Astronomy and Astrophysics – Astrophysics
Scientific paper
1996-03-15
In: Cosmoparticle Physics. I. Proc. of the 1st Int. Conf. on Cosmoparticle Physics "Cosmion-94" (Moscow, 5-14 Dec. 1994), eds.
Astronomy and Astrophysics
Astrophysics
8 pages, latex, no figures
Scientific paper
Spectrum of initial scalar and tensor perturbations created during an inflationary stage producing a closed or open FRW universe now is discussed. In the closed case, the CMB temperature anisotropy ${\Delta T/T}$ generated by scalar perturbations is enhanced for low multipoles. It is argued that in the open case there is no suppression of low multipoles. A possibility of the existence of a preferred space direction in the open case is noted.
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