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COMPUTATIONAL STUDIES OF TTR RELATED AMYLOIDOSIS: EXPLORATION OF CONFORMATIONAL SPACE THROUGH PETRI NET-BASED ALGORITHM

Abstract

Amyloidosis, a serious and widespread disease with a genetic background, manifests itself through the formation of dangerous fibrils in various organs. Apart from the polluted environment and an unhealthy lifestyle, genetic factors may accelerate this process leading in some cases to lethal damages to the body. Recently, a growing interest in amyloidogenic protein research has been observed. Transthyretin (TTR) is a tetrameric protein that transports thyroid hormone thyroxine and retinol binding protein in plasma and the cerebral fluid. Sometimes TTR breaks apart and forms fibrils. Several single point mutations, having destabilizing impact on the TTR complex, are involved in the amyloidogenic TTR cascade. Problems with the TTR tetramer stability and conformational space characteristics of the protein have not been addressed computationally before. We present selected results of our molecular dynamics (MD, ∼2 000 ns) and steered MD simulations (SMD) of three variants of TTR: Wild Type (WT), V30M and L55P. SMD has been used to enforce the dissociation of TTR. Conformational spaces of WT TTR and its amyloidogenic variants have been investigated using a novel “One Place One Conformation” (OPOC) algorithm based on a graph technique called Petri net (PN) formalism. While the PN approach alone does not permit a direct identification of protein regions with reduced stability, it gives quite a useful tool for an effective comparison of complex protein energy landscapes explored during classical and/or SMD steered molecular dynamics simulations.

Keywords:

transthyretin, amyloidosis, molecular dynamics, Petri nets, clustering, conformational space, graphs

Details

Issue
Vol. 18 No. 3 (2014)
Section
Research article
Published
2014-09-30
DOI:
https://doi.org/10.17466/TQ2014/18.3/J
Licencja:
Creative Commons License

This work is licensed under a Creative Commons Attribution 4.0 International License.

Author Biographies

RAFAL JAKUBOWSKI,
Nicolaus Copernicus University, Faculty of Physics, Astronomy and Informatics, Institute of Physics



ANNA GOGOLINSKA,
Nicolaus Copernicus University, Institute of Physics, Faculty of Physics, Astronomy and Informatics, Faculty of Mathematics and Computer Science



LUKASZ PEPLOWSKI,
Nicolaus Copernicus University, Institute of Physics, Faculty of Physics, Astronomy and Informatics



PIOTR SKRZYNIARZ,
Nicolaus Copernicus University, Institute of Physics, Faculty of Physics, Astronomy and Informatics



WIESLAW NOWAK,
Nicolaus Copernicus University, Institute of Physics, Faculty of Physics, Astronomy and Informatics



Authors

  • RAFAL JAKUBOWSKI

    Nicolaus Copernicus University, Faculty of Physics, Astronomy and Informatics, Institute of Physics
  • ANNA GOGOLINSKA

    Nicolaus Copernicus University, Institute of Physics, Faculty of Physics, Astronomy and Informatics, Faculty of Mathematics and Computer Science
  • LUKASZ PEPLOWSKI

    Nicolaus Copernicus University, Institute of Physics, Faculty of Physics, Astronomy and Informatics
  • PIOTR SKRZYNIARZ

    Nicolaus Copernicus University, Institute of Physics, Faculty of Physics, Astronomy and Informatics
  • WIESLAW NOWAK

    Nicolaus Copernicus University, Institute of Physics, Faculty of Physics, Astronomy and Informatics

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