The Orbit-Summable Fixed Point Criterion and its Relation to Caristi's Theorem

The relationship between geometric and variational principles remains central to Nonlinear Analysis. This paper introduces the \textbf{Orbit-Summability Fixed Point Criterion}, a novel, purely dynamical condition, and establishes its profound connection to \textbf{Caristis Fixed Point Theorem} in complete metric spaces. Our criterion, which requires only that the total displacement along a single orbit be finite (the orbit-summability property), provides a practical and concrete tool for checking the existence of fixed points without relying on the construction of an abstract potential function. We demonstrate that, under a minimal regularity assumption involving the function $f$ and the metric $d$, the Orbit-Summability Criterion is \textbf{precisely equivalent} to Caristis Fixed Point Theorem. This equivalence is conceptually significant as it creates a direct bridge between the geometric principle of \textbf{dynamical gap summability} (akin to the core idea in Banach`s Contraction Principle) and the variational principle of Caristi. As a direct consequence of this equivalence, the classical \textbf{Banach Contraction Principle is recovered as a straightforward corollary}. The methodology is designed to merge key elements from the Banach proof (orbit convergence via summability) with the structural requirements of Caristi (majorization by a well-behaved functional), effectively providing a unifying framework for these fundamental results. Thus, the Orbit-Summability Criterion offers an attractive and accessible perspective on these established cornerstones of Fixed Point Theory.

💡 Research Summary

The manuscript introduces a new purely dynamical fixed‑point condition called the Orbit‑Summability Fixed Point Criterion and proves that, under a modest regularity hypothesis, it is exactly equivalent to Caristi’s Fixed Point Theorem in complete metric spaces. The orbit‑summability property requires only that the total displacement along a single forward orbit be finite, i.e.
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