Sezione

HEP Colloquia 2021

by Dr Riccardo Murgia (LUPM Montpellier)

Europe/Rome
Online

Online

Description

Hitchhiker’s Guide to Cosmological Concordance

According to the standard cosmological (ΛCDM) model, the present universe is mainly composed of a cosmological constant, denoted by Λ, and by Cold DarkMatter (CDM). Such a paradigm is in tremendous agreement with Cosmic Microwave Background(CMB) and Large-Scale Structure (LSS) data, yet some tensions exist: namely, on the local, direct determinations of the expansion rate of the universe, H0, and the amplitude of the matter fluctuations today,σ8, which are45σ higher and 23σ lower, respectively, compared to the values inferred from early universe observations within ΛCDM. Furthermore, the amount of gravitational lensing determined from the CMB temperature and polarization power spectra from Planckis23σ higher than that measured from the lensing potential reconstruction, and expected in ΛCDM. Finally, assuming purely CDM, cosmological N-body simulations show some limits in reproducing the observed astrophysical properties on (sub-)galactic scales. In the absence of fully satisfactory solutions within the CDM framework, and driven by the fact that the nature of the dark sector is still unknown, a number of alternative scenarios have emerged as a possible way to explain the discrepancies. I will discuss why these tensions could hint to new physics, outline paths towards restoring cosmological concordance, and present up-to-date bounds on some of the most promising proposed resolutions, such as early dark energy, sterile neutrinos, DM interacting with dark radiation, decaying DM

 

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https://infn-it.zoom.us/j/83682324121?pwd=ZlhsNzgxbGQwVGhVT2wrUHVwOU1DUT09

Meeting ID: 836 8232 4121
Passcode: 318219
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Organised by

Prof. Umberto D'Alesio - umberto.dalesio@ca.infn.it
Ph.D. Michela Lai - michela.lai@ca.infn.it
Dr Luca Maxia - luca.maxia@ca.infn.it
Dr Mauro Oi - mauro.oi@ca.infn.it