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Response to a critique of "Cotton Gravity"
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We address in this article the criticism in a recently submitted article by Clement and Noiucer (arXiv:2312.17662 [gr-qc]) on "Cotton Gravity" (CG), a gravity theory alternative to General Relativity. These authors claim that CG is "not predictive" for producing "too many" spherically symmetric vacuum solutions, while taking the Bianchi I vacuum as test case they argue that geometric constraint on the Cotton tensor lead to an undetermined problem, concluding in the end that CG "is not a physical theory". We provide arguments showing that this critique is incorrect and misrepresents the theory.
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Cited by 4 Pith papers
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Thermodynamic formulation of Cotton gravity in the Codazzi parametrization
Horizon entropy in Cotton gravity is Bekenstein-Hawking plus a Codazzi correction whose sign diagnoses ordinary, vacuum, or phantom matter content.
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Generalized Vaidya Spacetime in Cotton and Conformal Killing Theories
Cotton Gravity and Conformal Killing Gravity are shown to admit generalized Vaidya solutions with extra geometric r-squared and r-cubed terms, but several displayed formulas have internal inconsistencies.
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Black Hole Thermodynamics in Harada's inspired theory of gravity: Stability, Phase Structure and Geometrothermodynamics
In Conformal Killing Gravity, the extra λ term changes black hole stability, heat capacity, and thermodynamic curvature, creating phase structures absent from general relativity.
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Non-Vacuum Solutions in Cotton Theory
Cotton theory admits generalized Kiselev and Dymnikova black hole metrics that add geometric linear and quadratic terms to the known general-relativistic solutions.
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