Shape dependence of Vainshtein screening

Scalar field theories that possess a Vainshtein mechanism are able to dynamically suppress the associated fifth forces in the presence of massive sources through derivative nonlinearities. The resulting equations of motion for the scalar are highly nonlinear, and therefore very few analytic solution...

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Main Authors: Bloomfield, Jolyon K., Burrage, Clare, Davis, Anne-Christine
Format: Article
Published: American Physical Society 2015
Online Access:https://eprints.nottingham.ac.uk/42098/
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author Bloomfield, Jolyon K.
Burrage, Clare
Davis, Anne-Christine
author_facet Bloomfield, Jolyon K.
Burrage, Clare
Davis, Anne-Christine
author_sort Bloomfield, Jolyon K.
building Nottingham Research Data Repository
collection Online Access
description Scalar field theories that possess a Vainshtein mechanism are able to dynamically suppress the associated fifth forces in the presence of massive sources through derivative nonlinearities. The resulting equations of motion for the scalar are highly nonlinear, and therefore very few analytic solutions are known. Here, we present a brief investigation of the structure of Vainshtein screening in symmetrical configurations, focusing in particular on the spherical, cylindrical and planar solutions that are relevant for observations of the cosmic web. We consider Vainshtein screening in both the Galileon model, where the nonlinear terms involve second derivatives of the scalar, and a k-essence theory, where the nonlinear terms involve only first derivatives of the scalar. We find that screening, and consequently the suppression of the scalar force, is most efficient around spherical sources, weaker around cylindrical sources and can be absent altogether around planar sources.
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spelling nottingham-420982020-05-04T17:07:03Z https://eprints.nottingham.ac.uk/42098/ Shape dependence of Vainshtein screening Bloomfield, Jolyon K. Burrage, Clare Davis, Anne-Christine Scalar field theories that possess a Vainshtein mechanism are able to dynamically suppress the associated fifth forces in the presence of massive sources through derivative nonlinearities. The resulting equations of motion for the scalar are highly nonlinear, and therefore very few analytic solutions are known. Here, we present a brief investigation of the structure of Vainshtein screening in symmetrical configurations, focusing in particular on the spherical, cylindrical and planar solutions that are relevant for observations of the cosmic web. We consider Vainshtein screening in both the Galileon model, where the nonlinear terms involve second derivatives of the scalar, and a k-essence theory, where the nonlinear terms involve only first derivatives of the scalar. We find that screening, and consequently the suppression of the scalar force, is most efficient around spherical sources, weaker around cylindrical sources and can be absent altogether around planar sources. American Physical Society 2015-04-07 Article PeerReviewed Bloomfield, Jolyon K., Burrage, Clare and Davis, Anne-Christine (2015) Shape dependence of Vainshtein screening. Physical Review D, D91 (8). 083510/1-083510/10. ISSN 2470-0029 https://journals.aps.org/prd/abstract/10.1103/PhysRevD.91.083510 doi:10.1103/PhysRevD.91.083510 doi:10.1103/PhysRevD.91.083510
spellingShingle Bloomfield, Jolyon K.
Burrage, Clare
Davis, Anne-Christine
Shape dependence of Vainshtein screening
title Shape dependence of Vainshtein screening
title_full Shape dependence of Vainshtein screening
title_fullStr Shape dependence of Vainshtein screening
title_full_unstemmed Shape dependence of Vainshtein screening
title_short Shape dependence of Vainshtein screening
title_sort shape dependence of vainshtein screening
url https://eprints.nottingham.ac.uk/42098/
https://eprints.nottingham.ac.uk/42098/
https://eprints.nottingham.ac.uk/42098/