Limits based on Mandelstam Variables: Difference between revisions

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<center><math>\textbf{\underline{Navigation}}</math>
<center><math>\underline{\textbf{Navigation}}</math>


[[U-Channel|<math>\vartriangleleft </math>]]
[[U-Channel|<math>\vartriangleleft </math>]]
[[VanWasshenova_Thesis#Moller_Scattering|<math>\triangle </math>]]
[[VanWasshenova_Thesis#Moller_Scattering|<math>\triangle </math>]]
[[Limits_based_on_Mandelstam_Variables|<math>\vartriangleright </math>]]
[[Limit_of_Energy_in_Lab_Frame|<math>\vartriangleright </math>]]


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<center><math>\Rightarrow  \theta_{t=0} = \arccos \ 1=0^{\circ}  \qquad \theta_{u=0} = \arccos \ -1=180^{\circ}</math></center>
<center><math>\Rightarrow  \theta_{t=0} = \arccos \ 1=0^{\circ}  \qquad \theta_{u=0} = \arccos \ -1=180^{\circ}</math></center>


Holding u constant at zero we can find the maximum of t
Holding u constant at zero we can find the minimum of t




<center><math>s+t \equiv 4m^2</math></center>
<center><math>s+t_{max} \equiv 4m^2</math></center>






<center><math>\Rightarrow t=4m^2-s</math></center>
<center><math>\Rightarrow t_{max}=4m^2-s</math></center>






<center><math>t=4m^2-4m^2+ 4p \ ^{*2})</math></center>
<center><math>t_{max}=4m^2-4m^2- 4p \ ^{*2}</math></center>






<center><math>t=4p \ ^{*2}</math></center>


The maximum transfer of momentum would be




<center><math>-2 p \ ^{*2}(1-cos\ \theta)=4p \ ^{*2}</math></center>
<center><math>t_{max}=-4p \ ^{*2}</math></center>






<center><math>(1-cos\ \theta)=-2</math></center>


<center><math>-2 p \ ^{*2}(1-cos\ \theta_{t=max})=-4p \ ^{*2}</math></center>




<center><math>-cos\ \theta=-3</math></center>


<center><math>(1-cos\ \theta_{t=max})=2</math></center>




<center><math> \theta_{max} \equiv \arccos 3</math></center>


<center><math>-cos\ \theta_{t=max}=1</math></center>


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°).  This implies for arccos 3, the range will include imaginary numbers.  Knowing that the range of the cosine function is -1 to +1 inclusive and the domain to be any angle




<center><math>x = \arccos{3}</math></center>
<center><math> \theta_{t=max} \equiv \arccos -1</math></center>




<center><math>cos(x) = \cos{\arccos{3}}</math></center>
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>\theta=180^{\circ}</math>


<center><math>\theta_{t=max}=180^{\circ}</math></center>


<center><math>\cos{x} = 3</math></center>


However, from the definition of s being invariant between frames of reference


From Euler's formula
<center><math>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></center>




<center><math>\cos{x} = \frac{e^{ix} + e^{-ix}}{2}</math></center>
In the center of mass frame of reference,


<center><math>E_1^*=E_2^*=E^* \quad and \quad \vec p \ _1^*=-\vec p \ _2^*= \vec p \ ^*</math></center>


<center><math> \frac{e^{ix} + e^{-ix}}{2} = 3</math></center>


<center><math>s \equiv 2m^2+2(E_1^{*2}+\vec p \ ^{*2} )</math></center>


<center><math> e^{ix} + e^{-ix} = 6</math></center>


Using the relativistic energy equation


Multiply with <math>e^{ix}</math>
<center><math>E^2 \equiv \vec p \ ^2+m^2</math></center>




<center><math>e^{2ix} + 1 = 6e^{ix}</math></center>
<center><math>s \equiv 2m^2+2((m^2+\vec p \ ^{*2})+\vec p \ ^{*2})</math></center>




<center>Letting <math>y = e^{ix}</math></center>
<center><math>s=4m^2+4 \vec p \ ^{*2})</math></center>




We get an quadratic equation:
<center><math>\frac{s-4m^2}{4}= \vec p \ ^{*2}</math></center>




<center><math>y^2 - 6y + 1 = 0</math></center>




<center><math>y = (6 ± √32)/2</math></center>
<center><math>t=-2 p \ ^{*2}(1-cos\ \theta)=\frac{-2(s-4m^2)}{4}(1-cos\ \theta)</math></center>




<center><math>y_1 = 5.828427 = e^{ix}</math></center>


<center><math>\frac{-2t}{s-4m^2}=(1-cos\ \theta)</math></center>




<center><math>y_2 = 0.171573 = e^{ix}</math></center>
<center><math>cos\ \theta=1-\frac{-2t}{s-4m^2}</math></center>






Apply ln on both sides gives the solution for arccos 3:
----




<center><math>x_1 = \frac{ln(5.828427) }{ i}=-1.76275i</math></center>


<center><math>\underline{\textbf{Navigation}}</math>


[[U-Channel|<math>\vartriangleleft </math>]]
[[VanWasshenova_Thesis#Moller_Scattering|<math>\triangle </math>]]
[[Limit_of_Energy_in_Lab_Frame|<math>\vartriangleright </math>]]


<center><math>x_2 = \frac{ln(0.171573) }{ i}=1.76275i</math></center>
</center>

Latest revision as of 19:07, 1 January 2019

[math]\displaystyle{ \underline{\textbf{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{ t=-2 p \ ^{*2}(1-cos\ \theta)=\frac{-2(s-4m^2)}{4}(1-cos\ \theta) }[/math]


[math]\displaystyle{ \frac{-2t}{s-4m^2}=(1-cos\ \theta) }[/math]


[math]\displaystyle{ cos\ \theta=1-\frac{-2t}{s-4m^2} }[/math]




[math]\displaystyle{ \underline{\textbf{Navigation}} }[/math]

[math]\displaystyle{ \vartriangleleft }[/math] [math]\displaystyle{ \triangle }[/math] [math]\displaystyle{ \vartriangleright }[/math]