Difference between revisions of "Notes for the July 11th, 2008 Meeting"
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<math>2 \cdot \sqrt{p_n ^2 + m _n ^2} = 15 MeV = m _d | <math>2 \cdot \sqrt{p_n ^2 + m _n ^2} = 15 MeV = m _d | ||
</math> | </math> | ||
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+ | <math>p _n = [\frac{15 MeV + m _d}{2}]^{2} - m _n ^{2}</math> | ||
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+ | <math>p _n = [\frac{15 + 1875.6}{2}]^{2} - 939.6 ^{2} = 104 MeV</math> | ||
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+ | KE = 5.3 MeV | ||
+ | |||
+ | β = .1 | ||
+ | |||
+ | θ = 85.6° -> Means that since they're moving forward, the angles will be pushed forward to be less than 90°. | ||
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+ | KE <sub>n</sub> <sup>fission</sup> = 1 MeV -> fission neutrons | ||
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+ | V = .05c | ||
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+ | -> 25 nsec/ft | ||
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+ | |||
+ | Beam pulse [[Image:stuff_for_july_11th.jpg]] | ||
+ | |||
+ | [http://wiki.iac.isu.edu/index.php/PhotoFission_with_Polarized_Photons_from_HRRL Go Back] |
Latest revision as of 06:26, 5 February 2009
= we'll have 2.5"
= tan(1.95)
radiator distance - collimator
x = 73.4" = 186.5 cm
radiator is 73.4" - 48" upstream of the wall
Something someone needs to do:
Look up which has the highest neutron production energy thresh hold: Cu, Zn, Ni
KE = 5.3 MeV
β = .1
θ = 85.6° -> Means that since they're moving forward, the angles will be pushed forward to be less than 90°.
KE n fission = 1 MeV -> fission neutrons
V = .05c
-> 25 nsec/ft