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Fusion energy: Progress, partnerships, and the path to deployment
Over the past decade, fusion energy has moved decisively from scientific aspiration toward a credible pathway to a new energy technology. Thanks to long-term federal support, we have significantly advanced our fundamental understanding of plasma physics—the behavior of the superheated gases at the heart of fusion devices. This knowledge will enable the creation and control of fusion fuel under conditions required for future power plants. Our progress is exemplified by breakthroughs at the National Ignition Facility and the Joint European Torus.
Itacil C. Gomes, Donald L. Smith, Edward T. Cheng
Fusion Science and Technology | Volume 34 | Number 3 | November 1998 | Pages 706-713
Neutronics Experiments and Analysis | doi.org/10.13182/FST98-A11963697
Articles are hosted by Taylor and Francis Online.
Current designs of fusion-reactor systems seek to use radiation-resistant, low-activation materials that support long service lifetimes and minimize radioactive-waste problems after decommissioning. Reliable assessment of fusion materials performance requires accurate neutron-reaction cross sections and radioactive-decay constants. The problem areas usually involve cross sections since decay parameters tend to be better known. The present study was motivated by two specific questions: i) Why are the 51V(n,np)50Ti cross section values in the ENDF/B-VI library so large (a gas production issue)? ii) How well known are the cross sections associated with producing 7.4times105 y 26Al in silicon carbide by the process 28Si(n,np+d)27Al(n,2n)26Al (a long-lived radioactivity issue)? The energy range 14–15 MeV of the D-T fusion neutrons is emphasized. Cross-section error bars are needed so that uncertainties in the gas and radioactivity generated over the lifetime of a reactor can be estimated. We address this issue by comparing values obtained from prominent evaluated cross-section libraries. Small differences between independent evaluations indicate that a physical quantity is well known while the opposite signals a problem. Hydrogen from 51V(n,p)51Ti and helium from 51V(n,α)48Sc are also important sources of gas in vanadium, so they too were examined. We conclude that 51V(n,p)51Ti is adequately known but 51V(n,np+d)50Ti is not. The status for helium generation data is quite good. Due to recent experimental work, 27Al(n,2n)26Al seems to be fairly well known. However, the situation for 28Si(n,np+d)27Al remains unsatisfactory.