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Induced gravitational topological term and the Einstein-Cartan modified theory
General Relativity and Quantum Cosmology · Submitted 12 Aug 2021
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim However, in particular, we find a non-trivial solution where the modified field equations do not reduce to the GR ones.
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The abstract, sentence by sentence
It is well known that only the axial piece of the torsion couples minimally to fermions in a Riemann-Cartan geometry, while the other ones decouple. In this paper, we consider the Dirac field minimally coupled to a dynamical background with torsion and compute its contribution to the fermionic one-loop effective action. Such a contribution owns topological nature since it can be linked with topological invariants from Riemann-Cartan spaces, like Nieh-Yan and Chern-Simons terms. Furthermore, we propose a novel modified theory of gravity constructed by adding the aforementioned one-loop contribution to the Einstein-Cartan action. The modified field equations reduce to those ones of GR under certain circumstances, providing therefore trivial solutions. However, in particular, we find a non-trivial solution where the modified field equations do not reduce to the GR ones.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | It is well known that only the axial piece of the torsion couples minimally to fermions in a Riemann-Cartan geometry, while the other ones decouple. | background 1.00 | 0.03 | 0.03 | asserted 1.00 |
| s1 | In this paper, we consider the Dirac field minimally coupled to a dynamical background with torsion and compute its contribution to the fermionic one-loop effective action. | contribution 0.86 | 0.95 | 0.04 | asserted 0.96 |
| s2 | Such a contribution owns topological nature since it can be linked with topological invariants from Riemann-Cartan spaces, like Nieh-Yan and Chern-Simons terms. | interpretation 0.52 | 0.71 | 0.11 | asserted 0.98 |
| s3 | Furthermore, we propose a novel modified theory of gravity constructed by adding the aforementioned one-loop contribution to the Einstein-Cartan action. | contribution 0.99 | 0.93 | 0.25 | asserted 0.98 |
| s4 | The modified field equations reduce to those ones of GR under certain circumstances, providing therefore trivial solutions. | result 0.94 | 0.79 | 0.08 | asserted 0.97 |
| s5 | However, in particular, we find a non-trivial solution where the modified field equations do not reduce to the GR ones. | result 1.00 | 0.96 | 0.51 | asserted 1.00 |
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The paper
Original abstract
It is well known that only the axial piece of the torsion couples minimally to fermions in a Riemann-Cartan geometry, while the other ones decouple. In this paper, we consider the Dirac field minimally coupled to a dynamical background with torsion and compute its contribution to the fermionic one-loop effective action. Such a contribution owns topological nature since it can be linked with topological invariants from Riemann-Cartan spaces, like Nieh-Yan and Chern-Simons terms. Furthermore, we propose a novel modified theory of gravity constructed by adding the aforementioned one-loop contribution to the Einstein-Cartan action. The modified field equations reduce to those ones of GR under certain circumstances, providing therefore trivial solutions. However, in particular, we find a non-trivial solution where the modified field equations do not reduce to the GR ones.
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References
How the literature uses it
5 arXiv papers cite this in 6 sentences
Papers citing it · 5 sentences without a confident label
Cites it as background 1 paper
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Nevertheless, exploring broader geometric frameworks, such as the inclusion of topological terms in a Riemann-Cartan setting [ref] .
Semi-Analytic Trajectory Analysis of Light in Generic Static Spacetimes · Example 2: Schwarzschild-like metric in metric-affine bumblebee gravity · 0.85
What it cites · 24 sentences without a confident label
Uses the method or tool of 1 paper
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Upon carrying out the trace over the Dirac gamma matrices and integration over the proper time $s$ (the step-by-step calculation can be made similarly to [ref] ), we obtain the first contribution to the desired effective action: Γ_NY,2 = 1/216π^2∫d^4x√(-g) ϵ^μνλρS_μ∂_νω̃_λabω̃_ρ^ab.
Lorentz violation and the proper-time method · ONE-LOOP INDUCED GRAVITATIONAL TOPOLOGICAL TERM · 0.96
Compares with 4 papers
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Apart from that, the divergence of Eq. ([ref]) imposes another constraint or consistency condition to hold the diffeomorphism invariance of the modified theory [equation] which is somewhat similar to the Pontryagin constraint in CSMGR [ref] .
Chern-Simons Modification of General Relativity · EINSTEIN-CARTAN MODIFIED THEORY WITH ADDITIVE TOPOLOGICAL TERM · 0.96
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In particular, Schwarzschild metric persists as a solution of our EC modified theory, in contrast to the modified theory proposed in [ref] .
Einstein-Cartan formulation of Chern-Simons Lorentz-violating Gravity · EINSTEIN-CARTAN MODIFIED THEORY WITH ADDITIVE TOPOLOGICAL TERM · 0.99
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It is worth to mention that this novel contact term resembles the interaction term proposed within the non-dynamical version of CSMGR [ref] , with the axial-vector torsion background field playing the role of the axial vector field $v_μ$ defined in those papers.
Chern-Simons Modified General Relativity · ONE-LOOP INDUCED GRAVITATIONAL TOPOLOGICAL TERM · 1.00
Cites as background 9 papers
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The tensor $X_μν$ is sometimes called the Cotton tensor [ref] .
Chern-Simons Modification of General Relativity · EINSTEIN-CARTAN MODIFIED THEORY WITH ADDITIVE TOPOLOGICAL TERM · 0.80
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First, let us begin exhibiting the Dirac action minimally coupled to gravity and torsion in a Riemann-Cartan background [ref] [equation] where $γ^a$ is the usual flat-space Dirac matrices and $e^a_ μ$ is the vierbein field.
Topological Invariants, Instantons and Chiral Anomaly on Spaces with Torsion · Fermions in a Riemann-Cartan space · 0.90
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First, let us begin exhibiting the Dirac action minimally coupled to gravity and torsion in a Riemann-Cartan background [ref] [equation] where $γ^a$ is the usual flat-space Dirac matrices and $e^a_ μ$ is the vierbein field.
Physical Aspects of the Space-Time Torsion · Fermions in a Riemann-Cartan space · 0.90
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