# On the extensions of the Diophantine triples in Gaussian integers

**Authors:** Nikola Ad\v{z}aga, Alan Filipin, Zrinka Franu\v{s}i\'c

arXiv: 1905.09332 · 2019-05-24

## TL;DR

This paper investigates whether certain Diophantine triples in Gaussian integers can be extended to quadruples, addressing the challenges with Diophantine approximations and employing linear forms in logarithms for partial solutions.

## Contribution

It extends the study of specific Diophantine triples in Gaussian integers and applies linear forms in logarithms to overcome previous methodological difficulties.

## Key findings

- Identified limitations of previous methods due to small gaps between elements.
- Successfully used linear forms in logarithms for partial extension results.
- Highlighted the complexity of extending Diophantine triples in Gaussian integers.

## Abstract

A Diophantine $m$-tuple is a set of $m$ distinct integers such that the product of any two distinct elements plus one is a perfect square. In this paper we study the extensibility of a Diophantine triple $\{k-1, k+1, 16k^3-4k\}$ in Gaussian integers $\mathbb{Z}[i]$ to a Diophantine quadruple. Similar one-parameter family, $\{k-1, k+1, 4k\}$, was studied in Franu\v{s}i\'c's previous paper, where it was shown that the extension to a Diophantine quadruple is unique (with an element $16k^3-4k$). The family of the triples of the same form $\{k-1, k+1, 16k^3-4k\}$ was already studied in rational integers. It appeared as a special case while solving the extensibility problem of Diophantine pair $\{k-1, k+1\}$, in which it was not possible to use the same method as in the other cases. As authors (Bugeaud, Dujella and Mignotte) point out, the difficulty appears because the gap between $k+1$ and $16k^3-4k$ is not sufficiently large. We find the same difficulty here while trying to use Diophantine approximations. Then we partially solve this problem by using linear forms in logarithms.

## Full text

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## References

14 references — full list in the complete paper: https://tomesphere.com/paper/1905.09332/full.md

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Source: https://tomesphere.com/paper/1905.09332