Abstract:We present a complete classification of symmetric superfluids, namely shift-symmetric and Poincaré invariant scalar field theories that have an enlarged set of classically conserved currents at leading order in derivatives. These theories arise in the decoupling limit of the effective field theory of shift-symmetric, single-clock cosmologies and our results pick out all models with couplings fixed by additional symmetry. Remarkably, in D ≥ 2 spacetime dimensions there are only two possibilities: the Dirac-Born… Show more
“…It isn't obvious whether one can construct an 'improved' traceless stress tensor [24][25][26][27][28], but it seems highly unlikely in the full nonlinear theory 2 . See [24,29] for discussions on this point in similar theories. Therefore these cases are scale but not conformal invariant (i.e.…”
Section: )mentioning
confidence: 99%
“…It is easy to extend the the above analysis of solids that realize SI to a simpler case, namely a SI relativistic superfluid, which consists in a single scalar field that has a temporal vev for the gradient, Ψ = t + ψ. This case has also been studied in [29]. The most general action at leading order in derivatives is S = d d xP (X (Ψ) ) where X (Ψ) ≡ ∂ µ Ψg µν ∂ ν Ψ.…”
Scale invariance (SI) can in principle be realized in the elastic response of solid materials. There are two basic options: that SI is a manifest symmetry or that it is spontaneously broken. The manifest case corresponds physically to the existence of a non-trivial infrared fixed point with phonons among its degrees of freedom. We use simple bottom-up AdS/CFT constructions to model this case. We characterize the types of possible elastic response and discuss how the sound speeds can be realistic, that is, sufficiently small compared to the speed of light. We also study the spontaneously broken case using Effective Field Theory (EFT) methods. We present a new oneparameter family of nontrivial EFTs that includes the previously known 'conformal solid' as a particular case as well as others which display small sound speeds. We also point out that an emergent Lorentz invariance at low energies could affect by order-one factors the relation between sound speeds and elastic moduli.
“…It isn't obvious whether one can construct an 'improved' traceless stress tensor [24][25][26][27][28], but it seems highly unlikely in the full nonlinear theory 2 . See [24,29] for discussions on this point in similar theories. Therefore these cases are scale but not conformal invariant (i.e.…”
Section: )mentioning
confidence: 99%
“…It is easy to extend the the above analysis of solids that realize SI to a simpler case, namely a SI relativistic superfluid, which consists in a single scalar field that has a temporal vev for the gradient, Ψ = t + ψ. This case has also been studied in [29]. The most general action at leading order in derivatives is S = d d xP (X (Ψ) ) where X (Ψ) ≡ ∂ µ Ψg µν ∂ ν Ψ.…”
Scale invariance (SI) can in principle be realized in the elastic response of solid materials. There are two basic options: that SI is a manifest symmetry or that it is spontaneously broken. The manifest case corresponds physically to the existence of a non-trivial infrared fixed point with phonons among its degrees of freedom. We use simple bottom-up AdS/CFT constructions to model this case. We characterize the types of possible elastic response and discuss how the sound speeds can be realistic, that is, sufficiently small compared to the speed of light. We also study the spontaneously broken case using Effective Field Theory (EFT) methods. We present a new oneparameter family of nontrivial EFTs that includes the previously known 'conformal solid' as a particular case as well as others which display small sound speeds. We also point out that an emergent Lorentz invariance at low energies could affect by order-one factors the relation between sound speeds and elastic moduli.
“…It belongs to a subclass of scalar-tensor theories where the Lorentz invariance is broken [18][19][20][21] and can be extended into more general class [22]. Aspects of symmetry in cuscuton gravity is studied in [23]. In particular, it has been shown that cuscuton gravity is useful in cosmology [24,25], for instance, a healthy bouncing solution without instabilities were realized [26].…”
We study Kaluza-Klein cosmology in cuscuton gravity and find an exact solution describing an accelerating 4-dimensional universe with a stable extra dimension. A cuscuton which is a nondynamical scalar field is responsible for the accelerating expansion and a vector field makes the extra dimensional space stable. Remarkably, the accelerating universe in our model is not exactly de Sitter.
CONTENTS
“…Consider the action S[φ] with a variational global symmetry group G and a vacuum solution φ 0 (x). In the active form, the symmetry group G acts on the fields φ(x) as 82) while the coordinates do not transform. A symmetry transformation for which g • φ 0 (x) = φ 0 (x) is broken by the vacuum field configuration.…”
Section: Spontaneous Symmetry Breaking and Nonlinear Realizationsmentioning
confidence: 99%
“…Jacobi identities ensure that the algebra up to first-order is that of the four-dimensional conformal algebra. It is not possible to extend the conformal algebra with the addition of G 2 apart from in two space-time dimensions (see for [82] more details.). Due to the lack of shift symmetry and Adler's zero for the scalar, there is no sense in which the resulting EFT of the dilaton has an enhanced soft limit.…”
CONTENTS function of space-time, rather than a (possibly infinite) series of constant coefficients. The former are proper gauge redundancies, the latter make up the large gauge transformations.
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