The Local Bubble Effects on the Cosmic Background Radiation

Physics – Plasma Physics

Scientific paper

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Cosmic Background Explorer Satellite, Bubbles, Anisotropy, Background Radiation, Spatial Distribution, Cosmic Rays, Dust, Milky Way Galaxy, Quadrupoles, Variations

Scientific paper

Temperature fluctuations delta T/T approximately equals 10-5 have been detected by the COBE team and also by other missions (RELICT, Tenerife) in the cosmic microwave background radiation (CMBR) over angular scales larger than 7 deg corresponding to linear sizes of approximately 1000 h-1 Mpc (for 0.5 is less than or equal to h is less than or equal to 1). These residual fluctuations become evident on the CMBR maps after subtracting out the known dipole and quadrupole contributions to anisotropy produced by the peculiar motion of the observer with respect to the local standard of rest and to the Milky Way. The pattern of the fluctuations does not spatially correlate with known extragalactic source distributions. Furthermore, spatially correlated Galactic free-free and dust emission cannot mimic either the spectrum or the spatial distribution of the fluctuations. The residual fluctuations are interpreted as the signatures of the primordial density/gravitational fluctuations imprinted at the recombination era, about 300,000 years after the big bang, through the Sachs-Wolf effect. Recently, Gouveia Dal Pino et al. have shown that the COBE temperature fluctuations can be fitted by a fractal distribution with a fractal dimension D=1.43 plus or minus 0.07.

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