Gespeichert in:
Bibliographische Detailangaben
Hauptverfasser: Saha, Dalia, Sanyal, Abhik Kumar
Format: Preprint
Veröffentlicht: 2025
Schlagworte:
Online-Zugang:https://arxiv.org/abs/2503.04551
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
_version_ 1866913722313736192
author Saha, Dalia
Sanyal, Abhik Kumar
author_facet Saha, Dalia
Sanyal, Abhik Kumar
contents The `Generalized Symmetric Teleparallel Gravity' (GSTG) does not admit diffeomorphic invariance, since the auxiliary field as well as the shift vector act as non-propagating dynamical variables carrying 1/2 degrees of freedom each. We show that in a minisuperspace model, which is devoid of the shift vector, the problem is alleviated for locally Lorentz invariant GSTG theory, and diffeomorphic invariance is established at least for one connection. However, the eerie structure of the Hamiltonian constructed even in the background of spatially flat isotropic and homogeneous Robertson-Walker space-time, can not be maneuvered. In contrast, the other two spatially flat connections containing an arbitrary time dependent function, doesn't admit non-linear extension to `Symmetric Teleparallel Equivalent to General Relativity (STEGR). We therefore construct the phase-space structure with three different spatially flat connections for the `Lorentz invariant' linear-scalar-vector-tensor GSTG action. Diffeomorphic invariance is established and the associated Hamiltonians are found to be well behaved for all the three cases.
format Preprint
id arxiv_https___arxiv_org_abs_2503_04551
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Phase space structure of symmetric teleparallel theory of gravity
Saha, Dalia
Sanyal, Abhik Kumar
General Relativity and Quantum Cosmology
The `Generalized Symmetric Teleparallel Gravity' (GSTG) does not admit diffeomorphic invariance, since the auxiliary field as well as the shift vector act as non-propagating dynamical variables carrying 1/2 degrees of freedom each. We show that in a minisuperspace model, which is devoid of the shift vector, the problem is alleviated for locally Lorentz invariant GSTG theory, and diffeomorphic invariance is established at least for one connection. However, the eerie structure of the Hamiltonian constructed even in the background of spatially flat isotropic and homogeneous Robertson-Walker space-time, can not be maneuvered. In contrast, the other two spatially flat connections containing an arbitrary time dependent function, doesn't admit non-linear extension to `Symmetric Teleparallel Equivalent to General Relativity (STEGR). We therefore construct the phase-space structure with three different spatially flat connections for the `Lorentz invariant' linear-scalar-vector-tensor GSTG action. Diffeomorphic invariance is established and the associated Hamiltonians are found to be well behaved for all the three cases.
title Phase space structure of symmetric teleparallel theory of gravity
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2503.04551