Generalized Noether symmetry in f(T) gravity
H. Mohseni Sadjadi

TL;DR
This paper applies generalized Noether symmetry to f(T) gravity to determine the form of the function f(T) and explores its implications for cosmic acceleration.
Contribution
It introduces a method using generalized Noether theorem with vector fields to find specific forms of f(T) in teleparallel gravity.
Findings
Derived explicit forms of f(T) consistent with symmetry
Explored cosmological implications of the obtained f(T) models
Provided a symmetry-based approach to modified gravity theories
Abstract
We consider modified teleparallel gravity, (f(T) gravity), as a framework to explain the present accelerated expansion of the universe. The matter component is assumed to be cold dark matter. To find the explicit form of the function , we utilize generalized Noether theorem and use generalized vector fields as variational symmetries of the corresponding Lagrangian. We study the cosmological consequences of the obtained results.
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.
