Paratingent cone

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In mathematics, the paratingent cone and contingent cone were introduced by Bouligand (1932), and are closely related to tangent cones.

Definition

Let S be a nonempty subset of a real normed vector space (X,‖⋅‖).

  1. Let some x¯∈cl⁡(S) be a point in the closure of S. An element h∈X is called a tangent (or tangent vector) to S at x¯, if there is a sequence (xn)n∈ℕ of elements xn∈S and a sequence (λn)n∈ℕ of positive real numbers λn>0 such that x¯=limn→∞xn and h=limn→∞λn(xn−x¯).
  2. The set T(S,x¯) of all tangents to S at x¯ is called the contingent cone (or the Bouligand tangent cone) to S at x¯.[1]

An equivalent definition is given in terms of a distance function and the limit infimum. As before, let (X,‖⋅‖) be a normed vector space and take some nonempty set S⊂X. For each x∈X, let the distance function to S be

dS(x):=inf⁡{‖x−x′‖∣x′∈S}.

Then, the contingent cone to S⊂X at x∈cl⁡(S) is defined by[2]

TS(x):={v:lim infh→0+dS(x+hv)h=0}.

References

  1. ↑ Johannes, Jahn (2011). Vector Optimization. Springer Berlin Heidelberg. pp. 90–91. doi:10.1007/978-3-642-17005-8. ISBN 978-3-642-17005-8. https://link.springer.com/book/10.1007/978-3-642-17005-8. 
  2. ↑ Aubin, Jean-Pierre; Frankowska, Hèléne (2009). "Chapter 4: Tangent Cones". Set-Valued Analysis. Modern Birkhäuser Classics. Boston: Birkhäuser. p. 121. doi:10.1007/978-0-8176-4848-0_4. ISBN 978-0-8176-4848-0. https://doi.org/10.1007/978-0-8176-4848-0_4.