Proca in the sky


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Date

2021-03

Publication Type

Journal Article

ETH Bibliography

yes

Citations

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Abstract

The standard model of cosmology, the ΛCDM model, describes the evolution of the Universe since the Big Bang with just a few parameters, six in its basic form. Despite being the simplest model, direct late-time measurements of the Hubble constant compared with the early-universe measurements result in the so-called H0 tension. It is claimed that a late time resolution is predestined to fail when different cosmological probes are combined. In this work, we shake the ground of this belief with a very simple model. We show how, in the context of cubic vector Galileon models, the Hubble tension can naturally be relieved using a combination of CMB, BAO and SNe observations without using any prior on H0. The tension can be reduced even further by including the local measurement of the Hubble constant.

Publication status

published

Editor

Book title

Volume

2021 (3)

Pages / Article No.

32

Publisher

IOP Publishing

Event

Edition / version

Methods

Software

Geographic location

Date collected

Date created

Subject

cosmological parameters from CMBR; dark energy theory; cosmology of theories beyond the SM; modified gravity

Organisational unit

09662 - Heisenberg, Lavinia (ehemalig) / Heisenberg, Lavinia (former) check_circle

Notes

Funding

179740 - Multimessenger constraints of modified gravity (SNF)

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