Skip to content
Research Article Open access CC BY 4.0

Gaussian Numbers with Generalized Pandita Numbers Components

Fatih Zahid KALCA, Yüksel Soykan

Asian Journal of Advanced Research and Reports · pp. 32–56 · Published 3 Jul 2025

10.9734/ajarr/2025/v19i71079

Abstract

In this study, we introduce and investigate a new class of numerical sequences in the complex domain—Gaussian generalized Pandita numbers—which extend the classical theory of linear recurrence relations. In particular, we focus on two distinct cases: the Gaussian Pandita numbers and the Gaussian Pandita-Lucas numbers. For these sequences, we derive and present a comprehensive set of mathematical results, including recurrence relations, closed-form expressions via Binet-type formulas, ordinary and exponential generating functions. In addition, we establish various algebraic identities, provide matrix representations, and prove generalized forms of Simpson’s formula. Summation identities are also developed to further explore the structural and analytical properties of these numbers. The findings contribute to the broader theory of Gaussian integer sequences and open new directions for applications in discrete mathematics and computational number theory.

Pandita numbers pandita-lucas numbers gaussian pandita numbers gaussian pandita-lucas numbers binet’s formulas generating functions exponential generating functions

Cited by 0

No indexed citations yet.

Article metrics

Real usage data collected on this platform.

0

Page views

0

PDF downloads

0

Outbound clicks

0

Citations

Views by country

Approximate, from request IP at view time — not citizenship or institution. Countries with fewer than 5 views are grouped as "Other".

No views recorded yet.

Traffic sources

Referring site, by host.

No traffic recorded yet.

Views and downloads exclude known bots/crawlers. Citations combines this platform's own DOI-resolved index with each external source's own reported total — see Cited by above for individually listed citing works. Last refreshed 0 seconds ago.