Difference between revisions of "Theoretical analysis of 2n accidentals rates"
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[[Production Analysis | go_back]] | [[Production Analysis | go_back]] | ||
==Introduction== | ==Introduction== | ||
| − | Every individual pulse of photons may cause any number of neutron-producing reactions, hereafter denoted by <math>n</math>, ranging form zero to "infinity". <math>n</math>, being the number of neutron-producing reactions ''actually'' occurring per pulse, is assumed to follow the Poissonian distribution as a limiting case of the binomial distribution. Each neutron-producing interaction produces <math>v_{i}</math> neutrons, where <math>v_{i}</math> is the distribution of the number of neutrons produced from a single given neutron-producing reaction. For our purposes, <math> | + | Every individual pulse of photons may cause any number of neutron-producing reactions, hereafter denoted by <math>n</math>, ranging form zero to "infinity". <math>n</math>, being the number of neutron-producing reactions ''actually'' occurring per pulse, is assumed to follow the Poissonian distribution as a limiting case of the binomial distribution. Each neutron-producing interaction produces <math>v_{i}</math> neutrons, where <math>v_{i}</math> is the distribution of the number of neutrons produced from a single given neutron-producing reaction. For our purposes, <math>v_{i}</math> is a combination of the 1n-knockout cross-section and the photo-fission multiplicity distribution. |
Revision as of 02:37, 9 January 2018
Introduction
Every individual pulse of photons may cause any number of neutron-producing reactions, hereafter denoted by , ranging form zero to "infinity". , being the number of neutron-producing reactions actually occurring per pulse, is assumed to follow the Poissonian distribution as a limiting case of the binomial distribution. Each neutron-producing interaction produces neutrons, where is the distribution of the number of neutrons produced from a single given neutron-producing reaction. For our purposes, is a combination of the 1n-knockout cross-section and the photo-fission multiplicity distribution.