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Fig. 1b demonstrates an example of the energy spectrum for the considered dependent mass profile.
Fig. 2 presents the considered mass profile which has a maximum value at ({sf{r}}=0).
For a specific position-dependent mass profile, the bound state solutions are obtained through an analytical form.
It is further pointed out that, at the mass profile discontinuities, the commonly accepted interface conditions for the Bastard Hamiltonian are not natural conditions.
For example, if simulating a star cluster of known mass profile M ( r ) and centre x 0, one may simply use a b ∼ G M ( r b ) r b − 2 with r b = | x b − x 0 |.
According to Fig. 1b, the energy spectrum for the considered mass profile is not so sensitive to the quantum number n, science the diagrams for (n=0) and (n=7) are not so different and are very close together.
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Her friend Damien Goodmon, another local activist, saw the whole thing as a conditioned response, akin to mass profiling.
Charge and mass profiles were determined.
Figure 5 shows the mass profiles over the study period.
The temperature, pressure and adsorbed mass profiles in the two adsorbers have been shown.
We derive the mass profiles without the assumption of analytical models.
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