Inflation model and Riemann tensor on non-associative algebra
V. Yu. Dorofeev

TL;DR
This paper explores a novel inflation model based on non-associative algebra, linking space reduction to inflation, and introduces a new gravitational constant derived from octonion algebra, with implications for early universe dynamics.
Contribution
It presents a new inflation framework using non-associative algebra and constructs a gravitational constant from octonion algebra, connecting algebraic structures to cosmological evolution.
Findings
Space reduction interpreted as inflation process.
Non-associativity leads to two-stage inflation.
Continuous link between Friedmann and inflationary stages.
Abstract
In this article the reduction of a -dimensional space to a -dimensional space is considered as a reduction of states to states, where stands for the number of single-particle states per unit of spatial length. It turns out, this space reduction could be understood as another definition of inflation. It is shown that the introduction of the non-associativity of the algebra of physical fields in a homogeneous space leads to a nonlinear equation, the solutions of which can be considered as two-stage inflation. Using the example of reduction to , it is shown that there is a continuous cross-linking of the Friedmann and inflationary stages of algebraic inflation at times with the number of baryons in the Universe. In this paper, we construct a new gravitational constant based on a nonassociative octonion algebra.
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Taxonomy
TopicsCosmology and Gravitation Theories · Relativity and Gravitational Theory · Geophysics and Gravity Measurements
