Static, spherically symmetric solutions in $f(Q)$-gravity and in nonmetricity scalar-tensor theory
Nikolaos Dimakis, Petros A. Terzis, Andronikos Paliathanasis and, Theodosios Christodoulakis

TL;DR
This paper derives new static, spherically symmetric solutions in $f(Q)$ gravity and nonmetricity scalar-tensor theory, analyzing their physical properties, conservation laws, and relation to general relativity.
Contribution
It introduces novel solutions within power-law $f(Q)$ gravity and scalar-tensor theory, including the derivation of the point-like Lagrangian and conservation laws.
Findings
New solutions for static, spherically symmetric spacetimes
Analysis of physical properties and GR limit
Construction of conservation laws and analytical solutions
Abstract
We solve the gravitational field equations for a static, spherically symmetric spacetime within the framework of the symmetric teleparallel theory of gravity. Specifically, we derive new solutions within the context of power-law gravity and the nonmetricity scalar-tensor theory. For the connection in the non-coincidence gauge, we present the point-like Lagrangian that describes the employed field equations. Furthermore, we construct two conservation laws, and for different values of these conserved quantities, we analytically solve the gravitational field equations. New solutions are obtained, we investigate their physical properties and their general relativistic limit. Finally, we discuss the algebraic properties for the derived spacetimes.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsCosmology and Gravitation Theories · Geophysics and Gravity Measurements · Solar and Space Plasma Dynamics
