TL;DR
This paper proposes a new inflationary cosmological model within general relativity that incorporates self-interacting spinning matter, extending the standard fluid model to better understand early universe dynamics.
Contribution
It introduces a generalized fluid model with spinning matter for inflation, providing estimates of physical parameters and expanding the theoretical framework.
Findings
Spinning matter can drive inflation in the early universe.
The generalized model offers new insights into inflationary dynamics.
Parameter estimates support the viability of the model.
Abstract
Following recent studies of Ford, we suggest -- in the framework of general relativity -- an inflationary cosmological model with the self-interacting spinning matter. A generalization of the standard fluid model is discussed and estimates of the physical parameters of the evolution are given.
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