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首页> 外文期刊>Journal of chemical theory and computation: JCTC >Reparameterization of RNA χ Torsion Parameters for the AMBER Force Field and Comparison to NMR Spectra for Cytidine and Uridine
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Reparameterization of RNA χ Torsion Parameters for the AMBER Force Field and Comparison to NMR Spectra for Cytidine and Uridine

机译:用于AMBER力场的RNAχ扭转参数的重新参数化和胞苷和尿苷的NMR光谱比较

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摘要

A reparameterization of the torsional parameters for the glycosidic dihedral angle, χ, for the AMBER99 force field in RNA nucleosides is used to provide a modified force field, AMBER99_χ. Molecular dynamics simulations of cytidine, uridine, adenosine, and guanosine in aqueous solution using the AMBER99 and AMBER99_χ force fields are compared with NMR results. For each nucleoside and force field, 10 individual molecular dynamics simulations of 30 ns each were run. For cytidine with AMBER99_χ force field, each molecular dynamics simulation time was extended to 120 ns for convergence purposes. Nuclear magnetic resonance (NMR) spectroscopy, including one-dimensional (1D) ~1H, steady-state 1D ~1H nuclear Overhauser effect (NOE), and transient 1D ~1H NOE, was used to determine the sugar puckering and preferred base orientation with respect to the ribose of cytidine and uridine. The AMBER99 force field overestimates the population of syn conformations of the base orientation and of C2'-endo sugar puckering of the pyrimidines, while the AMBER99_χ force field's predictions are more consistent with NMR results. Moreover, the AMBER99 force field prefers high anti conformations with glycosidic dihedral angles around 310° for the base orientation of purines. The AMBER99_χ force field prefers anti conformations around 185°, which is more consistent with the quantum mechanical calculations and known 3D structures of folded ribonucleic acids (RNAs). Evidently, the AMBER99_χ force field predicts the structural characteristics of ribonucleosides better than the AMBER99 force field and should improve structural and thermodynamic predictions of RNA structures.
机译:RNA核苷中AMBER99力场的糖苷二面角χ扭转参数的重新参数化用于提供修改后的力场AMBER99_χ。将使用AMBER99和AMBER99_χ力场的水溶液中胞苷,尿苷,腺苷和鸟苷的分子动力学模拟与NMR结果进行了比较。对于每个核苷和力场,进行了10个单独的分子动力学模拟,每个模拟都为30 ns。对于具有AMBER99_χ力场的胞苷,出于收敛目的,每个分子动力学模拟时间都延长至120 ns。核磁共振(NMR)光谱包括一维(1D)〜1H,稳态1D〜1H核Overhauser效应(NOE)和瞬态1D〜1H NOE,用于确定糖的起皱和优选的碱基取向关于胞苷和尿苷的核糖。 AMBER99力场高估了嘧啶的碱基方向和C2'-内糖褶皱的顺式构象,而AMBER99_χ力场的预测与NMR结果更一致。此外,对于嘌呤的基本取向,AMBER99力场更喜欢糖基二面角约为310°的高反构象。 AMBER99_χ力场偏爱185°附近的反构象,这与量子力学计算和折叠核糖核酸(RNA)的已知3D结构更加一致。显然,AMBER99_χ力场比AMBER99力场更好地预测了核糖核苷的结构特征,并应改善RNA结构的结构和热力学预测。

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