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Renormalization of the $3D$$SU(N)$ scalar energy-momentum tensor using the Wilson flow
In the holographic approach to cosmology, cosmological observables are described in terms of correlators of a three-dimensional boundary quantum field theory. As a concrete model, we study the 3D massless SU(N) scalar matrix field theory with a $\phi^4$ interaction. On the lattice, the energy-moment...
Autores principales: | , , , , , , , , |
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Lenguaje: | eng |
Publicado: |
2022
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.22323/1.396.0313 http://cds.cern.ch/record/2802265 |