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Interestingly, no changes were seen in the interaction of the surrounding olfactory genes (MOR5B1-3 and MOR3B1-4 [33]), or the expression level of the β-globin genes.
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According to the crystal structure, the T122K exchange can be expected to result in changes in the conformations and interactions of the surrounding residues.
While dynamics are available from MD, it can be quite challenging to accurately capture the strong polarization and other chemical interactions of the surrounding water molecules near complex transition-metal oxide surfaces [27, 32] using parameterized force fields.
In our study we focused on a computational investigation of the hydrolytic mechanism of human RNase HI (PDB Code 2QKK) [1] using a comprehensive QM/MM theoretical method that is based on DFT/B3LYP calculation of the interactions in the QM region and the inclusion of the interactions of the surrounding protein and solvent water in the MM region as implemented in the software package of NWChem [2].
Thus, the ICR affects the allele-specific interactions of the surrounding CTCF sites at the locus.
In contrast, the conformational reorganization that occurs during the microsecond to millisecond lifetimes of side chain ionizations commonly yields effective internal dielectric values near 20 (32, 32), implying roughly a 6−7-fold lower sensitivity to the electrostatic interactions of the surrounding protein structure than that observed for the peptide ionizations.
A polaron behaves as a negatively charged particle with a mass greater than that of an isolated electron because of its interaction with the surrounding atoms of the solid.
The decreased relaxivity could be caused by some loss of interaction between the surrounding water due to the absorption of IO-MHPC to the PCPP nanospheres.
The only - and crucial - approximation has to be made for the many-body interaction of the electrons surrounding the atomic nuclei which is done in the framework of density functional theory.
As above, the introduction of the two proper motions and relative to the neighboring stars could explain the duality of the motion of the HMS in space and prove also the absence of the C-G effect of CRs at low energies due to the motion of the HMS by the interaction of the SuHMS surrounding the HMS.
The radiation emitted by pulsars is caused by interaction of the plasma surrounding the neutron star with its rapidly rotating magnetic field.
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