Abstract
Despite the success of RNA secondary structure prediction for simple, short RNAs, the problem of predicting RNAs with long-range tertiary folds remains. Furthermore, RNA 3D structure prediction is hampered by the lack of the knowledge about the tertiary contacts and their thermodynamic parameters. Low-resolution structural modeling enables us to estimate the conformational entropies for a number of tertiary folds through rigorous statistical mechanical calculations. The models lead to 3D tertiary folds at coarse-grained level. The coarse-grained structures serve as the initial structures for all-atom molecular dynamics refinement to build the final all-atom 3D structures. In this paper, we present an overview of RNA computational models for secondary and tertiary structures’ predictions and then focus on a recently developed RNA statistical mechanical model—the Vfold model. The main emphasis is placed on the physics behind the models, including the treatment of the non-canonical interactions in secondary and tertiary structure modelings, and the correlations to RNA functions.
Highlights
The increasing discoveries of noncoding RNAs demand more than ever the information about RNA structure (Bachellerie et al 2002; Kertesz et al 2007; He et al 2008; Bartel 2009; Gong and Maquat 2011; Wang et al 2013)
For a physics-based approach, accurate evaluation of the energetic parameters for tertiary interactions is critical for 3D structure prediction
The primary focus of this article is on the statistical mechanics-based methods for predicting RNA 3D structures and folding energy landscapes, and the related quantitative insights into RNA functions
Summary
Received: 10 January 2015 / Accepted: 16 February 2015 / Published online: 9 July 2015
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