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Isotopes & Radiation
Members are devoted to applying nuclear science and engineering technologies involving isotopes, radiation applications, and associated equipment in scientific research, development, and industrial processes. Their interests lie primarily in education, industrial uses, biology, medicine, and health physics. Division committees include Analytical Applications of Isotopes and Radiation, Biology and Medicine, Radiation Applications, Radiation Sources and Detection, and Thermal Power Sources.
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2024 ANS Annual Conference
June 16–19, 2024
Las Vegas, NV|Mandalay Bay Resort and Casino
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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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Proving DRACO will deliver
The United States is now closer than it has been in over five decades to launching the first nuclear thermal rocket into space, thanks to DRACO—the Demonstration Rocket for Agile Cislunar Orbit.
T. C. Luu, J. L. Friar, A. C. Hayes
Nuclear Science and Engineering | Volume 152 | Number 1 | January 2006 | Pages 98-105
Technical Paper | doi.org/10.13182/NSE06-A2567
Articles are hosted by Taylor and Francis Online.
In high neutron flux environments where isomers can be strongly populated by nucleonic reactions, isotope abundances from reaction network chains can be affected by the population of nuclear isomers. At high temperatures and densities, there is the additional possibility of populating these isomers electromagnetically. Here, we examine the rates for electromagnetic excitation of the isotopes of several isomers of interest both in astrophysics and applied physics (e.g., 235U, 193Ir, and 87,88Y). We consider six possible electromagnetic processes, namely, photoabsorption, inverse internal conversion, inelastic electron scattering, coulomb excitation, and (,') and (e,e') reactions. We find that for plasma temperatures kT ~ 1 to 10 keV, the electromagnetic reactions rates are negligible. Thus, we conclude that reaction network calculations do not need to include the possibility of electromagnetically exciting nuclear isomers. This is true in both stellar and terrestrial thermonuclear explosions, as well as in plasma conditions expected at the National Ignition Facility.