Static Solutions with Spherical Symmetry in f(T) Theories
By Tower Wang. 2011
166 citations recorded by the source corpus.
The spherically symmetric static solutions are searched for in some $f(T)$ models of gravity theory with a Maxwell term. To do this, we demonstrate that reconstructing the Lagrangian of $f(T)$ theories is sensitive to the choice of frame, and then we introduce a particular frame based on the conformally Cartesian coordinates. In this particular frame, the existence conditions of various solutions are presented. Our results imply that only a limited class of $f(T)$ models can be solved in this frame. For more general models, the search for spherically symmetric static solutions is still an open and challenging problem, hopefully solvable in other frames.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/26c2777130ca48fce6cccef3896f899dd3591d86
How researchers see this paper
The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.
In Astronomy and Astrophysics
- Emmanuel N. Saridakis
- M. De Laurentis
- Salvatore Capozziello
- Yi-Fu Cai
- Chao-Qiang Geng
- Chung-Chi Lee
- Sergei D. Odintsov
- Lorenzo Iorio
In Nuclear and High Energy Physics
- Emmanuel N. Saridakis
- M. De Laurentis
- Salvatore Capozziello
- Yi-Fu Cai
- Chao-Qiang Geng
- Chung-Chi Lee
- Lorenzo Iorio
- Sergei D. Odintsov
Citations in the corpus
- Solar system constraints on f(T) gravity (2012, background): “…Setare & Houndjo (2012), Liuet al. (2012), Wu & Yu (2010b), Bengochea (2011), Gonzalez et al. (2012), Daouda et al. (2011), Daouda et al. (2012a), Boehmeret al (2011), Daouda et al. (2012b), Ferraro & Fiorini (2011c), Wang (2011), Miao et al. (2011), Wei et al (2012), Ferraro & Fiorini (2011b)).”
- Teleparallel theories of gravity: illuminating a fully invariant approach (2018, unknown): “[78] T.”
- f(T) teleparallel gravity and cosmology (2015, methodology): “We stress that, in this way, we obtain new solutions, that could not be obtained by the standard methods applied in [264, 265, 459, 522, 538].”
- Observational constraints on teleparallel dark energy (2011, background): “The first is to replace T by an arbitrary function f(T ) [41, 42, 46–72], similar to f(R) extensions of GR, and obtain new interesting terms in the field equations.”