Difference between revisions of "Notes from July 2nd, 2008 Meeting"
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<math>10^{-3} \frac{\frac{\gamma 's}{MeV}}{\frac{e^{-}}{radiation lengths}} \times 2 \cdot 10^{-4} radiation lengths \times 15 MeV \times 9.4 \cdot 10^{12} \frac{e^{-}}{sec}=2.8 \cdot 10^{7} \frac{\gamma}{sec}</math> | <math>10^{-3} \frac{\frac{\gamma 's}{MeV}}{\frac{e^{-}}{radiation lengths}} \times 2 \cdot 10^{-4} radiation lengths \times 15 MeV \times 9.4 \cdot 10^{12} \frac{e^{-}}{sec}=2.8 \cdot 10^{7} \frac{\gamma}{sec}</math> | ||
+ | |||
+ | ==Number of ɣ + d -> n + p events/sec== | ||
+ | |||
+ | <math>2.8 \cdot 10^{7} \frac{\gamma}{sec} \times 4 \cdot 10^{-4} = 10^{4}</math> | ||
+ | |||
+ | ==Probability of Photodisintegration Event== | ||
+ | |||
+ | target thickness in <math>\frac{Dnuclei}{cm^{2}} \times \sigma in cm^{2}</math> |
Revision as of 13:28, 3 July 2008
Numbers for rate of Brems intensity spectrum:
=
Number of ɣ + d -> n + p events/sec
Probability of Photodisintegration Event
target thickness in