On Doppler tracking in cosmological spacetimes

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dc.creatorCarrera, Matteo
dc.creatorGiulini, Domenico
dc.date2006-05-12
dc.date2006-11-20
dc.date.accessioned2026-07-07T07:09:43Z
dc.date.available2026-07-07T07:09:43Z
dc.descriptionWe give a rigorous derivation of the general-relativistic formula for the two-way Doppler tracking of a spacecraft in Friedmann-Lemaitre-Robertson-Walker and in McVittie spacetimes. The leading order corrections of the so-determined acceleration to the Newtonian acceleration are due to special-relativistic effects and cosmological expansion. The latter, although linear in the Hubble constant, is negligible in typical applications within the Solar System.
dc.description10 pages, 1 figure. Journal version
dc.identifierhttps://arxiv.org/abs/gr-qc/0605078
dc.identifierhttp://arxiv.org/abs/gr-qc/0605078
dc.identifierClass.Quant.Grav. 23 (2006) 7483-7492
dc.identifierdoi:10.1088/0264-9381/23/24/019
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/111180
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.subjectSpace Physics
dc.titleOn Doppler tracking in cosmological spacetimes
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