Phase space structure of symmetric teleparallel theory of gravity

Abstract 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, doesʼnt 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.

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Publication Details

Journal
Classical and Quantum Gravity
Published
2024-12-19
DOI
https://doi.org/10.1088/1361-6382/ada197
Citations
3
Primary Topic
Cosmology and Gravitation Theories
Type
article
Field-Weighted Citation Impact
0.99
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article

Phase space structure of symmetric teleparallel theory of gravity

Abhik Kumar Sanyal, Dalia Saha
3 citations
Classical and Quantum Gravity
Cosmology and Gravitation Theories
0.99
article

Phase space structure of symmetric teleparallel theory of gravity

Abhik Kumar Sanyal, Dalia Saha
article en
3 citations

Abstract

Abstract 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, doesʼnt 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.

Classical and Quantum GravityVol. 42(3)
Saha Institute of Nuclear Physics (IN), Murshidabad Medical College and Hospital (IN), University of Kalyani (IN)
Peace, Justice and strong institutions
Openalex Percentile: Top 22%
Cosmology and Gravitation Theories
0.99
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Phase space structure of symmetric teleparallel theory of gravity — Abhik Kumar Sanyal, Dalia Saha · Classical and Quantum Gravity (2024) | TGRS Research Map | TGRS