Modeling and Testing Screening Mechanisms in the Laboratory and in Space

Author:

Vardanyan Valeri12ORCID,Bartlett Deaglan J.3ORCID

Affiliation:

1. Kavli Institute for the Physics and Mathematics of the Universe (WPI), UTIAS, The University of Tokyo, Chiba 277-8583, Japan

2. Center for Data-Driven Discovery, Kavli IPMU (WPI), UTIAS, The University of Tokyo, Kashiwa, Chiba 277-8583, Japan

3. Institut d’Astrophysique de Paris (IAP), CNRS & Sorbonne Université, UMR 7095, 98 bis bd Arago, F-75014 Paris, France

Abstract

The non-linear dynamics of scalar fields coupled to matter and gravity can lead to remarkable density-dependent screening effects. In this short review, we present the main classes of screening mechanisms, and discuss their tests in laboratory and astrophysical systems. We particularly focused on reviewing numerical and technical aspects involved in modeling the non-linear dynamics of screening and on tests using laboratory experiments and astrophysical systems, such as stars, galaxies, and dark matter halos.

Funder

WPI Research Center Initiative, MEXT, Japan

JSPS KAKENHI

Simons Collaboration on “Learning the Universe”

Publisher

MDPI AG

Subject

General Physics and Astronomy

Reference204 articles.

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