Regresar

Kerr-de Sitter black hole revisited

Abstract:

We interpret the cosmological constant as the energy of the vacuum, and under a minimum amount of assumptions, we show that it is deformed in the vicinity of a black hole. This leads us to reexamine the Kerr-de Sitter solution. We provide a new solution, simpler and geometrically richer, which shows the impact of the rotation in form of a warped curvature. We carry out a detailed and exact study on the new black hole solution, and we conclude with a conjecture regarding the possible impact of our results on alternative theories.

Año de publicación:

2021

Keywords:

    Fuente:

    scopusscopus

    Tipo de documento:

    Article

    Estado:

    Acceso restringido

    Áreas de conocimiento:

    • Gravedad
    • Física

    Áreas temáticas:

    • Cuerpos y fenómenos celestes específicos

    Contribuidores:

    Stuchlik Z.Stuchlik Z.
    Ovalle J.Ovalle J.
    Ernesto ContrerasErnesto Contreras