Yan-Hong Yao, Jian-Qi Liu, Zhi-Qi Huang, Jun-Chao Wang, Yan Su
{"title":"A new unified dark sector model and its implications on the $σ_8$ and $S_8$ tensions","authors":"Yan-Hong Yao, Jian-Qi Liu, Zhi-Qi Huang, Jun-Chao Wang, Yan Su","doi":"arxiv-2409.04678","DOIUrl":null,"url":null,"abstract":"In this paper, we introduced the Unified Three-Form Dark Sector (UTFDS)\nmodel, a unified dark sector model that combines dark energy and dark matter\nthrough a three-form field. In this framework, the potential of the three-form\nfield acts as dark matter, while the kinetic term represents dark energy. The\ninteraction between dark matter and dark energy is driven by the energy\nexchange between these two terms. Given the dynamical equations of UTFDS, we\nprovide an autonomous system of evolution equations for UTFDS and perform a\nstability analysis of its fixed points. The result aligns with our expectations\nfor a unified dark sector. Furthermore, we discover that the dual Lagrangian of\nthe UTFDS Lagrangian is equivalent to a Dirac-Born-Infeld (DBI) Lagrangian. By\nfixing the parameter $\\kappa X_0$ to 250, 500, 750, we refer to the resulting\nmodels as the $\\overline{\\rm UTFDS}$ model with $\\kappa X_0$=250, 500, 750,\nrespectively. We then place constraints on these three $\\overline{\\rm UTFDS}$\nmodels and the $\\Lambda$CDM model in light of the Planck 2018 Cosmic Microwave\nBackground (CMB) anisotropies, Redshift Space Distortions (RSD) observations,\nBaryon Acoustic Oscillation (BAO) measurements, and the $S_8$ prior chosen\naccording to the KiDS1000 Weak gravitational Lensing (WL) measuement. We find\nthat the $\\overline{\\rm UTFDS}$ model with $\\kappa X_0$=500 is the only one\namong the four models where both $\\sigma_8$ and $S_8$ tensions, between CMB and\nRSD+BAO+WL datasets, are below 2.0$\\sigma$. Furthermore, the tensions are\nrelieved without exacerbating the $H_0$ tension. Although both the CMB and\nRSD+BAO+WL datasets provide definite/positive evidence favoring $\\Lambda$CDM\nover the $\\overline{\\rm UTFDS}$ model with $\\kappa X_0$=500, the evidence is\nnot strong enough to rule out further study of this model.","PeriodicalId":501207,"journal":{"name":"arXiv - PHYS - Cosmology and Nongalactic Astrophysics","volume":"72 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-09-07","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv - PHYS - Cosmology and Nongalactic Astrophysics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/arxiv-2409.04678","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
Abstract
In this paper, we introduced the Unified Three-Form Dark Sector (UTFDS)
model, a unified dark sector model that combines dark energy and dark matter
through a three-form field. In this framework, the potential of the three-form
field acts as dark matter, while the kinetic term represents dark energy. The
interaction between dark matter and dark energy is driven by the energy
exchange between these two terms. Given the dynamical equations of UTFDS, we
provide an autonomous system of evolution equations for UTFDS and perform a
stability analysis of its fixed points. The result aligns with our expectations
for a unified dark sector. Furthermore, we discover that the dual Lagrangian of
the UTFDS Lagrangian is equivalent to a Dirac-Born-Infeld (DBI) Lagrangian. By
fixing the parameter $\kappa X_0$ to 250, 500, 750, we refer to the resulting
models as the $\overline{\rm UTFDS}$ model with $\kappa X_0$=250, 500, 750,
respectively. We then place constraints on these three $\overline{\rm UTFDS}$
models and the $\Lambda$CDM model in light of the Planck 2018 Cosmic Microwave
Background (CMB) anisotropies, Redshift Space Distortions (RSD) observations,
Baryon Acoustic Oscillation (BAO) measurements, and the $S_8$ prior chosen
according to the KiDS1000 Weak gravitational Lensing (WL) measuement. We find
that the $\overline{\rm UTFDS}$ model with $\kappa X_0$=500 is the only one
among the four models where both $\sigma_8$ and $S_8$ tensions, between CMB and
RSD+BAO+WL datasets, are below 2.0$\sigma$. Furthermore, the tensions are
relieved without exacerbating the $H_0$ tension. Although both the CMB and
RSD+BAO+WL datasets provide definite/positive evidence favoring $\Lambda$CDM
over the $\overline{\rm UTFDS}$ model with $\kappa X_0$=500, the evidence is
not strong enough to rule out further study of this model.