Answers are grounded in this paper and cite their sources.
Chern-Simons modified gravity comprises the Einstein-Hilbert action and a higher-derivative interaction containing the Chern-Pontryagin density. We derive the analog of the Gibbons-Hawking-York boundary term required to render the Dirichlet boundary-value problem well defined. It turns out to be a boundary Chern-Simons action for the extrinsic curvature. We address applications to black hole thermodynamics.
No takes yet. Share an insight, caveat, or question.
Grumiller et al. (2008) studied this question.
Synapse has enriched 10 related papers. Consider them for comparative context: