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Numerical simulations verify the analytically predicted energy variations.
The measured energy variations are connected with a drift shell oscillations in the longitude direction.
Second, entropic effects are weighted by energetic effects (internal energy variations) during the deformation.
Resolving powers of 7000 and 16 100 have been achieved with kinetic energy variations of 34 and 10.5%, respectively.
EPID1 was significantly more sensitive to dose and energy variations and would require separate calibration data for EPID dosimetry.
We find that the S1 and S2 site orbital energy variations define the boarder lines of the most probable closed-shell orbital energy of Ni acting as Ni0 state under the thermodynamic equilibrium adsorption state.
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Thermodynamically consistent forces are derived by energy variation.
We further extend the computational efforts on the Ni-3d orbital energy variation with related to the change of Ni C bond length (Fig. 4f).
On the other hand, if the energy variation is decreasing, then it is primary.
Additionally, the phase energy variation is reduced by 18%, which benefits circulating current control.
Applying the principle of minimum potential energy and the energy variation approach, we derive the governing equations and boundary conditions.
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