Can late-time extensions solve the H0 and σ8 tensions

• Verfasst von: Heisenberg, Lavinia [VerfasserIn]
• Verfasst von: Villarrubia-Rojo, Héctor [VerfasserIn]
• Verfasst von: Zosso, Jann [VerfasserIn]
• Titel: Can late-time extensions solve the H0 and σ8 tensions
• Verf.angabe: Lavinia Heisenberg, Hector Villarrubia-Rojo and Jann Zosso
• E-Jahr: 2022
• Jahr: 2 August 2022
• Umfang: 12 S.
• Fussnoten: Im Titel ist "0" und "8" jeweils tiefgestellt ; Gesehen am 30.09.2022
• Titel Quelle: Enthalten in: Physical review
• Ort Quelle: Woodbury, NY : Inst., 2016
• Jahr Quelle: 2022
• Band/Heft Quelle: 106(2022), 4, Artikel-ID 043503, Seite 1-12
• ISSN Quelle: 2470-0029
• DOI: doi:10.1103/PhysRevD.106.043503
• Datenträger: Online-Ressource
• Sprache: eng
• K10plus-PPN: 181788770X

Abstract

We analyze the properties that any late-time modification of the Lambda CDM expansion history must have in order to consistently solve both the H-0 and the sigma(8) tensions. Taking a model-independent approach, we obtain a set of necessary conditions that can be applied to any late-time extension whose main effect is a deviation from the.CDM background. Our results are fully analytical and merely based on the assumptions that the deviations from the.CDM background remain small. For the concrete case of a dark energy fluid with equation of state w(z), we derive the following general requirements: (i) Solving the H-0 tension demands w(z) < -1 at some z (ii) Solving both the H-0 and sigma(8) tensions requires w(z) to cross the phantom divide. Finally, we also allow for small deviations on the effective gravitational constant. In this case, our method is still able to constrain the functional form of these deviations.