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Twist (differential geometry)

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Differential geometry term For twists of curves in algebraic geometry, see twists of elliptic curves.

In differential geometry, the twist of a ribbon is its rate of axial rotation. Let a ribbon ( X , U ) {\displaystyle (X,U)} be composed of a space curve, X = X ( s ) {\displaystyle X=X(s)} , where s {\displaystyle s} is the arc length of X {\displaystyle X} , and U = U ( s ) {\displaystyle U=U(s)} the a unit normal vector, perpendicular at each point to X {\displaystyle X} . Since the ribbon ( X , U ) {\displaystyle (X,U)} has edges X {\displaystyle X} and X = X + ε U {\displaystyle X'=X+\varepsilon U} , the twist (or total twist number) T w {\displaystyle Tw} measures the average winding of the edge curve X {\displaystyle X'} around and along the axial curve X {\displaystyle X} . According to Love (1944) twist is defined by

T w = 1 2 π ( U × d U d s ) d X d s d s , {\displaystyle Tw={\dfrac {1}{2\pi }}\int \left(U\times {\dfrac {dU}{ds}}\right)\cdot {\dfrac {dX}{ds}}ds\;,}

where d X / d s {\displaystyle dX/ds} is the unit tangent vector to X {\displaystyle X} . The total twist number T w {\displaystyle Tw} can be decomposed (Moffatt & Ricca 1992) into normalized total torsion T [ 0 , 1 ) {\displaystyle T\in [0,1)} and intrinsic twist N Z {\displaystyle N\in \mathbb {Z} } as

T w = 1 2 π τ d s + [ Θ ] X 2 π = T + N , {\displaystyle Tw={\dfrac {1}{2\pi }}\int \tau \;ds+{\dfrac {\left_{X}}{2\pi }}=T+N\;,}

where τ = τ ( s ) {\displaystyle \tau =\tau (s)} is the torsion of the space curve X {\displaystyle X} , and [ Θ ] X {\displaystyle \left_{X}} denotes the total rotation angle of U {\displaystyle U} along X {\displaystyle X} . Neither N {\displaystyle N} nor T w {\displaystyle Tw} are independent of the ribbon field U {\displaystyle U} . Instead, only the normalized torsion T {\displaystyle T} is an invariant of the curve X {\displaystyle X} (Banchoff & White 1975).

When the ribbon is deformed so as to pass through an inflectional state (i.e. X {\displaystyle X} has a point of inflection), the torsion τ {\displaystyle \tau } becomes singular. The total torsion T {\displaystyle T} jumps by ± 1 {\displaystyle \pm 1} and the total angle N {\displaystyle N} simultaneously makes an equal and opposite jump of 1 {\displaystyle \mp 1} (Moffatt & Ricca 1992) and T w {\displaystyle Tw} remains continuous. This behavior has many important consequences for energy considerations in many fields of science (Ricca 1997, 2005; Goriely 2006).

Together with the writhe W r {\displaystyle Wr} of X {\displaystyle X} , twist is a geometric quantity that plays an important role in the application of the Călugăreanu–White–Fuller formula L k = W r + T w {\displaystyle Lk=Wr+Tw} in topological fluid dynamics (for its close relation to kinetic and magnetic helicity of a vector field), physical knot theory, and structural complexity analysis.

References

  • Banchoff, T.F. & White, J.H. (1975) The behavior of the total twist and self-linking number of a closed space curve under inversions. Math. Scand. 36, 254–262.
  • Goriely, A. (2006) Twisted elastic rings and the rediscoveries of Michell’s instability. J Elasticity 84, 281-299.
  • Love, A.E.H. (1944) A Treatise on the Mathematical Theory of Elasticity. Dover, 4th Ed., New York.
  • Moffatt, H.K. & Ricca, R.L. (1992) Helicity and the Calugareanu invariant. Proc. R. Soc. London A 439, 411-429. Also in: (1995) Knots and Applications (ed. L.H. Kauffman), pp. 251-269. World Scientific.
  • Ricca, R.L. (1997) Evolution and inflexional instability of twisted magnetic flux tubes. Solar Physics 172, 241-248.
  • Ricca, R.L. (2005) Inflexional disequilibrium of magnetic flux tubes. Fluid Dynamics Research 36, 319-332.
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