On the Exterior Solution of Spherically Symmetric Stationary Space-time in a Vector-tensor Gravity | Chapter 2 | Current Perspective to Physical Science Research Vol. 5

 In this place chapter vector-tensor (VT) hypotheses are studied evolving the stationary spherically symmetric resolution. In the absence of matter content, the answer obtained is similar to the Reissner-Nordström-de Keeper one of Approximate Relativity, but the role of the energetic charge is played by few parameters related to the VT hypothesis. Blackhole and cosmological horizons are also intentional. A deviation of the sweep of the VT black hole horizon concerning the Kottler-Schwazschild-de Sitter individual is found. Finally, from a study of the border conditions it is raise that the cosmological constant appears in a organic way from these heading-tensor theories.

Author(s) Details:

Roberto Dale,
Departament d’Estadística, Matemàtica i Informàtica and Centre of Operations Research (CIO), Universidad Miguel Hernández, 03202 Elx, Spain.

Màrius J. Fullana,
Institut de Matemàtica Multicisciplinària, Universitat Politècnica de València, 46022 València, Spain.

Alicia Herrero,
Institut de Matemàtica Multicisciplinària, Universitat Politècnica de València, 46022 València, Spain.

Please see the link here: https://stm.bookpi.org/CPPSR-V5/article/view/12909