Subluminal Cosmology  

Subluminal Cosmology

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作  者:Rainer Burghardt 

机构地区:[1]Independent Researcher, Obritz, Austria

出  处:《Journal of Modern Physics》2017年第4期583-601,共19页现代物理(英文)

摘  要:The standard model of cosmology is considered critically. A model with pressure is proposed which is linearly expanding and which is an exact solution of Einstein’s field equations. The recession velocity of the galaxies of this model never exceeds the speed of light. The model is closely related to the Rh=ct model of Melia, which is flat and infinite. However, our subluminal model is spatially positively curved and closed. Nevertheless all data from observations gathered and surveyed by Melia support our model.The standard model of cosmology is considered critically. A model with pressure is proposed which is linearly expanding and which is an exact solution of Einstein’s field equations. The recession velocity of the galaxies of this model never exceeds the speed of light. The model is closely related to the Rh=ct model of Melia, which is flat and infinite. However, our subluminal model is spatially positively curved and closed. Nevertheless all data from observations gathered and surveyed by Melia support our model.

关 键 词:EXPANDING COSMOS with Pressure SUBLUMINAL EXPANSION COVARIANT Representation 

分 类 号:O1[理学—数学]

 

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