2013/02/13 by Tetsuya Shiromizu, Seiju Ohashi
Physics and Astronomy · #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #Einstein #Gauss–Bonnet theorem #Mathematical physics #Physics #Relativity and Gravitational Theory #Theoretical physics #gr-qc #hep-th
paper · pdf · doi:10.1103/physrevd.87.087501
published as Phys.Rev.D87:087501,2013 · 3 pages
arxiv created 2013/02/13 · openalex publication_date 2013/04/02 · arxiv updated 2015/10/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
In the Einstein gravity, it is well known that strictly stationary and vacuum regular spacetime should be the Minkowski spacetime. In the Einstein-Gauss-Bonnet theory, we shall show that strictly static (no event horizon), vacuum, and asymptotically flat spacetimes with conformally static slices are the Minkowski spacetime when the curvature corrections are small.