Relieving the $S_8$ Tension: Exploring the Surface-type DBI Model as a Dark Matter Paradigm

TL;DR

This paper investigates a surface-type DBI model as a dark matter paradigm to address the $S_8$ tension, showing that it yields consistent low-redshift measurements and may resolve small-scale CDM issues.

Contribution

The study introduces the surface-type DBI model and demonstrates its potential to reconcile $S_8$ measurements from different cosmological probes.

Findings

sDBI model yields $S_8$ values consistent with low-redshift observations.

The model shows self-consistency across high- and low-redshift data.

Discussion on non-linear effects suggests potential to solve small-scale CDM problems.

Abstract

Recent observations from weak gravitational lensing (WL) surveys indicate a smoother Universe compared to the predictions of the Cosmic Microwave Background (CMB). This inconsistency is commonly referred to as the $\sigma_8$ tension or $S_8$ tension, where $\sigma_8$ represents the present root-mean-square matter fluctuation averaged over a sphere of radius $8 h^{-1} \mathrm{Mpc}$, and $S_8 \equiv \sigma_8\sqrt{\Omega_m/0.3}$. In this article, we investigate a kind of general Dirac-Born-Infeld (DBI) Lagrangian referred to as \textit{surface-type DBI} (sDBI) model. We find that up to the linear order, the constraints on the sDBI model with high-redshift probe (CMB) and low-redshift probes (WL and Galaxy Clustering, GC) yield $S_8= 0.7448_{-0.21}^{+0.031}$ and $0.7426_{-0.085}^{+0.054}$, respectively. Remarkably, these values not only demonstrate self-consistency but also align with the values obtained from the majority of low-redshift probes. Furthermore, we present a discussion on exploring the non-linear effects of this model, which holds the potential to address additional challenges associated with Cold Dark Matter (CDM) on small scales.