Degrees of Freedom of New General Relativity I: Type 2, Type 3, Type 5, and Type 8
arXiv:2410.15056 · doi:10.1103/4ggt-6nd4
Abstract
We investigate the degrees of freedom of new general relativity. This theory is a three-parameter theory and is classified into nine irreducible types according to the rotation symmetry of on each leaf of ADM-foliation. In this work, we focus on unveiling the degrees of freedom of the physically interesting types of NGR: Type 2, Type 3, Type 5, and Type 8, which contain the gravitational propagating degrees of freedom. First, we revisit the theory based on the gauge approach to gravity and reformulate the Lagrangian of the theory. Second, we review the irreducible decomposition of the theory while focusing on the Hamiltonian and the primary constraints in each type. Third, we perform the Dirac-Bergmann analysis to unveil the degrees of freedom of the theory in the case of Type 2, Type 3, Type 5, and Type 8. We find a novel new behavior of constraints in Type 8, which is classified as second-class but not to determine any Lagrange multipliers and to provide the gauge invariance of the theory under the satisfaction of a specific condition of the multipliers. The degrees of freedom of Type 2, Type 3, and Type 5 are unveiled as six, five, and seven, respectively. The degrees of freedom of Type 8 is either four under a specific condition to the Lagrange multipliers or six in the generic case. Finally, we conclude this work with five future perspectives.
arXiv comment16 pages. arXiv admin note: text overlap with arXiv:2410.04848. v2: 16 pages, added references and comments, minor changed overlap text, for submission. v3: 18 pages, added comments on regularity of NGR in Sec.III-A and physical interpretation in Sec.III-F, minor changes, accepted in PRD
References in corpus (65)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- The Cosmological Constant and Dark Energy
- f(R) theories
- Cosmological Constant - the Weight of the Vacuum
- Introduction to Modified Gravity and Gravitational Alternative for Dark Energy
- The Cosmological Constant
- The Dynamics of General Relativity
- In the Realm of the Hubble tension a Review of Solutions
- Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM
- Large-Scale Structure of the Universe and Cosmological Perturbation Theory
- Metric-Affine Gauge Theory of Gravity: Field Equations, Noether Identities, World Spinors, and Breaking of Dilation Invariance
- Planck 2018 results. I. Overview and the cosmological legacy of Planck
- f(T) teleparallel gravity and cosmology
- H0LiCOW XIII. A 2.4% measurement of from lensed quasars: tension between early and late-Universe probes
- Coincident General Relativity
- Cosmological perturbations
- The teleparallel equivalent of general relativity
- Teleparallel Gravity: From Theory to Cosmology
- Dynamical systems applied to cosmology: dark energy and modified gravity
- Equation of state for dark energy in gravity
- An introduction to the Vainshtein mechanism
- A systematic approach to generalisations of General Relativity and their cosmological implications
- The Atacama Cosmology Telescope: DR6 Gravitational Lensing Map and Cosmological Parameters
- Infrared-modified gravities and massive gravitons
- Phases of massive gravity
- Degrees of freedom of gravity
- Covariant formulation of f(Q) theory
- Lagrange formulation of the symmetric teleparallel gravity
- Symmetric Teleparallel Gravity: Some exact solutions and spinor couplings
- Cosmological Perturbation in f(T) Gravity Revisited
- General Teleparallel Quadratic Gravity
- Hamiltonian formulation of general relativity in the teleparallel geometry
- Hamiltonian formalism for f(T) gravity
- Can late-time extensions solve the and tensions?
- Slow-roll inflation in non-metric gravity
- Hamiltonian structure of the teleparallel formulation of GR
- Local symmetries and physical degrees of freedom in gravity: a Dirac Hamiltonian constraint analysis
- Degrees of Freedom in Massive Gravity
- Review of Observational Evidence for Dark Matter in the Universe and in upcoming searches for Dark Stars
- Slow-roll inflation in f(R,T) gravity and a modified Starobinsky-like inflationary model
- BAO+BBN revisited -- Growing the Hubble tension with a 0.7km/s/Mpc constraint
- Complete dark energy scenario in gravity
- Hamiltonian and primary constraints of new general relativity
- Inflationary Cosmology: From Theory to Observations
- Perturbations in Non-Flat Cosmology for gravity
- Hamiltonian formulation of teleparallel gravity
- ADM formulation and Hamiltonian analysis of gravity
- Non-trivial Minkowski backgrounds in f(T) gravity
- Gauge symmetries of the teleparallel theory of gravity
- Cosmological perturbations in modified teleparallel gravity models: Boundary term extension
- Logamediate Inflation in f(T) Teleparallel Gravity
- Dirac-Bergmann analysis and Degrees of Freedom of Coincident -gravity
- Cosmological Perturbation Theory in Metric-Affine Gravity
- Integrated perturbation theory for cosmological tensor fields. I. Basic formulation
- Revisiting Stability in New General Relativity
- Hamilton's equations in the covariant teleparallel equivalent of general relativity
- A novel approach to autoparallels for the theories of symmetric teleparallel gravity
- Integrated perturbation theory for cosmological tensor fields. III. Projection effects
- Integrated perturbation theory for cosmological tensor fields. II. Loop corrections
- Gravitational Waves in New General Relativity
- Teleparallel bigravity
- Integrated perturbation theory for cosmological tensor fields. IV. Full-sky formulation
- On the well-posed variational principle in degenerate point particle systems using embeddings of the symplectic manifold
- A unified-description of curvature, torsion, and non-metricity of the metric-affine geometry with the Möbius representation