Generalized Einstein theory with fundamental cosmological stress tensor
Arlen Anderson

TL;DR
This paper generalizes Einstein's theory by incorporating a cosmological stress tensor, derived through variational principles and diffeomorphism restrictions, interpreting gravity as a cosmological fluid.
Contribution
It introduces a new generalized Einstein theory that includes a cosmological stress tensor based on variational principles and symmetry restrictions.
Findings
Derivation of a generalized Einstein equation with a cosmological stress tensor
Interpretation of gravity as a cosmological fluid
Field equations correspond to the stress tensor of the theory
Abstract
Careful analysis of parametrized variational principles in mechanics and field theory leads to a generalization of Einstein theory that includes a cosmological stress tensor. This generalization also follows by restricting variations of the metric in the Hilbert action to spacetime diffeomorphisms. The equation of motion for the generalized theory is the twice-contracted Bianchi identity while the field equations constitute the stress tensor of the theory. Gravity is interpreted as a cosmological fluid.
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Taxonomy
TopicsCosmology and Gravitation Theories · Relativity and Gravitational Theory · Black Holes and Theoretical Physics
