Fundamental theorem on gauge fixing at the action level
arXiv:1608.00071 · doi:10.1103/PhysRevD.94.124021
Abstract
Regardless of the long history of gauge theories, it is not well recognized under which condition gauge fixing at the action level is legitimate. We address this issue from the Lagrangian point of view, and prove the following theorem on the relation between gauge fixing and Euler-Lagrange equations: In any gauge theory, if a gauge fixing is complete, i.e., the gauge functions are determined uniquely by the gauge conditions, the Euler-Lagrange equations derived from the gauge-fixed action are equivalent to those derived from the original action supplemented with the gauge conditions. Otherwise, it is not appropriate to impose the gauge conditions before deriving Euler-Lagrange equations as it may in general lead to inconsistent results. The criterion to check whether a gauge fixing is complete or not is further investigated. We also provide applications of the theorem to scalar-tensor theories and make comments on recent relevant papers on theories of modified gravity, in which there are confusions on gauge fixing and counting physical degrees of freedom.
arXiv comment25 pages; matches published version
References in corpus (29)
- Resummation of Massive Gravity
- Generalization of the Fierz-Pauli Action
- Invariant Variation Problems
- Healthy theories beyond Horndeski
- Degenerate higher derivative theories beyond Horndeski: evading the Ostrogradski instability
- Transforming gravity: from derivative couplings to matter to second-order scalar-tensor theories beyond the Horndeski Lagrangian
- Exploring gravitational theories beyond Horndeski
- On the Extra Mode and Inconsistency of Horava Gravity
- Brane World Cosmology - Gauge-Invariant Formalism for Perturbation
- Hamiltonian analysis of higher derivative scalar-tensor theories
- Unifying framework for scalar-tensor theories of gravity
- Healthy degenerate theories with higher derivatives
- Horndeski: beyond, or not beyond?
- Self-accelerating Massive Gravity: Exact solutions for any isotropic matter distribution
- Hamiltonian analysis of spatially covariant gravity
- Shortcuts to high symmetry solutions in gravitational theories
- Counting the degrees of freedom of generalized Galileons
- Canonical Quantization of Cosmological Perturbations in the One Bubble Open Universe
- The Self-Accelerating Universe with Vectors in Massive Gravity
- Hamiltonian structure of scalar-tensor theories beyond Horndeski
- Stability of the Self-accelerating Universe in Massive Gravity
- Noether Identities and Gauge-Fixing the Action for Cosmological Perturbations
- Substituting fields within the action: consistency issues and some applications
- Self-accelerating solutions in massive gravity on an isotropic reference metric
- Self-accelerating Massive Gravity: Superluminality, Cauchy Surfaces and Strong Coupling
- Self-accelerating Massive Gravity: Bimetric Determinant Singularities
- Canonical invariance of spatially covariant scalar-tensor theory
- Plugging the Gauge Fixing into the Lagrangian
- Self-accelerating Massive Gravity: Covariant Perturbation Theory
Cited by in corpus (56)
- Static response and Love numbers of Schwarzschild black holes
- Extended Cuscuton: Formulation
- Exact black hole solutions in shift-symmetric quadratic degenerate higher-order scalar-tensor theories
- Linear stability analysis of hairy black holes in quadratic degenerate higher-order scalar-tensor theories: Odd-parity perturbations
- Weakly-coupled stealth solution in scordatura degenerate theory
- General Relativity solutions in modified gravity
- General Relativity solutions with stealth scalar hair in quadratic higher-order scalar-tensor theories
- General invertible transformation and physical degrees of freedom
- Black hole solutions in shift-symmetric degenerate higher-order scalar-tensor theories
- Noether symmetries and stability of ideal gas solution in Galileon Cosmology
- A general theory of linear cosmological perturbations: stability conditions, the quasistatic limit and dynamics
- Black hole perturbations in DHOST theories: Master variables, gradient instability, and strong coupling
- Spatially covariant gravity with velocity of the lapse function: the Hamiltonian analysis
- Nonlinear definition of the shadowy mode in higher-order scalar-tensor theories
- Linear perturbation analysis of hairy black holes in shift-symmetric Horndeski theories: Odd-parity perturbations
- Built-in scordatura in U-DHOST
- Effective Field Theory for the Perturbations of a Slowly Rotating Black Hole
- Generalized disformal Horndeski theories: cosmological perturbations and consistent matter coupling
- Extended Cuscuton as Dark Energy
- Quasinormal Modes from EFT of Black Hole Perturbations with Timelike Scalar Profile
- Spontaneous scalarization of black holes in the Horndeski theory
- Generalized Regge-Wheeler Equation from Effective Field Theory of Black Hole Perturbations with a Timelike Scalar Profile
- Generalized Slow Roll in the Unified Effective Field Theory of Inflation
- Perturbations and quasi-normal modes of black holes with time-dependent scalar hair in shift-symmetric scalar-tensor theories
- Reconsidering the Ostrogradsky theorem: Higher-derivatives Lagrangians, Ghosts and Degeneracy
- Black holes with a nonconstant kinetic term in degenerate higher-order scalar tensor theories
- Linear stability of black holes in shift-symmetric Horndeski theories with a time-independent scalar field
- Linear stability of black holes with static scalar hair in full Horndeski theories: generic instabilities and surviving models
- Tidal Love Numbers from EFT of Black Hole Perturbations with Timelike Scalar Profile
- Effective description of generalized disformal theories
- Vanishing of Quadratic Love Numbers of Schwarzschild Black Holes
- Invertibility conditions for field transformations with derivatives: toward extensions of disformal transformation with higher derivatives
- Generating functional for gravitational null initial data
- Massive mimetic cosmology
- The dimensional reduction of linearized spin-2 theories invariant under transverse diffeomorphisms
- Constraining Palatini-Horndeski theory with gravitational waves after GW170817
- On the equivalence between different canonical forms of F(R) theory of gravity
- Black hole perturbations in higher-order scalar-tensor theories: initial value problem and dynamical stability
- Some disquisitions on cosmological 2-form dualities
- Theories with limited extrinsic curvature and a nonsingular anisotropic universe
- Scalar Bispectrum Beyond Slow-Roll in the Unified EFT of Inflation
- Black hole perturbation under 2 + 2 decomposition in the action
- Black hole ringdown from physically sensible initial value problem in higher-order scalar-tensor theories
- Higher order self-dual models for spin-3 particles in
- Ghost-free resummation of gravitational interactions of a 2-form gauge field
- Off-shell duality invariance of Schwarzschild perturbation theory
- Soldering spin-3 opposite helicities in
- Weyl and transverse diffeomorphism invariant spin-2 models in D=2+1
- A note on higher rank descriptions of massless and massive spin-1 particles
- Quasinormal Modes from EFT of Black Hole Perturbations in Vector-Tensor Gravity
- Self-dual models in from dimensional reduction
- Quantum wormholes at spatial infinity
- The Black Hole Window on Cosmic Inflation
- Absence of the Higuchi bound in a family of alternative linear massive spin-2 models
- Probing higher curvature gravity via ringdown with overtones
- Cosmological Lorentzian Wormholes via Noether symmetry approach