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PreprintCC BY 4.0arXiv

Non-Hermitian Holographic Flows to Little Rip Cosmologies

Abstract

Spacelike singularities supported by matter satisfying the null energy condition (NEC) are expected to fall within the Belinski--Khalatnikov--Lifshitz (BKL) paradigm. We show that controlled violations of the NEC in holography can lead to different black hole interiors. In a holographic model dual to a strongly coupled non-Hermitian 𝒫𝒯-symmetric QFT, we uncover a novel non-Kasner regime within its real, 𝒫𝒯-restored phase. The deep-interior geometry describes an isotropic FLRW cosmology undergoing super-accelerated expansion and approaching a Little Rip. This regime leaves a characteristic imprint on two-sided heavy-operator correlators, allowing it to be distinguished from a standard Kasner interior. Our construction provides a concrete holographic realization of a Little Rip cosmology and lays the groundwork for a Little Rip/CFT correspondence, in which such cosmological regimes can be explored through observables in a non-Hermitian quantum field theory.

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BibTeX
@misc{arean2026nonhermitian,
  title = {{Non-Hermitian Holographic Flows to Little Rip Cosmologies}},
  author = {Daniel Arean and David Garcia-Fariña and Juan F. Pedraza},
  howpublished = {arXiv},
  year = {2026},
  month = sep,
  doi = {10.48550/arxiv.2607.14284},
  eprint = {2607.14284},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2607.14284},
  note = {CC BY 4.0},
}
RIS
TY  - UNPB
TI  - Non-Hermitian Holographic Flows to Little Rip Cosmologies
AU  - Daniel Arean
AU  - David Garcia-Fariña
AU  - Juan F. Pedraza
PY  - 2026
DA  - 2026/09/10
PB  - arXiv
DO  - 10.48550/arxiv.2607.14284
UR  - https://arxiv.org/abs/2607.14284
AB  - Spacelike singularities supported by matter satisfying the null energy condition (NEC) are expected to fall within the Belinski--Khalatnikov--Lifshitz (BKL) paradigm. We show that controlled violations of the NEC in holography can lead to different black hole interiors. In a holographic model dual to a strongly coupled non-Hermitian 𝒫𝒯-symmetric QFT, we uncover a novel non-Kasner regime within its real, 𝒫𝒯-restored phase. The deep-interior geometry describes an isotropic FLRW cosmology undergoing super-accelerated expansion and approaching a Little Rip. This regime leaves a characteristic imprint on two-sided heavy-operator correlators, allowing it to be distinguished from a standard Kasner interior. Our construction provides a concrete holographic realization of a Little Rip cosmology and lays the groundwork for a Little Rip/CFT correspondence, in which such cosmological regimes can be explored through observables in a non-Hermitian quantum field theory.
ER  -