*2}cos\ \theta) = 0 }[/math]
[math]\displaystyle{ 2 p \ ^{*2}cos\ \theta = 2 p \ ^{*2} \qquad -2 p \ ^{*2}cos\ \theta = 2 p \ ^{*2} }[/math]
[math]\displaystyle{ \cos\ \theta = 1 \qquad \cos\ \theta = -1 }[/math]
[math]\displaystyle{ \Rightarrow \theta_{t=0} = \arccos \ 1=0^{\circ} \qquad \theta_{u=0} = \arccos \ -1=180^{\circ} }[/math]
Holding u constant at zero we can find the minimum of t
[math]\displaystyle{ s+t_{max} \equiv 4m^2 }[/math]
[math]\displaystyle{ \Rightarrow t_{max}=4m^2-s }[/math]
[math]\displaystyle{ t_{max}=4m^2-4m^2- 4p \ ^{*2} }[/math]
The maximum transfer of momentum would be
[math]\displaystyle{ t_{max}=-4p \ ^{*2} }[/math]
[math]\displaystyle{ -2 p \ ^{*2}(1-cos\ \theta_{t=max})=-4p \ ^{*2} }[/math]
[math]\displaystyle{ (1-cos\ \theta_{t=max})=2 }[/math]
[math]\displaystyle{ -cos\ \theta_{t=max}=1 }[/math]
[math]\displaystyle{ \theta_{t=max} \equiv \arccos -1 }[/math]
The domain of the arccos function is from −1 to +1 inclusive and the range is from 0 to π radians inclusive (or from 0° to 180°). We find as expected for u=0 at [math]\displaystyle{ \theta=180^{\circ} }[/math]
[math]\displaystyle{ \theta_{t=max}=180^{\circ} }[/math]
However, from the definition of s being invariant between frames of reference
[math]\displaystyle{ s \equiv \overbrace{\left({\mathbf P_1^*}+ {\mathbf P_2^{*}}\right)^2=\left({\mathbf P_1^{'*}}+ {\mathbf P_2^{'*}}\right)^2}^{CM\ FRAME}=\overbrace{\left({\mathbf P_1}+ {\mathbf P_2}\right)^2 = \left({\mathbf P_1^{'}}+ {\mathbf P_2^{'}}\right)^2}^{LAB\ FRAME} }[/math]
In the center of mass frame of reference,
[math]\displaystyle{ E_1^*=E_2^*=E^* \quad and \quad \vec p \ _1^*=-\vec p \ _2^*= \vec p \ ^* }[/math]
[math]\displaystyle{ s \equiv 2m^2+2(E_1^{*2}+\vec p \ ^{*2} ) }[/math]
Using the relativistic energy equation
[math]\displaystyle{ E^2 \equiv \vec p \ ^2+m^2 }[/math]
[math]\displaystyle{ s \equiv 2m^2+2((m^2+\vec p \ ^{*2})+\vec p \ ^{*2}) }[/math]
[math]\displaystyle{ s=4m^2+4 \vec p \ ^{*2}) }[/math]
[math]\displaystyle{ \frac{s-4m^2}{4}= \vec p \ ^{*2} }[/math]
[math]\displaystyle{ \frac{s(s-4m^2)}{4s}= \vec p \ ^{*2} }[/math]
[math]\displaystyle{ t=-2 p \ ^{*2}(1-cos\ \theta)=\frac{-2s(s-4m^2)}{4s}(1-cos\ \theta) }[/math]