What question did this study set out to answer?

The research aims to establish a new framework for understanding cosmic inflation and dark sectors through emergent gravity and topology.

May 12, 2026Open Access

The Zero-Sum Anomaly Hypothesis (ZSAH): A Topological and Emergent Gravity Model for Inflation and Dark Sectors

Puntos clave

The research aims to establish a new framework for understanding cosmic inflation and dark sectors through emergent gravity and topology.
Proposes a cosmological framework that integrates emergent gravity, conformal cyclic cosmology, and primordial black holes.
Describes the universe's origin as a stochastic excursion from a zero-energy vacuum state.
Analyzes galactic rotation curves and cosmic acceleration within this new model.
Presents a unified explanation for observed galactic rotation curves without dark matter particles.
Demonstrates accelerated expansion as a response of the vacuum, implying interconnectedness of dark sectors.
Suggests that current dark sectors reflect aspects of a singular geometric property of the universe's vacuum.

Resumen

I propose a novel cosmological framework where the universe originates as a discrete stochastic excursion from a flat, zero-energy vacuum state ("The Canvas"). In this model, the Big Bang is not an isolated singularity but a localized positive energy anomaly DE>0 compensated by non-local, distributed negative potential wells throughout the global vacuum. By integrating Emergent Gravity (Verlinde), Conformal Cyclic Cosmology (Penrose), and Primordial Black Holes (PBHs) as topological anchors, I provide a unified explanation for galactic rotation curves and accelerated expansion without the need for undetected dark particles. This synthesis suggests that the current "Dark Sectors" are partial observations of a single, underlying geometric response of the vacuum.

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