Difference between revisions of "Photofission neutron rate"
Jump to navigation
Jump to search
| Line 5: | Line 5: | ||
<math>N_{1n}\propto \int \sigma_{1n}(E_{\gamma})\epsilon_{1n}(E_{\gamma})*\gamma(E_{\gamma})dE_{\gamma} </math> | <math>N_{1n}\propto \int \sigma_{1n}(E_{\gamma})\epsilon_{1n}(E_{\gamma})*\gamma(E_{\gamma})dE_{\gamma} </math> | ||
| − | <math>N_{fiss}\propto \int \sigma_{fiss}(E_{\gamma})\epsilon_{fiss} | + | <math>N_{fiss}\propto \int \sigma_{fiss}(E_{\gamma})\epsilon_{fiss}*\gamma(E_{\gamma})dE_{\gamma} </math> |
[[File:(G,1n).png|450px]] [[File:FractionAbove0.5MeV.png|420px]] | [[File:(G,1n).png|450px]] [[File:FractionAbove0.5MeV.png|420px]] | ||
Revision as of 01:53, 20 December 2016
Overview
The goal of this calculation is to determine the portion of detected neutron singles that originate from photofission in a Th-232 target, as opposed to neutrons from gamma, 1n knockout. MCNP is used to determine the bremsstrahlung energy spectrum entering the experimental cell. This calculation cannot be done entirely in MCNP6 since it is missing cross section tables for Th-232 photofission. The neutron detectors are assumed to have 100% efficiency for neutrons above 0.5 MeV ,and 0% below 0.5 MeV.
calculation
.png)
