Emulating $\Lambda$CDM-like expansion on the Phantom brane

TL;DR

This paper corrects a previous expression for dark energy density on the phantom brane, demonstrating how it can emulate $ ext{Lambda}$CDM expansion, and explores its connection to quintessence fields and distinguishable perturbation growth.

Contribution

The authors derive a corrected expression for dark energy density on the phantom brane that mimics $ ext{Lambda}$CDM expansion and connect it to quintessence potentials, clarifying previous inaccuracies.

Findings

Corrected the expression for $ ho_{DE}$ on the phantom brane.

Showed that DDE can be modeled by a quintessence field with a specific potential.

Identified differences in density perturbation growth between braneworld and $ ext{Lambda}$CDM models.

Abstract

In [Schmidt PRD 80 123003 (2009)], the author suggested that dynamical dark energy (DDE) propagating on the phantom brane could mimick $\Lambda$CDM. Schmidt went on to derive a phenomenological expression for $\rho_{\rm DE}$ which could achieve this. We demonstrate that while Schmidt's central premise is correct, the expression for $\rho_{\rm DE}$ derived in Schmidt (2009) is flawed. We derive the correct expression for $\rho_{\rm DE}$ which leads to $\Lambda$CDM-like expansion on the phantom brane. We also show that DDE on the brane can be associated with a Quintessence field and derive a closed form expression for its potential $V(\phi)$. Interestingly the $\alpha$-attractor based potential $V(\phi) \propto \coth^2{\lambda\phi}$ makes braneworld expansion resemble $\Lambda$CDM. However the two models can easily be distinguished on the basis of density perturbations which grow at different rates on the braneworld and in $\Lambda$CDM.