Small Scale Fluctuations of the Microwave Background in the Quasi-Steady State Cosmology
| dc.creator | Narlikar, J. V. | |
| dc.creator | Vishwakarma, R. G. | |
| dc.creator | Burbidge, G. | |
| dc.creator | Hoyle, F. | |
| dc.date | 2001-01-31 | |
| dc.date.accessioned | 2026-07-07T01:57:34Z | |
| dc.date.available | 2026-07-07T01:57:34Z | |
| dc.description | In this paper we show that, within the framework of the QSSC, the small scale deviations on angular scales $\lesssim 1^{0}$ expected in the MBR are due to inhomogeneities in the distribution of galaxies and clusters. It is shown how these can be estimated on the galaxy-cluster-supercluster scale at the epoch of redshift $\sim 5$ when the universe was last passing through the minimum phase of the scale factor. Rich clusters on the scale of 5-10 Mpc generate the kind of peak in the fluctuation power spectrum observed by the Boomrang and Maxima projects. Weaker inhomogeneities on smaller scales with $l~\sim 10^3$ are expected to arise from individual galaxies and small groups. | |
| dc.description | LaTeX, 11 pages | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0101551 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0101551 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/2436 | |
| dc.subject | Astrophysics | |
| dc.title | Small Scale Fluctuations of the Microwave Background in the Quasi-Steady State Cosmology | |
| dc.type | text |