Gravitational lens time-delay as a probe of a possible time variation of the fine-structure constant

Abstract A new method based on large scale structure observations is proposed to probe a possible temporal variation of the fine-structure constant ( $$\alpha $$ α ). Our analyses are based on time-delay of Strong Gravitational Lensing and Type Ia Supernovae observations. By considering the runaway...

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Main Authors: L. R. Colaço, J. E. Gonzalez, R. F. L. Holanda
Format: Article
Language:English
Published: SpringerOpen 2021-06-01
Series:European Physical Journal C: Particles and Fields
Online Access:https://doi.org/10.1140/epjc/s10052-021-09319-x
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author L. R. Colaço
J. E. Gonzalez
R. F. L. Holanda
author_facet L. R. Colaço
J. E. Gonzalez
R. F. L. Holanda
author_sort L. R. Colaço
collection DOAJ
description Abstract A new method based on large scale structure observations is proposed to probe a possible temporal variation of the fine-structure constant ( $$\alpha $$ α ). Our analyses are based on time-delay of Strong Gravitational Lensing and Type Ia Supernovae observations. By considering the runaway dilaton scenario, where the cosmological temporal evolution of the fine-structure constant is given by $$\frac{\Delta \alpha }{\alpha } \approx -\gamma \ln {(1+z)}$$ Δ α α ≈ - γ ln ( 1 + z ) , we obtain limits on the physical properties parameter of the model ( $$\gamma $$ γ ) at the level $$10^{-2}$$ 10 - 2 ( $$1\sigma $$ 1 σ ). Although our limits are less restrictive than those obtained by quasar spectroscopy, the approach presented here provides new bounds on the possibility of $$\frac{\Delta \alpha }{\alpha } \ne 0$$ Δ α α ≠ 0 at a different range of redshifts.
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spelling doaj.art-60bfbc0d520e43f299d71ce3def515d12022-12-21T18:25:19ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60441434-60522021-06-018161910.1140/epjc/s10052-021-09319-xGravitational lens time-delay as a probe of a possible time variation of the fine-structure constantL. R. Colaço0J. E. Gonzalez1R. F. L. Holanda2Departamento de Física, Universidade Federal do Rio Grande do NorteDepartamento de Física, Universidade Federal do Rio Grande do NorteDepartamento de Física, Universidade Federal do Rio Grande do NorteAbstract A new method based on large scale structure observations is proposed to probe a possible temporal variation of the fine-structure constant ( $$\alpha $$ α ). Our analyses are based on time-delay of Strong Gravitational Lensing and Type Ia Supernovae observations. By considering the runaway dilaton scenario, where the cosmological temporal evolution of the fine-structure constant is given by $$\frac{\Delta \alpha }{\alpha } \approx -\gamma \ln {(1+z)}$$ Δ α α ≈ - γ ln ( 1 + z ) , we obtain limits on the physical properties parameter of the model ( $$\gamma $$ γ ) at the level $$10^{-2}$$ 10 - 2 ( $$1\sigma $$ 1 σ ). Although our limits are less restrictive than those obtained by quasar spectroscopy, the approach presented here provides new bounds on the possibility of $$\frac{\Delta \alpha }{\alpha } \ne 0$$ Δ α α ≠ 0 at a different range of redshifts.https://doi.org/10.1140/epjc/s10052-021-09319-x
spellingShingle L. R. Colaço
J. E. Gonzalez
R. F. L. Holanda
Gravitational lens time-delay as a probe of a possible time variation of the fine-structure constant
European Physical Journal C: Particles and Fields
title Gravitational lens time-delay as a probe of a possible time variation of the fine-structure constant
title_full Gravitational lens time-delay as a probe of a possible time variation of the fine-structure constant
title_fullStr Gravitational lens time-delay as a probe of a possible time variation of the fine-structure constant
title_full_unstemmed Gravitational lens time-delay as a probe of a possible time variation of the fine-structure constant
title_short Gravitational lens time-delay as a probe of a possible time variation of the fine-structure constant
title_sort gravitational lens time delay as a probe of a possible time variation of the fine structure constant
url https://doi.org/10.1140/epjc/s10052-021-09319-x
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