Phantom scalar-tensor models and cosmological tensions
M. Ballardini, A. G. Ferrari, F. Finelli

TL;DR
This paper investigates extended scalar-tensor gravity models with negative kinetic terms, analyzing their cosmological implications and constraints, and finds that certain modifications can help reduce the H_0 tension in cosmology.
Contribution
It explores the effects of negative kinetic terms in scalar-tensor models on cosmological parameters and demonstrates potential in alleviating the H_0 tension.
Findings
Negative kinetic term models behave as negative energy density components.
Cosmological data constrain these models close to General Relativity.
Quartic coupling in phantom models can reduce the H_0 tension.
Abstract
We study three different extended scalar-tensor theories of gravity by also allowing a negative sign for the kinetic term for the scalar field in the Jordan frame. Our scope is to understand how the observational constraints for these models cope with the volume of the parameter space in which the theory is healthy. Models with a negative kinetic term lead to decreasing effective gravitational constant with redshift and behave as an effective relativistic component with a negative energy density as opposite to their corresponding version with a standard kinetic term. As a consequence, we find that the extended branch with a negative sign for the kinetic term correspond in general to lower and compared to CDM. We find that in all the cases with a negative sign for the kinetic term studied here, cosmological observations constrain these models around GR and…
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Taxonomy
TopicsCosmology and Gravitation Theories · Relativity and Gravitational Theory
