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Cosmology

  • Ermis MitsouEmail author
Chapter
Part of the Springer Theses book series (Springer Theses)

Abstract

Here we work in \(D=4\) and consider the background cosmology of the action-based \(\xi \)-MM model ( 4.4.15) and the projector-based \(\xi \)-M model ( 4.4.10). This chapter is based on, and extends, (Foffa et al., Int. J. Mod. Phys. A 29:1450116, 2014 [1]), (Dirian and Mitsou, JCAP 10:065, 2014 [2]).

Keywords

Dark Energy Friedmann Equation Dark Energy Component Modify Friedmann Equation Effective Dark Energy 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Springer International Publishing Switzerland 2016

Authors and Affiliations

  1. 1.Department of Physics, Institute for Strings, Cosmology and Astroparticle PhysicsColumbia UniversityNew YorkUSA

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