engleski

Gravitational Chern-Simons terms in D>3

I’ll talk about the consequences of adding the gravitational Chern-Simons terms to existing covariant action (e.g. to Einstein-Hilbert) in certain D>3 cases. In particular about the consequences on the solutions, black hole solutions, the definition and the value of the black hole entropy.

Chern-Simons gravity

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