Screening mechanisms for a three-form field around a dense source such as the Sun are investigated. Working with the dual vector, we can obtain a thin-shell where field interactions are short range. The field outside the source adopts the configuration of a dipole which is a manifestly distinct behaviour from the one obtained with a scalar field or even a previously proposed vector field model. We identify the region of parameter space where this model satisfies present solar system tests.
@article{arxiv.1610.00357,
title = {Screening three-form fields},
author = {Tiago Barreiro and Ugo Bertello and Nelson J. Nunes},
journal= {arXiv preprint arXiv:1610.00357},
year = {2017}
}