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Next the normal modes are calculated and simulated.
Electronic structures and vibrational modes are calculated employing DFT.
The exergy efficiencies and the exergy destructions in the cooling and heating modes are calculated.
Normal modes are calculated to validate the existence of optimal cluster structures.
The residuals of inter prediction modes are calculated by performing a motion estimation.
The non-rotating modes are calculated by using a finite element cyclic symmetry approach.
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The activation energies of failure modes were calculated.
The umbrella modes were calculated in the range 1373 1367 cm−1373 1367
For As2S1+4/2 cluster, LF Raman active modes were calculated at 31.7, 43.1 and 58.8 cm−1.
The sound velocities of QLA and quasi-TA modes were calculated in [9].
The critical loading required to make this transition from long to short wavelength buckling modes is calculated.
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