Parameters of the ultrastable expansive nondecelerative universe

Details Parameters of the ultrastable expansive nondecelerative universe Parameters of the ultrastable expansive nondecelerative universe

May 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.215..137s&link_type=abstract

Astrophysics and Space Science, vol. 215, no. 1, p. 137-147

Astronomy and Astrophysics

Astrophysics

2

Big Bang Cosmology, Cosmic Noise, Deviation, Expansion, Cosmic Background Explorer Satellite, Gravitational Fields, Microwave Radiometers

Scientific paper

The measurement of the temperature of the cosmic microwave background radiation (CMBR) with the Far InfraRed Absolute Spectrophotometer (FIRAS) on the Cosmic Background Explorer (COBE) satellite gives a possibility for determination of all mutually related parameters of the ultrastable expansive nondecelerative Universe (ENU) with deviations smaller than 0.4%. The measurement of the large-scale anisotropy of the CMBR with the Differential Microwave Radiometers (DMR) on the COBE satellite allows us to determine the mass density of gravitationally bound systems of large-scale structures of the ENU.

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