Static spacetimes with/without black holes in dynamical Chern-Simons gravity

2013/03/25 by Tetsuya Shiromizu, Kentaro Tanabe · 19 citations
Physics and Astronomy · #Advanced Differential Geometry Research #Black Holes and Theoretical Physics #Black hole (networking) #Chern–Simons theory #Classical mechanics #Computer science #Cosmology and Gravitation Theories #Gauge theory #Mathematical physics #Minkowski space #Physics #Quantum field theory in curved spacetime #Quantum gravity #Quantum mechanics #Schwarzschild radius #Spacetime #Spherically symmetric spacetime #Stationary spacetime #gr-qc #hep-th

paper · pdf · doi:10.1103/physrevd.87.081504

published in Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields 87(8) (American Physical Society) · 3 pages

arxiv created 2013/03/25 · openalex publication_date 2013/04/23 · arxiv updated 2015/06/15 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

We show that the static and asymptotically flat black hole spacetime is unique to be Schwarzschild spacetime in the dynamical Chern-Simons gravity. In addition, we show that the strictly static spacetimes should be the Minkowski spacetime.

Citations

• How do black holes spin in Chern-Simons modified gravity?
• Proof of the positive mass theorem. II
• A new proof of the positive energy theorem
• Black hole uniqueness theorems in higher dimensional spacetimes
• Chern-Simons Modified General Relativity
• Chern-Simons modification of general relativity

Cited by

• Static black holes and strictly static spacetimes in Einstein-Gauss-Bonnet gravity with gauge field