Skip to content
DraconiticResearch
Search Sources API
203,234 studies31 sourcesUpdated 27 min ago
PreprintarXiv licencearXiv

Evidence for an Obstruction to Perturbative Renormalization Group in Stochastic Turbulence

Abstract

We examine whether the perturbative renormalization group (RG) regime of stochastic turbulence can be continued from small ε to the physical value εphys=2, corresponding to large-scale forcing. Exploiting the simplifications of the large-d limit, we calculate the correction exponent ω to five-loop order and find a simple structure suggesting a closed analytic form. This form implies that the fixed point stable near ε=0 ceases to be simultaneously real and infrared stable before reaching εphys=2, pointing to a possible change of infrared regime rather than a controlled perturbative RG extrapolation.

Related

  1. Regularization of stochastic fluid dynamics and non-perturbative renormalization of the shear viscosity of incompressible fluids
    Mattis Harhoff, Cedric Riedel, Johannes Roth +1
    arXivPreprintarXiv licenceFull textFluid dynamicsHigh-energy & particle physicsarXiv
  2. Perturbative Renormalization of Noether Currents in SYM with Improved Discretizations
    Marios Costa, Elias Antoniou, Salomi Dimou +4
    arXivPreprintarXiv licenceFull textHigh-energy & particle physicsarXiv
  3. The Mass Gap Approach to QCD. II. The non-perturbative renormalization theory for the massive gluon fields
    V. Gogokhia, G. G. Barnafoldi
    arXivPreprintCC BY 4.0Full textHigh-energy & particle physicsarXiv
  4. Quark and hybrid stars with renormalization group improvement of NNLO perturbative QCD
    Loïc Fernandez, Jean-Loïc Kneur, Marcus Benghi Pinto +3
    arXivPreprintCC BY 4.0Full textHigh-energy astrophysicsHigh-energy & particle physicsarXiv
  5. Non-Perturbative Renormalization Group for Ising-Nematic Criticality: A Closed-Form Nonlocal Ansatz
    Hyeon Jung Kim, Kyoung-Min Kim, Ki-Seok Kim
    arXivPreprintarXiv licenceFull textCondensed matterarXiv
BibTeX
@misc{adzhemyan2026evidence,
  title = {{Evidence for an Obstruction to Perturbative Renormalization Group in Stochastic Turbulence}},
  author = {L. Ts. Adzhemyan and D. A. Davletbaeva and D. A. Evdokimov and M. V. Kompaniets},
  howpublished = {arXiv},
  year = {2026},
  month = oct,
  doi = {10.48550/arxiv.2610.01507},
  eprint = {2610.01507},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2610.01507},
}
RIS
TY  - UNPB
TI  - Evidence for an Obstruction to Perturbative Renormalization Group in Stochastic Turbulence
AU  - L. Ts. Adzhemyan
AU  - D. A. Davletbaeva
AU  - D. A. Evdokimov
AU  - M. V. Kompaniets
PY  - 2026
DA  - 2026/10/01
PB  - arXiv
DO  - 10.48550/arxiv.2610.01507
UR  - https://arxiv.org/abs/2610.01507
AB  - We examine whether the perturbative renormalization group (RG) regime of stochastic turbulence can be continued from small ε to the physical value ε_phys=2, corresponding to large-scale forcing. Exploiting the simplifications of the large-d limit, we calculate the correction exponent ω to five-loop order and find a simple structure suggesting a closed analytic form. This form implies that the fixed point stable near ε=0 ceases to be simultaneously real and infrared stable before reaching ε_phys=2, pointing to a possible change of infrared regime rather than a controlled perturbative RG extrapolation.
ER  -