6533b827fe1ef96bd12871e4
RESEARCH PRODUCT
The roughness of the last scattering surface
J. L. SanzVicent J. MartínezSilvestre ParedesJose M. DiegoEnrique Martínez-gonzálezSilvia MollerachSilvia Mollerachsubject
Normalization (statistics)PhysicsSpectral indexScatteringCosmic microwave backgroundAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsSurface finishAstrophysicsAstrophysicsOmegaAmplitudeSpace and Planetary ScienceAtomic physicsAnisotropydescription
We propose an alternative analysis of the microwave background temperature anisotropy maps that is based on the study of the roughness of natural surfaces. We apply it to large angle anisotropies, such as those measured by COBE-DMR. We show that for a large signal to noise experiment, the spectral index can be determined independently of the normalization. We then analyze the 4 yr COBE map and find for a flat $\Omega=1$ universe, that the best-fitting value for the spectral index is $n = 1.15^{+0.39}_{-0.34}$ and for the amplitude $Q_{rms-PS}= 14.1^{+3.9}_{-3.5}\mu K$. For $n=1$, the best-fitting normalization is $Q_{rms-PS}|_{n=1}= 16.2^{+1.4}_{-1.3}\mu K$.
year | journal | country | edition | language |
---|---|---|---|---|
1999-06-22 |