The healthy DGP branch in a state of self-acceleration
Mariam Bouhmadi-Lopez
TL;DR
This paper introduces a method to self-accelerate the normal DGP branch by deriving maximally symmetric solutions and analyzing their stability, contributing to understanding cosmic acceleration mechanisms.
Contribution
It presents a novel approach to self-accelerate the normal DGP branch and examines the stability of resulting solutions.
Findings
Successfully derived maximally symmetric solutions
Identified conditions for stability of solutions
Enhanced understanding of self-acceleration in DGP models
Abstract
We present a method to self-accelerate the normal DGP branch. We obtain the maximally symmetric solutions and study their stability.
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