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Planck 2013 results. XXVII. Doppler boosting of the CMB: Eppur si muove

AutorScott, D.; Barreiro, R. Belén ; Curto, Andrés ; Diego, José María ; González-Nuevo, J. ; López-Caniego, M. ; Martínez-González, Enrique ; Rebolo López, Rafael; Toffolatti, L. ; Vielva, P. ; Planck Collaboration
Palabras claveReference systems
Relativistic processes
Cosmic background radiation
Cosmology: observations
Fecha de publicación2014
EditorEDP Sciences
CitaciónAstronomy and Astrophysics 571: A27 (2014)
ResumenOur velocity relative to the rest frame of the cosmic microwave background (CMB) generates a dipole temperature anisotropy on the sky which has been well measured for more than 30 years, and has an accepted amplitude of v/c = 1.23 × 10-3, or v = 369. In addition to this signal generated by Doppler boosting of the CMB monopole, our motion also modulates and aberrates the CMB temperature fluctuations (as well as every other source of radiation at cosmological distances). This is an order 10-3 effect applied to fluctuations which are already one part in roughly 105, so it is quite small. Nevertheless, it becomes detectable with the all-sky coverage, high angular resolution, and low noise levels of the Planck satellite. Here we report a first measurement of this velocity signature using the aberration and modulation effects on the CMB temperature anisotropies, finding a component in the known dipole direction, (l,b) = (264°,48°), of 384 km s-1 ± 78 km s-1 (stat.) ± 115 km s-1 (syst.). This is a significant confirmation of the expected velocity.
Versión del editorhttp://dx.doi.org/10.1051/0004-6361/201321556
URIhttp://hdl.handle.net/10261/110630
DOI10.1051/0004-6361/201321556
Identificadoresdoi: 10.1051/0004-6361/201321556
issn: 0004-637X
e-issn: 1432-0746
Aparece en las colecciones: (IFCA) Artículos
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