Barbero-Immirzi field in canonical formalism of pure gravity
arXiv:0902.0957 · doi:10.1103/PhysRevD.79.084004
Abstract
The Barbero-Immirzi (BI) parameter is promoted to a field and a canonical analysis is performed when it is coupled with a Nieh-Yan topological invariant. It is shown that, in the effective theory, the BI field is a canonical pseudoscalar minimally coupled with gravity. This framework is argued to be more natural than the one of the usual Holst action. Potential consequences in relation with inflation and the quantum theory are briefly discussed.
10 pages
References in corpus (6)
- The Barbero-Immirzi Parameter as a Scalar Field: K-Inflation from Loop Quantum Gravity?
- Topological Interpretation of Barbero-Immirzi Parameter
- From the Einstein-Cartan to the Ashtekar-Barbero canonical constraints, passing through the Nieh-Yan functional
- Fermions in Loop Quantum Cosmology and the Role of Parity
- Superconducting loop quantum gravity and the cosmological constant
- Quantum gravity as a Fermi liquid
Cited by in corpus (36)
- Horizon-scale tests of gravity theories and fundamental physics from the Event Horizon Telescope image of Sagittarius A
- Extreme- and Intermediate-Mass Ratio Inspirals in Dynamical Chern-Simons Modified Gravity
- Testing gravitational parity violation with coincident gravitational waves and short gamma-ray bursts
- Interaction of the Barbero--Immirzi Field with Matter and Pseudo-Scalar Perturbations
- Testing Chern-Simons Modified Gravity with Gravitational-Wave Detections of Extreme-Mass-Ratio Binaries
- Peccei--Quinn mechanism in gravity and the nature of the Barbero--Immirzi parameter
- Polarized primordial gravitational waves in the ghost-free parity-violating gravity
- Coupling Metric-Affine Gravity to a Higgs-Like Scalar Field
- Big-bounce and future time singularity resolution in Bianchi I: the projective invariant Nieh-Yan case
- Tensor non-Gaussianity in chiral scalar-tensor theories of gravity
- Matter matters in Einstein-Cartan gravity
- Holographic Dark Energy Models and Higher Order Generalizations in Dynamical Chern-Simons Modified Gravity
- Seeking the Loop Quantum Gravity Barbero-Immirzi Parameter and Field in 4D, = 1 Supergravity
- Scale and Weyl Invariance in Einstein-Cartan Gravity
- I-Love-Q Relations for Neutron Stars in dynamical Chern Simons Gravity
- Big-Bounce cosmology in the presence of Immirzi field
- Coupling Metric-Affine Gravity to the Standard Model and Dark Matter Fermions
- Torsion in string-inspired cosmologies and the universe dark sector
- Dark matter candidate from torsion
- Super-entropic black hole with Immirzi hair
- Generation of gravitational waves in dynamical Chern-Simons gravity
- The Immirzi parameter from an external scalar field
- The real Chern-Simons wave function
- Torsion at different scales: from materials to the Universe
- Dimensionless physics: continuation
- Quantum cosmology of a dynamical Lambda
- Resonant gravitational waves in dynamical Chern-Simons-axion gravity
- The Barbero-Immirzi Parameter: An Enigmatic Parameter of Loop Quantum Gravity
- Gauge invariant coupling of fields to torsion: a string inspired model
- Slow-rotating charged black hole solution in dynamical Chern-Simons modified gravity
- Mimetic-Metric-Torsion with induced Axial mode and Phantom barrier crossing
- Squeezed gravitons from superradiant axion fields around rotating black holes
- Breaking parity: the case of the trispectrum from chiral scalar-tensor theories of gravity
- Quantum-Ordering Ambiguities in Weak Chern-Simons 4D Gravity and Metastability of the Condensate-Induced Inflation
- Geometric Baryogenesis with Chiral-Time Equivalence
- New effective theories of gravitation and their phenomenological consequences