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    Planck 2013 results. XXIII. Isotropy and statistics of the CMB

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    Planck2013ResultsXXI ... (7.826Mb)
    Identificadores
    URI: http://hdl.handle.net/10902/9541
    DOI: 10.1051/0004-6361/201321534
    ISSN: 0004-6361
    ISSN: 1432-0746
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    Autoría
    Ade, Peter Anthony Robert; Barreiro Vilas, Rita BelénAutoridad Unican; Bonavera, Laura; Curto Martín, Andrés; Diego Rodríguez, José MaríaAutoridad Unican; González-Nuevo González; Joaquín; Herranz Muñoz, DiegoAutoridad Unican; López-Caniego Alcarria, Marcos; Martínez González, Enrique; Toffolatti, Luigi; Vielva Martínez, PatricioAutoridad Unican; Cruz Rodríguez, MarcosAutoridad Unican
    Fecha
    2014-11
    Derechos
    © 2014 ESO
    Publicado en
    Astronomy & Astrophysics, 2014, 571, A23
    Editorial
    EDP Sciences
    Enlace a la publicación
    https://doi.org/10.1051/0004-6361/201321534
    Resumen/Abstract
    The two fundamental assumptions of the standard cosmological model-that the initial fluctuations are statistically isotropic and Gaussian-are rigorously tested using maps of the cosmic microwave background (CMB) anisotropy from the Planck satellite. The detailed results are based on studies of four independent estimates of the CMB that are compared to simulations using a fiducial ΛCDM model and incorporating essential aspects of the Planck measurement process. Deviations from isotropy have been found and demonstrated to be robust against component separation algorithm, mask choice, and frequency dependence. Many of these anomalies were previously observed in the WMAP data, and are now confirmed at similar levels of significance (about 3σ). However, we find little evidence of non-Gaussianity, with the exception of a few statistical signatures that seem to be associated with specific anomalies. In particular, we find that the quadrupole-octopole alignment is also connected to a low observed variance in the CMB signal. A power asymmetry is now found to persist on scales corresponding to about â.," = 600 and can be described in the low-â.," regime by a phenomenological dipole modulation model. However, any primordial power asymmetry is strongly scale-dependent and does not extend to arbitrarily small angular scales. Finally, it is plausible that some of these features may be reflected in the angular power spectrum of the data, which shows a deficit of power on similar scales. Indeed, when the power spectra of two hemispheres defined by a preferred direction are considered separately, one shows evidence of a deficit in power, while its opposite contains oscillations between odd and even modes that may be related to the parity violation and phase correlations also detected in the data. Although these analyses represent a step forward in building an understanding of the anomalies, a satisfactory explanation based on physically motivated models is still lacking.
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    UNIVERSIDAD DE CANTABRIA

    Repositorio realizado por la Biblioteca Universitaria utilizando DSpace software
    Contacto | Sugerencias
    Metadatos sujetos a:licencia de Creative Commons Reconocimiento 4.0 España