Difference between revisions of "Pair Production Rate Calculation"

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====bremsstrahlung for Ti====
 
====bremsstrahlung for Ti====
  
[[File:bremss44MeV.png | 400 px]
+
[[File:bremss44MeV.png]
  
 
in (10,20) MeV region we have about '''0.1 photons/electrons/MeV/r.l'''
 
in (10,20) MeV region we have about '''0.1 photons/electrons/MeV/r.l'''
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====bremsstrahlung for Al====
 
====bremsstrahlung for Al====
  
[[File:Aluminum-44MeV.png | 400 px]]
+
[[File:Aluminum-44MeV.png | 600 px]]
  
 
in (10,20) MeV region we have about '''0.1 photons/electrons/MeV/r.l'''
 
in (10,20) MeV region we have about '''0.1 photons/electrons/MeV/r.l'''

Revision as of 04:36, 2 February 2011

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LINAC parameters used in calculations

1) pulse width 50 ps
2) pulse current 50 A
3) repetition rate 300 Hz
4) energy 44 MeV

Number of electrons/sec on radiator

[math] 50\ \frac{C}{sec} \times \frac{1\cdot e^-}{1.6\cdot 10^{-19}\ C} \times 50\ \mbox{ps} \times 300\ \mbox{Hz} = 0.47 \cdot 10^{13}\ \frac{e^-}{sec}[/math]

Number of photons/sec out of radiator

1/2 mil of Ti

  1. [math]\sigma_{brems}=0.1\ \mbox{photons/electrons/MeV/r.l}[/math]
  2. [math]\mbox{r.l.(Ti)} = 3.59\ \mbox{cm}[/math]
  3. [math]\mbox{radiator}\ \mbox{thickness} = 12.5\ \mu m[/math]


[math]\frac{12.5\ \mu m}{3.59\ cm} = 3.48 \cdot 10^{-4}\ r.l.[/math]
[math]0.47 \cdot 10^{13}\ \frac{e^-}{sec} \times 0.1\ \frac{\gamma 's}{(e^- \cdot MeV \cdot r.l.)} \times 3.48 \cdot 10^{-4}\ r.l. \times 10\ MeV =1.63 \cdot 10^{9} \frac{\gamma}{sec}[/math]

Alex factor is 6.85 %

[math]1.63 \cdot 10^{9} \frac{\gamma}{sec} \cdot 6.85\ % = 1.12 \cdot 10^{8} \frac{\gamma}{sec}[/math]

1/2 mil of Al

  1. [math]\sigma_{brems}=xxx\ \mbox{photons/electrons/MeV/r.l}[/math]
  2. [math]\mbox{r.l.(Al)} = 8.89\ \mbox{cm}[/math]
  3. [math]\mbox{radiator}\ \mbox{thickness} = 12.5\ \mu m[/math]


[math]\frac{12.5\ \mu m}{8.89\ cm} = 1.41 \cdot 10^{-4}\ r.l.[/math]
[math]0.47 \cdot 10^{13}\ \frac{e^-}{sec} \times xxx\ \frac{\gamma 's}{(e^- \cdot MeV \cdot r.l.)} \times 1.41 \cdot 10^{-4}\ r.l. \times 10\ MeV =xxx \cdot 10^{9} \frac{\gamma}{sec}[/math]

Alex factor is 6.85 %

[math]xxx \cdot 10^{9} \frac{\gamma}{sec} \cdot 6.85\ % = xxx \cdot 10^{8} \frac{\gamma}{sec}[/math]

Conversion factor from Ti to Al

All my following calculation for pair production rate are based on (1/2) mil of Ti radiator. If we want to recalculate for (1/2) mil of Al converter we need to use the conversion factor:

[math]\frac{aaa}{1.12} = ddd [/math]

Appendix

bremsstrahlung for Ti

[[File:bremss44MeV.png]

in (10,20) MeV region we have about 0.1 photons/electrons/MeV/r.l

bremsstrahlung for Al

Aluminum-44MeV.png

in (10,20) MeV region we have about 0.1 photons/electrons/MeV/r.l

Pair production rate

out of Al converter

[math]\sigma_{pairs} = 0.5\ \frac{\mbox{barns}}{\mbox{atom}}[/math]
[math]l = 3.0\ \mu m[/math] (by varying width we can vary the yield)
[math]N_{Al} = \frac{2.70\ \frac{g}{cm^3} \times 6.02 \cdot 10^{23}\ \frac{atoms}{mol} \times 3.0\ \mu m} {26.98\ \frac{g}{mol}} = 1.81 \cdot 10^{23}\ \frac{\mbox{atoms}}{m^2}[/math]
[math]\frac {1.12 \cdot 10^{8}\ \frac{\gamma}{sec} \times \sigma_{pairs} \times N_{Al}} {f} = 3.38\ \frac{\mbox{pairs}}{\mbox{pulse}} [/math]

through 1 m of air

Assume air consists entirely from Nitrogen:

[math]\sigma_{pairs}\ (\mbox{Nitrogen}) = 0.15\ \frac{\mbox{barns}}{\mbox{atom}}[/math] 
[math]l = 1.0\ \mbox{m}[/math]
[math]N_{\mbox{Nitrogen}} = \frac{0.00125\ \frac{g}{cm^3} \times 6.02 \cdot 10^{23}\ \frac{atoms}{mol} \times 1.0\ \mbox{m}} {14.01\ \frac{g}{mol}} = 5.37 \cdot 10^{25}\ \frac{\mbox{atoms}}{m^2}[/math]
[math]\frac {1.12 \cdot 10^{8}\ \frac{\gamma}{sec} \times \sigma_{\mbox{pairs}} \times N_{\mbox{Nitrogen}}} {f} = 300\ \frac{\mbox{pairs}}{\mbox{pulse}} [/math]

Appendix

pair production cross sections in an Al target

Ref. Geant4 and Theoretical Pair Production Cross Sections for 1 MeV - 100 GeV photons in Aluminum. Vakho Makarashvili, December 18, 2007


Pair production Al.png

pair production cross sections in a Nitrogen

Ref. Photon Cross Section, Attenuation Coefficients, and Energy Absorption Coefficients From 10 keV to 100 Gev. J.H.Hubbell. Center for Radiation Research.National Bureau of Standards. Washington, D.C. 20234

Pair prodiction nitrogen.png


Here I just plotted the table above for pair production cross section in (0, 40) MeV energy region


Sigma nitrogen fitted m2.png



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