Difference between revisions of "Neutron Polarimeter"
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==low energy approximation== | ==low energy approximation== | ||
− | As we can see from Fig.2 for low energy neutrons (0- | + | As we can see from Fig.2 for low energy neutrons (0-21 MeV)<br> |
energy dependence of incident photons is linear | energy dependence of incident photons is linear | ||
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<math> T_{\gamma}(T_n) | <math> T_{\gamma}(T_n) | ||
− | = \frac{T_{\gamma}(21\ MeV) - T_{\gamma}(0\ MeV)}{21\ MeV - 0\ MeV}\ T_n + T_{\gamma}(0\ MeV) | + | = \frac{T_{\gamma}(21\ MeV) - T_{\gamma}(0\ MeV)}{21\ MeV - 0\ MeV}\ T_n + T_{\gamma}(0\ MeV) </math> |
− | + | ||
+ | Finally for low energy neutrons (0-21 MeV):<br> | ||
+ | <math> T_{\gamma}(T_n) = 2.051\ T_n + 1.715 </math> | ||
[http://wiki.iac.isu.edu/index.php/PhotoFission_with_Polarized_Photons_from_HRRL Go Back] | [http://wiki.iac.isu.edu/index.php/PhotoFission_with_Polarized_Photons_from_HRRL Go Back] |
Revision as of 03:16, 7 June 2010
Analysis of energy dependence
four-vectors algebra
writing four-vectors:
Doing four-vector algebra:
Detector is located at
, so
and visa versa
plots
low energy approximation
As we can see from Fig.2 for low energy neutrons (0-21 MeV)
energy dependence of incident photons is linear
Find that dependence. We have:
So, the equation of the line is:
Finally for low energy neutrons (0-21 MeV):