Primordial Angular Gradients In The Temperature Of The CMBR And The Density Fluctuations |
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| Authors: | M Melek |
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| Institution: | (1) Astronomy And Meteorology Department, Faculty of Science, Cairo University, Orman, Giza, Egypt |
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| Abstract: | A non-conventional approach is developed and used to find the primordial angular gradient, anisotropy, of the temperature
of the Cosmic Microwave Background Radiation (CMBR), as well as the density fluctuations in an adiabatic expanding universe.
The obtained results is a consequence of considering the magnitude of the angular gradient of the temperature of the CMBR
as a constant function with respect to the proper time of the spatially perturbed FRW expanding universe.
This revised version was published online in July 2006 with corrections to the Cover Date. |
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