Test of local realism via entangled $$\Lambda \bar{\Lambda }$$ system
Not provided.
Engineering topics
Publications and source records attributed to Fu, J..
Not provided.
Not provided.
The interpretation of cosmic spectra relies on a vast sea of atomic data which are not readily obtainable from analytic expressions or simple calculations. Rather, their evaluation typically requires state-of-the-art atomic physics calculations, with the inclusion of weaker effects (spin-orbit and configuration interactions, relaxation, Auger broadening, etc.), to achieve the level of accuracy needed for use by astrophysicists. Our NASA-supported research program is focused on calculating data for three important atomic processes, 1) dielectronic recombination (DR), 2) inner-shell photoabsorption, and 3) fluorescence and Auger decay of inner-shell vacancy states. Some additional details and examples of our recent findings are given.
This work suggests that the hot dwell duration for each test should be determined in two steps: a minimum hot duration of 80 hours be required and then followed by specific tailoring be conducted to arrive at the proper test duration.