Distribution of Mass and Energy in Five General Cosmic Models

Fadel A. Bukhari^*

Department of Astronomy, Faculty of Science, King Abdulaziz University, Jeddah, KSA.

DOI: 10.4236/ijaa.2015.51004                

Abstract

Distributions of the universe horizon distance and universe horizon volume were investigated in the light of five general cosmic models which were constructed in a previous study. Both distributions increase so slowly up to t ≈ 21.5444 Myr, then they start raising very fast up to t ≈ 60 Gyr. Afterwards, they increase again very slowly until t ≈ 124 Gyr. Distributions of mass of radiation, matter and dark energy within the horizon volume of the universe were also studied in the five general cosmic models. The masses of both radiation and matter decrease gradually with time while the mass of dark energy increases. The mass of radiation prevailed in the early universe up to t ≈ 34627.5 - 55916.2 yr, where it becomes equal to the mass of matter. Then the mass of matter dominated until t ≈ 9.4525 - 10.0632 Gyr, where it becomes equal to the mass of dark energy. Thenceforward, the mass of dark energy prevails the universe. The cosmic space becomes approximately matter empty in the so far future of the universe.

Keywords

General Cosmic Models, Distribution of Mass and Energy

Conflicts of Interest

The authors declare no conflicts of interest.

References

[1]	Bukhari, F.A. (2013) Five General Cosmic Models. Journal of King Abdulaziz University: Science, 25.
[2]	Bukhari, F.A. (2013) Cosmological Distances in Five General Cosmic Models. International Journal of Astronomy and Astrophysics, 3, 183-188.