Results 21 to 30 of about 1,443 (288)
Analytic bootstrap of mixed correlators in the O(n) CFT
We use large spin perturbation theory and the Lorentzian inversion formula to compute order-ϵ corrections to mixed correlators in the O(n) Wilson-Fisher CFT in 4 − ϵ dimensions.
Francesco Bertucci +2 more
doaj +1 more source
SUSY shields the scaling symmetry of conformal quantum mechanics [PDF]
Renormalization of the inverse square potential usually breaks its classical conformal invariance. In a strongly attractive potential, the scaling symmetry is broken to a discrete subgroup while, in a strongly repulsive potential, it is preserved at quantum level. In the intermediate, weak-medium range of the coupling, an anomalous length scale appears
Lima, A. A. +3 more
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The pseudo-conformal universe: scale invariance from spontaneous breaking of conformal symmetry [PDF]
51 pages, 3 figures. v2 discussion and refs added, minus sign in transformation laws fixed.
Hinterbichler, Kurt, Khoury, Justin
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Tensors and spinors in de Sitter space
We construct the Wightman function for symmetric traceless tensors and Dirac fermions in dS d+1 in a coordinate and index free formalism using a d + 2 dimensional ambient space. We expand the embedding space formalism to cover spinor and tensor fields in
Ben Pethybridge, Vladimir Schaub
doaj +1 more source
Observation of Conformal Symmetry Breaking and Scale Invariance in Expanding Fermi Gases [PDF]
11 pages, 8 ...
Elliott, E. +2 more
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A CFT interpretation of cosmological correlation functions in α−vacua in de-Sitter space
De-Sitter(dS) space allows for a generalized class of vacua, known as α–vacua, described by some parameters. The Bunch-Davies (BD) vacuum is a point in this parameter space. The cosmological correlation function in BD vacuum in four dimensions and can be
Sachin Jain +4 more
doaj +1 more source
On scale versus conformal symmetry in turbulence [PDF]
4 pages, revtex, ref. added. We discuss the modification of our conclusions in the presence of vacuum expectation values of negative dimension ...
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CONFORMAL SCALING GAUGE SYMMETRY AND INFLATIONARY UNIVERSE [PDF]
Considering the conformal scaling gauge symmetry as a fundamental symmetry of nature in the presence of gravity, a scalar field is required and used to describe the scale behavior of the universe. In order for the scalar field to be a physical field, a gauge field is necessary to be introduced.
openaire +3 more sources
Modular differential equations with movable poles and admissible RCFT characters
Studies of modular linear differential equations (MLDE) for the classification of rational CFT characters have been limited to the case where the coefficient functions (in monic form) have no poles, or poles at special points of moduli space.
Arpit Das +3 more
doaj +1 more source
Softly broken conformal symmetry and the stability of the electroweak scale [PDF]
We point out a possible mechanism by which the electroweak hierarchy problem can be avoided in the low energy effective quantum field theory. Assuming the existence of a UV complete underlying fundamental theory and treating the cutoff scale Λ of the effective field theory as a real physical scale we argue that the hierarchy problem would be solved if
Chankowski, P. +3 more
openaire +4 more sources

