Exact $f(R)$-cosmological model coming from the request of the existence of a Noether symmetry
S. Capozziello, P. Martin-Moruno, C. Rubano

TL;DR
This paper introduces an exact $f(R)$-cosmological model derived from Noether symmetry principles, capable of describing both decelerated and accelerated phases of the universe's expansion.
Contribution
It presents a novel $f(R)$-model with an exact solution based on Noether symmetry, bridging decelerated and accelerated cosmic phases.
Findings
Model describes a dust-dominated decelerated phase
Model transitions to current accelerated expansion
Exact analytic solution obtained from symmetry considerations
Abstract
We present an -cosmological model with an exact analytic solution, coming from the request of the existence of a Noether symmetry, which is able to describe a dust-dominated decelerated phase before the current accelerated phase of the universe.
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