Time drift of cosmological redshifts and its variance

Jean Philippe Uzan; Francis Bernardeau; Yannick Mellier

doi:10.1103/PhysRevD.77.021301

Time drift of cosmological redshifts and its variance

Jean Philippe Uzan, Francis Bernardeau, Yannick Mellier

Research output: Contribution to journal › Article › peer-review

Abstract

The contribution of cosmological perturbations to the time drift of the cosmological redshift is derived. It is shown that the dominant correction arises from the local acceleration of both the emitter and the observer. The amplitude of this effect is estimated to be of the order of 1% of the drift signal at z=2-4, but can easily be lowered down to 0.1% by using many absorption lines and quasars.

Original language	English
Article number	021301
Journal	Physical Review D - Particles, Fields, Gravitation and Cosmology
Volume	77
Issue number	2
DOIs	https://doi.org/10.1103/PhysRevD.77.021301
Publication status	Published - 29 Jan 2008
Externally published	Yes

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10.1103/PhysRevD.77.021301

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title = "Time drift of cosmological redshifts and its variance",

abstract = "The contribution of cosmological perturbations to the time drift of the cosmological redshift is derived. It is shown that the dominant correction arises from the local acceleration of both the emitter and the observer. The amplitude of this effect is estimated to be of the order of 1\% of the drift signal at z=2-4, but can easily be lowered down to 0.1\% by using many absorption lines and quasars.",

author = "Uzan, \{Jean Philippe\} and Francis Bernardeau and Yannick Mellier",

year = "2008",

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doi = "10.1103/PhysRevD.77.021301",

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AU - Uzan, Jean Philippe

AU - Bernardeau, Francis

AU - Mellier, Yannick

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N2 - The contribution of cosmological perturbations to the time drift of the cosmological redshift is derived. It is shown that the dominant correction arises from the local acceleration of both the emitter and the observer. The amplitude of this effect is estimated to be of the order of 1% of the drift signal at z=2-4, but can easily be lowered down to 0.1% by using many absorption lines and quasars.

AB - The contribution of cosmological perturbations to the time drift of the cosmological redshift is derived. It is shown that the dominant correction arises from the local acceleration of both the emitter and the observer. The amplitude of this effect is estimated to be of the order of 1% of the drift signal at z=2-4, but can easily be lowered down to 0.1% by using many absorption lines and quasars.

U2 - 10.1103/PhysRevD.77.021301

DO - 10.1103/PhysRevD.77.021301

M3 - Article

AN - SCOPUS:38849156943

SN - 1550-7998

VL - 77

JO - Physical Review D - Particles, Fields, Gravitation and Cosmology

JF - Physical Review D - Particles, Fields, Gravitation and Cosmology

IS - 2

M1 - 021301

ER -

Time drift of cosmological redshifts and its variance

Abstract

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