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Interpreting A and B metrics with Λ as gravitational field of a tachyon in an (anti–)de Sitter universe

2018/08/10 by Ondrej Hruska, Ondřej Hruška, Jiřı́ Podolský +1 · 2 citations
Mathematics · Physics and Astronomy · #Advanced Differential Geometry Research #Algorithm #Artificial intelligence #Black Holes and Theoretical Physics #Boundary (topology) #Classical mechanics #Computer science #Cosmology and Gravitation Theories #De Sitter universe #Gravitation #Mathematical analysis #Mathematical physics #Mathematics #Minkowski space #Physics #Quantum mechanics #Schwarzschild radius #Universe #gr-qc #hep-th

paper · pdf · doi:10.1103/physrevd.99.084037

published in Physical review. D/Physical review. D. 99(8) (American Physical Society) · 30 pages, 16 figures

arxiv created 2018/08/10 · openalex created_date 2018/08/22 · openalex publication_date 2019/04/18 · arxiv updated 2019/04/24 · openalex updated_date 2026/08/05

Abstract

We investigate the main properties and mutual relations of the so-called A and B metrics with any value of the cosmological constant. In particular, we explicitly show that both the AII and BI metrics are, in fact, the famous Schwarzschild--(anti--)de Sitter spacetime (that is the AI metric) boosted to superluminal speed. Together, they can be combined to form a complete gravitational field of a tachyon in an asymptotically Minkowski or (anti--)de Sitter background. The boundary separating the AII and BI regions is the Mach-Cherenkov shockwave on which the curvature is unbounded. We analyze various geometric features of such spacetimes, provide their natural physical interpretation, and visualize them using convenient background coordinates and embeddings.

Citations