Horava's quantum gravity illustrated by embedding diagrams of the Kehagias-Sfetsos spacetimes

Autor(es)

Goluchova, Katerina ^[1] ; Kulczycki, Konrad ^[1] ; Vieira, Ronaldo S. S. ^{[2, 3, 4]} ; Stuchlik, Zdenek ^[1] ; Kluzniak, Wlodek ^[4] ; Abramowicz, Marek ^{[4, 1, 5]}

Afiliação do(s) autor(es)

^[1] Silesian Univ Opava, Inst Phys, Fac Philosophy & Sci, Opava 74601 - Czech Republic

^[2] Univ Estadual Campinas, Inst Fis Gleb Wataghin, BR-13083859 Campinas, SP - Brazil

^[3] Univ Sao Paulo, Inst Astron Geofis & Ciencias Atmosfer, BR-05508090 Sao Paulo, SP - Brazil

^[4] Copernicus Astron Ctr, PL-00716 Warsaw - Poland

^[5] Gothenburg Univ, Dept Phys, S-41296 Gothenburg - Sweden

• Tipo de documento: Artigo Científico
• Fonte: GENERAL RELATIVITY AND GRAVITATION; v. 47, n. 11 NOV 2015.
• Citações Web of Science: 2

Resumo

Possible astrophysical consequences of the Horava quantum gravity theory have been recently studied by several authors. They usually employ the Kehagias-Sfetsos (KS) spacetime which is a spherically symmetric vacuum solution of a specific version of Horava's gravity. The KS metric has several unusual geometrical properties that in the present article we examine by means of the often used technique of embedding diagrams. We pay particular attention to the transition between naked singularity and black-hole states, which is possible along some particular sequences of the KS metrics. (AU)

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