# On the $1/3-2/3$ Conjecture

**Authors:** Emily J. Olson, Bruce E. Sagan

arXiv: 1706.04985 · 2018-02-02

## TL;DR

This paper advances the $1/3-2/3$ Conjecture by proving it for specific classes of finite posets, including lattices, Young diagram-based orders, and certain dimension 2 posets, and explores related balanced pair conditions.

## Contribution

The paper proves the $1/3-2/3$ Conjecture for several families of posets such as lattices, Young diagram orders, and some dimension 2 posets, extending known cases.

## Key findings

- The conjecture holds for Boolean, set partition, and subspace lattices.
- It is valid for posets derived from Young diagrams.
- Certain posets with automorphisms have a 1/2-balanced pair.

## Abstract

Let $(P,\leq)$ be a finite poset (partially ordered set), where $P$ has cardinality $n$. Consider linear extensions of $P$ as permutations $x_1x_2\cdots x_n$ in one-line notation. For distinct elements $x,y\in P$, we define $\mathbb{P}(x\prec y)$ to be the proportion of linear extensions of $P$ in which $x$ comes before $y$. For $0\leq \alpha \leq \frac{1}{2}$, we say $(x,y)$ is an $\alpha$-balanced pair if $\alpha \leq \mathbb{P}(x\prec y) \leq 1-\alpha.$ The $1/3-2/3$ Conjecture states that every finite partially ordered set which is not a chain has a $1/3$-balanced pair. We make progress on this conjecture by showing that it holds for certain families of posets. These include lattices such as the Boolean, set partition, and subspace lattices; partial orders that arise from a Young diagram; and some partial orders of dimension $2$. We also consider various posets which satisfy the stronger condition of having a $1/2$-balanced pair. For example, this happens when the poset has an automorphism with a cycle of length $2$. Various questions for future research are posed.

## Full text

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## Figures

40 figures with captions in the complete paper: https://tomesphere.com/paper/1706.04985/full.md

## References

14 references — full list in the complete paper: https://tomesphere.com/paper/1706.04985/full.md

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Source: https://tomesphere.com/paper/1706.04985