Skip to content
DraconiticResearch
Search Sources API
197,768 studies31 sourcesUpdated 11 min ago
PreprintarXiv licencearXiv

Localized zero modes enhance massive Casimir interactions

Abstract

Massive quantum fields ordinarily produce strongly screened Casimir interactions at large separation. We show that a normalisable localised zero mode can change this asymptotic behaviour: it opens an additional interaction channel whose decay is parametrically slower than that due to the exchange of massive quantum fluctuations, even though the continuum itself remains gapped. We demonstrate this mechanism analytically and show that the massive quantum fluctuations provide the local dressing of each object's coupling to the zero-mode fluctuations. The sine-Gordon kink provides an exactly solvable realisation in which the Casimir interaction exhibits the predicted zero-mode-dominated large-distance behaviour, with the enhancement localised around the kink.

Related

  1. Localised zero modes enhance massive Casimir interactions
    Jose M. Muñoz-Castañeda, Inés Cavero-Peláez, Gonzalo Sancho-Garrido
    Physics Letters BPeer-reviewedCC BY 4.0High-energy & particle physicsCrossref
  2. Dynamical Stability and Quasinormal Modes of Casimir Wormholes in dRGT Massive Gravity
    Piyali Bhar, Dhruba Jyoti Gogoi, A. Errehymy
    arXivPreprintCC BY 4.0Full textGravitation & general relativityarXiv
  3. Casimir effect for a massive scalar field confined between parallel plates with a spatially varying effective mass
    R. L. Araújo Xavier, M. H. B. Chaves, E. R. Bezerra de Mello +1
    arXivPreprintCC BY 4.0Full textMathematical physicsGravitation & general relativityarXiv
  4. Quasinormal modes of massive scalar perturbations in slow-rotation bumblebee black holes with traceless conformal electrodynamics
    Yassine Sekhmani, Wentao Liu, Weike Deng +1
    Physics of the Dark UniversePeer-reviewedLicence not stated7 citedHigh-energy & particle physicsOpenAlex
  5. Boundary-localized non-Hermitian modes in an absorbing quantum walk
    Francisco Riberi
    arXivPreprintCC BY 4.0Full textQuantum physics & quantum informationarXiv
BibTeX
@misc{munozcastaneda2026localized,
  title = {{Localized zero modes enhance massive Casimir interactions}},
  author = {Jose M. Muñoz-Castañeda and Inés Cavero-Peláez and Gonzalo Sancho-Garrido},
  howpublished = {arXiv},
  year = {2026},
  month = sep,
  doi = {10.48550/arxiv.2607.05530},
  eprint = {2607.05530},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2607.05530},
}
RIS
TY  - UNPB
TI  - Localized zero modes enhance massive Casimir interactions
AU  - Jose M. Muñoz-Castañeda
AU  - Inés Cavero-Peláez
AU  - Gonzalo Sancho-Garrido
PY  - 2026
DA  - 2026/09/29
PB  - arXiv
DO  - 10.48550/arxiv.2607.05530
UR  - https://arxiv.org/abs/2607.05530
AB  - Massive quantum fields ordinarily produce strongly screened Casimir interactions at large separation. We show that a normalisable localised zero mode can change this asymptotic behaviour: it opens an additional interaction channel whose decay is parametrically slower than that due to the exchange of massive quantum fluctuations, even though the continuum itself remains gapped. We demonstrate this mechanism analytically and show that the massive quantum fluctuations provide the local dressing of each object's coupling to the zero-mode fluctuations. The sine-Gordon kink provides an exactly solvable realisation in which the Casimir interaction exhibits the predicted zero-mode-dominated large-distance behaviour, with the enhancement localised around the kink.
ER  -