Einstein's General Relativity w/o Cosmological Constant

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SUMMARY

The discussion centers on Einstein's General Relativity without the cosmological constant, specifically addressing the Einstein Field Equation represented as ##G_{\mu \nu}=\kappa T_{\mu \nu}##. By setting the cosmological constant ##\Lambda=0##, the term can either be eliminated or integrated into the stress-energy tensor. This simplification leads to a clearer understanding of gravitational interactions in a vacuum without the influence of dark energy.

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  • Understanding of Einstein's Field Equations
  • Familiarity with the concepts of stress-energy tensors
  • Basic knowledge of general relativity principles
  • Mathematical proficiency in tensor calculus
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  • Study the implications of setting the cosmological constant to zero in cosmological models
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Physicists, astrophysicists, and students of theoretical physics interested in the foundations of general relativity and its applications in cosmology.

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I mean, what's "general relativity but without the cosmological constant term" (##G_{\mu \nu}=\kappa T_{\mu \nu}##) called?
 
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The Einstein Field Equation. All you've done is set ##\Lambda=0## or subsume the term into the stress-energy tensor.
 
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