Davenport–Schinzel sequences were first defined in 1965 by Harold Davenport and Andrzej Schinzel to analyze linear differential equations.
Following Atallah (1985) these sequences and their length bounds have also become a standard tool in discrete geometry and in the analysis of geometric algorithms.
Due to the very rapid growth of the Ackermann function, its inverse α grows very slowly, and is at most four for problems of any practical size.
[3] Using big O and big Θ notation, the following bounds are known: The value of λs(n) is also known when s is variable but n is a small constant:[10] When s is a function of n the upper and lower bounds on Davenport-Schinzel sequences are not tight.
For instance, a non-vertical line segment in the plane can be interpreted as the graph of a function mapping an interval of x values to their corresponding y values, and the lower envelope of a collection of line segments forms a Davenport–Schinzel sequence of order three because any two line segments can form an alternating subsequence with length at most four.