Temperature Fluctuation and an Expected Limit of Hubble Parameter in the Self-Consistent Model

Details Temperature Fluctuation and an Expected Limit of Hubble Parameter in the Self-Consistent Model Temperature Fluctuation and an Expected Limit of Hubble Parameter in the Self-Consistent Model

2004-12-08

arxiv.org/abs/gr-qc/0412036v1

J.Korean Astron.Soc.39:81,2006

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

8 pages, Latex file

Scientific paper

The temperature gradient of microwave background radiation (CMBR) is calculated in the Self Consistent Model. An expected values for Hubble parameter have been presented in two different cases. In the first case the temperature is treated as a function of time only, while in the other one the temperature depends on relaxation of isotropy condition in the self-consistent model and the assumption that the universe expands adiabatically. The COBE's or WMAP's fluctuations in temperature of CMBR may be used to predict a value for Hubble parameter.

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