Space and energy dependent theoretical formula for the third order neutron correlation technique

Bell, 1970

Dragt, 1967, Threefold correlations and third order moments in reactor noise, Nukleonik, 10, 7

Endo, T., Kitamura, Y., Yamane, Y., 2003. Absolute measurement of the subcriticality based on the third order neutron correlation in consideration of the finite nature of the neutron counts data. ICNC2003, Tokai, Ibaraki, Japan, October 20–24.

Feynman, 1956, Dispersion of the neutron emission in U-235 fission, J. Nucl. Energ., 3, 64

Furuhashi, 1968, Third moment of the number of neutrons detected in short time intervals, J. Nucl. Sci. Technol., 5, 48, 10.3327/jnst.5.48

Gwin, 1984, Measurements of the energy dependence of prompt neutron emission from 233U, 235U, 239Pu, and 241Pu for En=0.005 to 10eV relative to emission from spontaneous fission of 252Cf, Nucl. Sci. Eng., 87, 381, 10.13182/NSE84-A18506

Kitamura, Y., Endo, T., Yamane, Y., Misawa, T., Unesaki, H., 2002. Absolute measurement of the subcriticality by using the third order moment of the number of neutrons detected. PHYSOR 2002, Seoul, Korea, October 7–10.

Mihalczo, 1978, Determination of reactivity from power spectral density measurements with californium-252, Nucl. Sci. Eng., 66, 29, 10.13182/NSE78-A15186

Misawa, 1990, Measurement of prompt neutron decay constant and large subcriticality by the Feynman-α method, Nucl. Sci. Eng., 104, 53, 10.13182/NSE104-53

Otsuka, 1965, Space-dependent formula for Rossi-α measurements, Nukleonik, 7, 488

Otsuka, 1965, Space-time correlation in neutron distributions in a multiplying medium, J. Nucl. Sci. Technol., 2, 191, 10.3327/jnst.2.191

Pázsit, 1998, The variance-to-mean ratio in subcritical systems driven by a spallation source, Ann. Nucl. Energ., 25, 667, 10.1016/S0306-4549(97)00117-5

Simmons, 1958, A pulsed neutron technique for reactivity determination, Nucl. Sci. Eng., 3, 595, 10.13182/NSE3-595-608

Sjöstrand, 1956, Measurements on a subcritical reactor using a pulsed neutron source, Arkiv för Fysik, 11, 233