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Fusion Science and Technology
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A year in orbit: ISS deployment tests radiation detectors for future space missions
The predawn darkness on a cool Florida night was shattered by the ignition of nine Merlin engines on a SpaceX Falcon 9 rocket. The thrust of the engines shook the ground miles away. From a distance, the rocket appeared to slowly rise above the horizon. For the cargo onboard, the launch was anything but gentle, as the ignition of liquid oxygen generated more than 1.5 million pounds of force. After the rocket had been out of sight for several minutes, the booster dramatically returned to Earth with several sonic booms in a captivating show of engineering designed to make space travel less expensive and more sustainable.
Ruihuan Li, Bo Zhang, Dan Sun, Xiaoxiao Cao, Jijun Zhao
Fusion Science and Technology | Volume 80 | Number 2 | February 2024 | Pages 244-252
Research Article | doi.org/10.1080/15361055.2023.2223744
Articles are hosted by Taylor and Francis Online.
In order to characterize the behaviors of interstitial oxygen (O) in the vanadium (V) alloy, the interactions between O and Ti with respect to atomic separation distance have been investigated using first-principles calculations. We observe an attractive interaction between Ti and O within the third nearest neighbor (nn) (3nn) distance. The stability of the Ti-vacancy (Ti-Va) clusters has been studied by calculating the binding energy between Ti and monovacancy in the vanadium alloy, and our results show that the stable configurations are Ti1Va1, Ti2Va1, and Ti4Va1 clusters. The TinVa1 clusters prefer to trap two O atoms and form stable Ti1O2Va1, Ti2O2Va1, and Ti4O2Va1 clusters. Furthermore, the self-trapping energies of the Hex clusters by the TinO2Va1 clusters have been calculated. When four He atoms are trapped, the Hex clusters are stable. Furthermore, the trapping energies for the multiple He atoms captured by the TinO2Va1 clusters are calculated, and the TinO2 clusters are found to impede the vacancy trapping of He atoms to form He bubbles.