Risking your NEC

Carlos Hoyos (Department of Physics and Instituto de Ciencias y Tecnologías Espaciales de Asturias (ICTEA), Universidad de Oviedo, c/Federico García Lorca 18, Oviedo, E-33007/33004, Spain) ; Niko Jokela (Department of Physics and Helsinki Institute of Physics, P.O. Box 64, University of Helsinki, Helsinki, FIN-00014, Finland) ; José Penín (Department of Physics and Helsinki Institute of Physics, P.O. Box 64, University of Helsinki, Helsinki, FIN-00014, Finland; Mathematical Sciences and STAG Research Center, University of Southampton, University Road, Southampton, SO17 1BJ, U.K.) ; Alfonso Ramallo (Departamento de Física de Partículas and Instituto Galego de Física de Altas Enerxías (IGFAE), Universidade de Santiago de Compostela, Rúa de Xoaquín Díaz de Rábago s/n, Santiago de Compostela, E-15782, Spain) ; Javier Tarrío (Department of Physics and Helsinki Institute of Physics, P.O. Box 64, University of Helsinki, Helsinki, FIN-00014, Finland)

Energy conditions, especially the null energy condition (NEC), are generically imposed on solutions to retain a physically sensible classical field theory and they also play an important role in the AdS/CFT duality. Using this duality, we study non-trivially deformed strongly coupled quantum field theories at large-N c . The corresponding dual classical gravity constructions entail the use of radially non-monotonic D-brane distributions. The distributions are phenomenological in the sense that they do not correspond to the smearing of known probe D-brane embeddings. The gravity backgrounds are supersymmetric and hence perturbatively stable, and do not possess curvature singularities. There are no short-cuts through the bulk spacetime for signal propagation which assures that the field theory duals are causal. Nevertheless, some of our solutions violate the NEC in the gravity dual. In these cases the non-monotonicity of the D-brane distributions is reflected in the properties of the renormalization group flow: none of the c-functions proposed in the literature are monotonic. This further suggests that the non-monotonic behavior of the c-functions within previously known anisotropic backgrounds does not originate from the breaking of Lorentz invariance. We surmise that NEC violations induced by quantum corrections also need to be considered in holographic duals, but can be studied already at the classical level.

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      "value": "Energy conditions, especially the null energy condition (NEC), are generically imposed on solutions to retain a physically sensible classical field theory and they also play an important role in the AdS/CFT duality. Using this duality, we study non-trivially deformed strongly coupled quantum field theories at large-N  c . The corresponding dual classical gravity constructions entail the use of radially non-monotonic D-brane distributions. The distributions are phenomenological in the sense that they do not correspond to the smearing of known probe D-brane embeddings. The gravity backgrounds are supersymmetric and hence perturbatively stable, and do not possess curvature singularities. There are no short-cuts through the bulk spacetime for signal propagation which assures that the field theory duals are causal. Nevertheless, some of our solutions violate the NEC in the gravity dual. In these cases the non-monotonicity of the D-brane distributions is reflected in the properties of the renormalization group flow: none of the c-functions proposed in the literature are monotonic. This further suggests that the non-monotonic behavior of the c-functions within previously known anisotropic backgrounds does not originate from the breaking of Lorentz invariance. We surmise that NEC violations induced by quantum corrections also need to be considered in holographic duals, but can be studied already at the classical level."
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Published on:
14 October 2021
Publisher:
Springer
Published in:
Journal of High Energy Physics , Volume 2021 (2021)
Issue 10
Pages 1-53
DOI:
https://doi.org/10.1007/JHEP10(2021)112
arXiv:
2104.11749
Copyrights:
The Author(s)
Licence:
CC-BY-4.0

Fulltext files: