Energy in Topologically Massive Gravity
S. Deser, Bayram Tekin
TL;DR
This paper defines and verifies conserved gravitational charges in topologically massive gravity with a cosmological constant, providing a surface integral formulation applicable to de-Sitter and flat vacua.
Contribution
It introduces a new method to compute conserved charges in topologically massive gravity with cosmological extension, verified on key solutions.
Findings
Conserved charges are expressed as surface integrals.
Verification on de-Sitter and flat vacua solutions.
Consistency with known solutions confirmed.
Abstract
We define conserved gravitational charges in -cosmologically extended- topologically massive gravity, exhibit them in surface integral form about their de-Sitter or flat vacua and verify their correctness in terms of two basic types of solution.
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