Primordial Angular Gradients In The Temperature Of The CMBR And The Density Fluctuations

Details Primordial Angular Gradients In The Temperature Of The CMBR And The Density Fluctuations Primordial Angular Gradients In The Temperature Of The CMBR And The Density Fluctuations

Sep 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002ap%26ss.281..743m&link_type=abstract

Astrophysics and Space Science, v. 281, Issue 4, p. 743-750 (2002).

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

A non-conventional approach is developed and used to find the primordial angular gradient, anisotropy, of the temperature of the Cosmic Microwave Background \underline{R}adiation (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.

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