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

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Summary

METHODS

Received: 10 January 2015 / Accepted: 16 February 2015 / Published online: 9 July 2015

INTRODUCTION
Findings
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