Scaling properties of the cosmic background plasma and radiation

Details Scaling properties of the cosmic background plasma and radiation Scaling properties of the cosmic background plasma and radiation

2003-05-22

arxiv.org/abs/astro-ph/0305433v1

Int.J.Mod.Phys. D12 (2003) 509-517

Astronomy and Astrophysics

Astrophysics

Scientific paper

10.1142/S0218271803003219

Scaling properties of the cosmic microwave background (CMB) radiation are studied using satellite (COBE-DMR maps), balloon-borne and ground-based (combined QMASK map) data. Quantitative consistency is found between the multiscaling properties of the COBE-DMR and QMASK CMB maps. Surprisingly, it is found that the observed CMB temperature multiscaling resembles quantitatively the multiscaling properties of fluid turbulence, that indicates primordial plasma turbulence as an origin of the CMB temperature space anisotropy.

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