Reactor coolant 2026-10-20
A material carrying heat from a reactor core. heat capacity, transport properties, chemical compatibility, neutron interactions and stability must be considered together.
Using the orbital order after 28 supplied in the simple shell model, proton counts 32 and 38 fill and , so the odd 39th proton occupies . With paired valence neutrons this gives a yttrium-91 ground-state prediction. The daughter has paired 40 protons and one neutron beyond the 50-neutron closure in , giving . The inferred ground-state beta transition is therefore first-forbidden unique. This is a stated paired-shell model deduction; an endpoint diagram alone does not determine the spin assignment or an evaluated isotope mass.
Single-particle nuclear magnetic moment Created 2026-10-18 Updated 2026-10-20
In the simplest nuclear shell model of an odd-mass number nucleus, paired nucleons contribute zero total angular momentum and magnetic dipole moment. The last unpaired nucleon supplies the nuclear spin and the stretched-state moment , where is the Landé g-factor and the nuclear magneton.
Using addition of angular momentum with gives
For , this reduces to . For , it gives
The free-nucleon orbital factors are for a proton and for a neutron. Residual nuclear interactions and configuration mixing can shift measured moments away from this ideal prediction. A single hole in an otherwise closed shell has the same stretched-state moment as a particle in that shell: removing the particle leaves total and moment .
Slow neutron 2026-10-18
A slow neutron has low kinetic energy relative to the fast neutrons commonly emitted in nuclear reactions. The term covers an energy range, rather than a single speed. A neutron moderator transfers kinetic energy to surrounding matter through collisions. Slowing a neutron can increase its chance of causing particular neutron capture reactions, even though each collision has reduced its kinetic energy. The Fermi slow-neutron activation experiment made this surprising distinction experimentally visible.
SNO solar-neutrino flavor experiment Created 2026-10-18 Updated 2026-10-20
In 2001, live days, reconstructed radius below and effective electron kinetic energy above gave a CC neutrino flux of for the assumed boron-8 spectrum. Source calibrations measured instrumental-cut signal loss. SNO's own CC–ES difference was ; comparison with Super-Kamiokande's precise ES flux gave evidence for non-electron active neutrinos. This was not an NC measurement.[ref]
In 2002 the pure-heavy water analysis used live days and a reconstructed kinetic-energy threshold. NC neutrons captured on deuterons emitted gamma rays, producing secondary electron light. The NC reaction threshold was , a different quantity. Californium-252 calibrated capture efficiency, but only detection efficiency after fiducial and energy cuts. Assays constrained backgrounds from radioactive decay and photodisintegration.[ref]
Energy, radius and direction relative to the Sun statistically separated channels. Assuming the standard boron-8 spectral shape, the NC total active neutrino flux was , consistent with stellar structure predictions. The non-electron active component differed from zero by . This established active flavour conversion, without individually tagging muon neutrinos and tau neutrinos. It did not exclude every sterile admixture.[ref]
For in a sphere of radius , with zero surface density and regularity at the origin, the lowest spherically symmetric normal mode is . Substitution of in the radial Laplacian gives , and regularity removes the cosine solution. The Dirichlet boundary condition gives ; a radial mode with no interior zeros requires . Thus diffusion leakage suppresses growth below the displayed threshold, while the mode is stationary at equality. The expression at uses its continuous limit. In a linear neutron multiplication model this is the competition between bulk production and surface loss.
For a nearly massless incident tau neutrino and stationary target of mass , the initial Mandelstam variables give . At threshold the final tau lepton and the lightest allowed recoil system have no relative momentum, so . This proves the formula. A free neutron recoil channel gives approximately ; an electron target has a different recoil and a threshold near .
Thermal neutron 2026-10-18
A thermal neutron belongs to a population approximately in thermal equilibrium with its surroundings. Such a population has a distribution of kinetic energies, not one fixed energy. The scale uses the Boltzmann constant and thermodynamic temperature; it is about at . The mean translational kinetic energy for a classical three-dimensional equilibrium population is . Not every slow neutron has reached this equilibrium.
With only up/down valence quarks and no antiquarks, the quark number sum rule and leading parton model expression give the charge-squared number moment . The squared charges are for up and for down, so the proton has and the neutron has . Restricting the flavour list to up/down does not itself remove antiquarks; the no-sea assumption is essential for these individual moments.
Zirconium alloy 2026-10-20
An alloy based on zirconium. Low neutron absorption and corrosion behaviour motivate nuclear fuel cladding applications; irradiation growth, creep and hydrogen uptake remain constraints.