Spectrum of Initial Perturbations in Open and Closed Inflationary Models
| dc.creator | Starobinsky, A. A. | |
| dc.date | 1996-03-15 | |
| dc.date.accessioned | 2026-07-07T02:21:01Z | |
| dc.date.available | 2026-07-07T02:21:01Z | |
| dc.description | 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 ${ΔT/T}$ 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. | |
| dc.description | 8 pages, latex, no figures | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9603075 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9603075 | |
| dc.identifier | In: Cosmoparticle Physics. I. Proc. of the 1st Int. Conf. on Cosmoparticle Physics "Cosmion-94" (Moscow, 5-14 Dec. 1994), eds. M.Yu. Khlopov, M.E. Prokhorov, A.A. Starobinsky, J. Tran Thanh Van, Edition Frontiers, 1996, pp. 43-52. | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/10405 | |
| dc.subject | Astrophysics | |
| dc.title | Spectrum of Initial Perturbations in Open and Closed Inflationary Models | |
| dc.type | text |