Distortions of the CMB by Large Voids in the Primordial Universe

Details Distortions of the CMB by Large Voids in the Primordial Universe Distortions of the CMB by Large Voids in the Primordial Universe

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998tx19.confe.576o&link_type=abstract

Abstracts of the 19th Texas Symposium on Relativistic Astrophysics and Cosmology, held in Paris, France, Dec. 14-18, 1998. Eds.:

Astronomy and Astrophysics

Astrophysics

Scientific paper

The first objects that formed had masses ~106 Modot and, after their short lives, probably ended in primordial supernova explosions, which have been shown to produce voids of galaxies <= 60h^{-1}Mpc (Miranda and Opher 1996, 1997). Due to the higher temperature of the voids, distortions of the CMB were created for spherical harmonics l >= q 200 (first acoustic peak). We investigate the distortions in the CMB, as a consequence of the formation and evolution of the voids.

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