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Star-Shaped Structures of Dihedral Symmetry

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Tensegrity Structures

Part of the book series: Mathematics for Industry ((MFI,volume 6))

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Abstract

This chapter presents self-equilibrium as well as super-stability conditions for star-shaped structures that have dihedral symmetry. Star-shaped tensegrity structures have the same dihedral symmetry and similar configurations to the prismatic structures studied in Chap. 6. The star-shaped structures have more infinitesimal mechanisms than prismatic structures due to the two additional (center) nodes, nevertheless, they are super-stable if certain connectivity conditions are satisfied. Moreover, some star-shaped structures that are not super-stable might be multi-stable; i.e., they may have more than one stable configuration.

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Notes

  1. 1.

    The divisible star-shaped structures might not be physically separated into serval substructures because they share the common center nodes.

References

  1. Fowler, P. W., & Guest, S. D. (2000). A symmetry extension of Maxwell’s rule for rigidity of frames. International Journal of Solids and Structures, 37(12), 1793–1804.

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  3. Kettle, S. F. A. (2007). Symmetry and structure: readable group theory for chemists. New York: Wiley.

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Correspondence to Jing Yao Zhang .

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Zhang, J.Y., Ohsaki, M. (2015). Star-Shaped Structures of Dihedral Symmetry. In: Tensegrity Structures. Mathematics for Industry, vol 6. Springer, Tokyo. https://doi.org/10.1007/978-4-431-54813-3_7

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  • DOI: https://doi.org/10.1007/978-4-431-54813-3_7

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  • Publisher Name: Springer, Tokyo

  • Print ISBN: 978-4-431-54812-6

  • Online ISBN: 978-4-431-54813-3

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