Is the Energy Density of the Cosmic Quaternionic Field a Possible Candidate for the Black Energy?

TL;DR

This paper explores the hypothesis that the energy density of the cosmic quaternionic field could serve as a candidate for dark energy, potentially explaining the universe's accelerated expansion.

Contribution

It proposes a novel candidate for dark energy based on the properties of the cosmic quaternionic field, linking quaternionic field theory to cosmological observations.

Findings

Suggests the quaternionic field's energy density aligns with dark energy characteristics

Provides theoretical basis for quaternionic field as dark energy candidate

Encourages further investigation into quaternionic fields in cosmology

Abstract

We try to show that the energy density of the cosmic quaternionic field might be a possible candidate for the black energy.