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At present, models predicting shell multistability are often characterised by a compromise between computational efficiency and result accuracy.
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In the 1960s, the shell effect was introduced in the macroscopic model (macroscopic microscopic model), predicting a strong nuclear shell effect at Z = 114 and N = 184 (refs. 6,17).
Previous energy-based models predict that multiple "tunnel" cracks in the weak layers of the shell account for a factor of 20 of this increase in fracture energy.
Other models predict no effects.
Models predict trends in climate, not particular events.
In terms of damage volume the PFA-TWB models predicts slightly higher values which can be traced back to the inevitable differences in the failure criteria formulation in the one-dimensional and the shell model, respectively.
Models predict the trend will continue.
Previous models predicted too many gas giants.
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This is simply what the models predicted would happen.
But maybe it will happen faster than the models predict.
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