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Nuclear Energy Conference & Expo (NECX)
September 8–11, 2025
Atlanta, GA|Atlanta Marriott Marquis
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The Standards Committee is responsible for the development and maintenance of voluntary consensus standards that address the design, analysis, and operation of components, systems, and facilities related to the application of nuclear science and technology. Find out What’s New, check out the Standards Store, or Get Involved today!
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Powering the future: How the DOE is fueling nuclear fuel cycle research and development
As global interest in nuclear energy surges, the United States must remain at the forefront of research and development to ensure national energy security, advance nuclear technologies, and promote international cooperation on safety and nonproliferation. A crucial step in achieving this is analyzing how funding and resources are allocated to better understand how to direct future research and development. The Department of Energy has spearheaded this effort by funding hundreds of research projects across the country through the Nuclear Energy University Program (NEUP). This initiative has empowered dozens of universities to collaborate toward a nuclear-friendly future.
Yung-An Chao
Nuclear Science and Engineering | Volume 80 | Number 3 | March 1982 | Pages 476-480
Technical Note | doi.org/10.13182/NSE82-A19836
Articles are hosted by Taylor and Francis Online.
A space-time kinetic theory is proposed based on the recognition of a much shorter neutron spectral relaxation time than the spatial relaxation time. The neutron flux is factorized into a slowly varying energy-space-time-dependent spectral-shape function ψ(E, r, t) and a fast varying space-time-dependent local amplitude function A(r, t). The energy-independent self-adjoint diffusion equation that determines the local amplitude A(r, t) is defined as the space-time kinetic equation. This space-time kinetic equation is then solved by further decomposing A(r, t) into a relatively slowly varying space-time-dependent spatial-shape function R(r, t) and a fast varying time-dependent point amplitude T(t), which satisfies the point kinetic equation. The functions T(t), R(r, t), and ψ(E, r, t) are iteratively successively calculated, each one with a time increment step of a different order of magnitude. The fast varying delayed-neutron-precursor distribution functions are calculated together with T(t), however without complicating the point kinetic equation. Compared to the conventional approach, this proposed theory makes use less frequently of the multigroup diffusion equation, but more frequently the self-adjoint space-time kinetic equation. In this formulation, the instantaneous flux, not the adjoint flux, is the natural weighting function. This makes the space-time kinetic parameters deducible from monitored neutron spatial distribution data, and therefore the formulation a more appropriate basis for an inverse kinetic theory.