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Gradients in the Temperature of CMBR
M. MELEK
Cairo University, Egypt.
A nonconventional approach is developed to nd the primordial
angular gradient in the temperature of the Cosmic Microwave
Background Radiation. It is found that it depends on the
nowadays recent detected value of the angular gradient in the
temperature of the CMBR, dierent rates of universe's expansion
through its dierent phases and the cosmic time period of each
phase. The obtained result is a consequence of considering the
magnitude of the angular gradient in the temperature of the
CMBR is a constant function with respect to the proper time, in
spacially perturbed FRW expanding universe.
References:
1. M.Melek, p.461- 464 in "Examining The Big Bang And Diuse
Background Radiations", edited by M.Kafatos and Y.Kondo,
Proceedings of the 168th Symposium of IAU, Kluwer Acad. Pub.,
1996.
2. M.Melek, Astrophys. and Sp. Sc., 228, 327- 330, 1995.
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