Gravitational Chern-Simons Lagrangian terms and spherically symmetric spacetimes
arXiv:1105.4792 · doi:10.1088/0264-9381/28/19/195009
Abstract
We show that for general spherically symmetric configurations, contributions of general gravitational and mixed gauge-gravitational Chern-Simons terms to the equations of motion vanish identically in dimensions. This implies that such terms in the action do not affect Birkhoff's theorem or any previously known spherically symmetric solutions. Furthermore, we investigate the thermodynamical properties using the procedure described in an accompanying paper. We find that in static spherically symmetric case Chern-Simons terms do not contribute to the entropy either. Moreover, if one requires only for the metric tensor to be spherically symmetric, letting other fields unrestricted, the results extend almost completely, with only one possible exception --- Chern-Simons Lagrangian terms in which the gravitational part is just the irreducible gravitational Chern-Simons term.
16 pages, updated to match published version
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- Quasilocal Conserved Charges with a Gravitational Chern-Simons Term
- Quasi-local conserved charges and holography
- Symmetry inheritance of scalar fields
- Black hole entropy in the Chern-Simons-like theories of gravity and Lorentz-diffeomorphism Noether charge
- Covariant Noether Charge for Higher Dimensional Chern-Simons Terms
- Symmetries and gravitational Chern-Simons Lagrangian terms
- Does three dimensional electromagnetic field inherit the spacetime symmetries?
- A new look at hidden conformal symmetries of black holes
- Generalizations and challenges for the spacetime block-diagonalization
- Stationary rotating black holes in theories with gravitational Chern-Simons Lagrangian term
- Stationary spacetimes with time-dependent real scalar fields
- Gravitational Chern-Simons terms and black hole entropy. Global aspects
- Weighing the curvature invariants
- Parity-odd surface anomalies and correlation functions on conical defects
- Symmetry Inheritance and Jebsen-Birkhoff Theorem