Difference between revisions of "Pair Production Rate Calculation"
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<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><br><br> | <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><br><br> | ||
− | ==Number of photons/sec out of 1/2 mil of Ti radiator== | + | ==Number of photons/sec out of Ti radiator== |
+ | |||
+ | ===1/2 mil of Ti=== | ||
+ | |||
+ | #<math>\sigma_{brems}=0.1\ \mbox{photons/electrons/MeV/r.l}</math> | ||
+ | #<math>\mbox{r.l.(Ti)} = 3.59\ \mbox{cm}</math> | ||
+ | #<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><br> | ||
+ | |||
+ | <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><br><br> | ||
+ | |||
+ | '''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><br><br> | ||
+ | |||
+ | |||
+ | ===1/2 mil of Al=== | ||
#<math>\sigma_{brems}=0.1\ \mbox{photons/electrons/MeV/r.l}</math> | #<math>\sigma_{brems}=0.1\ \mbox{photons/electrons/MeV/r.l}</math> |
Revision as of 23:48, 29 January 2011
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
Number of photons/sec out of Ti radiator
1/2 mil of Ti
Alex factor is 6.85 %
1/2 mil of Al
Alex factor is 6.85 %
Pair production rate
out of Al converter
(by varying width we can vary the yield)
through 1 m of air
Assume air consists entirely from Nitrogen:
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 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
Here I just plotted the table above for pair production cross section in (0, 40) MeV energy region