Home » 2013 Volume 8, 3. Relativity and gravitation, 4. Astrophysics, 5. Cosmology » TPAC: 4488-029 v2, Vol. 8, p. 16–23

The frequency and intensity stasis effects for radiation crossed galaxy clusters.

2. Isotropy and anisotropy of CMB

 Zahid Zakir [1]


     In the previous two papers it has been studied a new class of general relativistic effects – the frequency and intensity stasis of radiation crossing gravitationally-bound regions (GBRs), such as galaxy clusters, due to switching out from the cosmological expansion flow. In the present paper the theory of stasis effects is applied to cosmic microwave background (CMB). For a part of CMB crossing a cluster these effects lead to the stasis of its temperature and «heating» w.r.t. a normally expanded flow outside the cluster. As a result, instead of former paradigm about almost sterile propagation of CMB from the recombination epoch, in fact, general relativity and cosmological principle lead to the opposite picture. Mixing of flows of relic photons, repitedly isolated many times from expansion flow in GBRs along their path, sufficienly changes the physical characteristics of CMB, particularly, leads to its isotropy and loss of earlier times perturbations. The observing anisotropy follows from the stasis effects at crossing of multiple layers of clusters at our nearest environment.

PACS: 98.80.Es, 97.60.Bw, 98.65.Cw, 98.62.Py, 98.62.Ck, 98.62.Qz, 98.80.Jk, 98.70.Vc

Key words: cosmology, galaxy clusters, gravitation, background radiation, anisotropy  

Vol. 8, No 1, p. 16 –23, v1,  15 April 2013

Online: TPAC: 4488-029 v1,   15 April 2013; DOI: 10.9751/TPAC.4488-029

[1] Centre for Theoretical Physics and Astrophyics, Tashkent, Uzbekistan



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