The Effective Field Theory of Vector-Tensor Theories
arXiv:2111.08119 · doi:10.1088/1475-7516/2022/01/059
Abstract
We investigate a systematic formulation of vector-tensor theories based on the effective field theory (EFT) approach. The input of our EFT is that the spacetime symmetry is spontaneously broken by the existence of a preferred timelike direction in accordance with the cosmological principle. After clarifying the difference of the symmetry breaking pattern from the conventional EFT of inflation/dark energy, we find an EFT description of vector-tensor theories around the cosmological background. This approach not only serves as a unified description of vector-tensor theories but also highlights universal differences between the scalar-tensor theories and the vector-tensor theories. The theories having different symmetry breaking patterns are distinguished by a phenomenological function and consistency relations between the EFT coefficients. We study the linear cosmological perturbations within our EFT framework and discuss the characteristic properties of the vector-tensor theories in the context of dark energy. In particular, we compute the effective gravitational coupling and the slip parameter for the matter density contrast in terms of the EFT coefficients.
39 pages + appendices, 1 figure, published version
References in corpus (18)
- The Effective Field Theory of Inflation
- Causality, Analyticity and an IR Obstruction to UV Completion
- Starting the Universe: Stable Violation of the Null Energy Condition and Non-standard Cosmologies
- Exploring gravitational theories beyond Horndeski
- Maximal freedom at minimum cost: linear large-scale structure in general modifications of gravity
- Inflationary Universe with Anisotropic Hair
- The Effective Theory of Quintessence: the w<-1 Side Unveiled
- A unifying description of dark energy
- Breaking of Vainshtein screening in scalar-tensor theories beyond Horndeski
- Weakly-coupled stealth solution in scordatura degenerate theory
- Spontaneous Lorentz Breaking at High Energies
- Black hole perturbations in DHOST theories: Master variables, gradient instability, and strong coupling
- Weakening Gravity on Redshift-Survey Scales with Kinetic Matter Mixing
- Accelerating Universe and Cosmological Perturbation in the Ghost Condensate
- Stealth dark energy in scordatura DHOST theory
- Constraining DHOST theories with linear growth of matter density fluctuations
- On the 1+3 Formalism in General Relativity
- Positivity vs. Lorentz-violation: an explicit example
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- Schwarzschild quasi-normal modes of non-minimally coupled vector fields
- Some disquisitions on cosmological 2-form dualities
- Causality Constraint on Circuit Complexity from