# Linear programming based approximation for unweighted induced matchings   --- breaking the $\Delta$ barrier

**Authors:** Julien Baste, Maximilian F\"urst, Dieter Rautenbach

arXiv: 1812.05930 · 2018-12-17

## TL;DR

This paper introduces improved approximation algorithms for unweighted induced matchings in graphs, surpassing previous bounds and conjecturing tighter integrality gaps, with specific results for graphs of maximum degree 3.

## Contribution

It presents primal-dual approximation algorithms with ratios close to the conjectured integrality gap for unweighted induced matchings, improving upon prior methods.

## Key findings

- Approximation ratio of (1-ε)Δ + 0.5 for general Δ with ε ≈ 0.02005
- Approximation ratio of 7/3 for Δ=3
- Proved a best-possible bound on fractional induced matching number

## Abstract

A matching in a graph is induced if no two of its edges are joined by an edge, and finding a large induced matching is a very hard problem. Lin et al. (Approximating weighted induced matchings, Discrete Applied Mathematics 243 (2018) 304-310) provide an approximation algorithm with ratio $\Delta$ for the weighted version of the induced matching problem on graphs of maximum degree $\Delta$. Their approach is based on an integer linear programming formulation whose integrality gap is at least $\Delta-1$, that is, their approach offers only little room for improvement in the weighted case. For the unweighted case though, we conjecture that the integrality gap is at most $\frac{5}{8}\Delta+O(1)$, and that also the approximation ratio can be improved at least to this value. We provide primal-dual approximation algorithms with ratios $(1-\epsilon) \Delta + \frac{1}{2}$ for general $\Delta$ with $\epsilon \approx 0.02005$, and $\frac{7}{3}$ for $\Delta=3$. Furthermore, we prove a best-possible bound on the fractional induced matching number in terms of the order and the maximum degree.

## Full text

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## Figures

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## References

12 references — full list in the complete paper: https://tomesphere.com/paper/1812.05930/full.md

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Source: https://tomesphere.com/paper/1812.05930