Skip to content
DraconiticResearch
Search Sources API
197,787 studies31 sourcesUpdated 31 min ago
PreprintCC BY 4.0arXiv

Curved momentum space and finite Landau spectrum in κ-Minkowski spacetime

Abstract

We derive the κ-Poincaré Casimir from the de Sitter geometry of momentum space and employ it as the dynamical constraint governing charged particles within the framework of Poisson gauge theory. The resulting formalism is applied to scalar and spin-1/2 particles in a constant magnetic field. Within the semiclassical Poisson-gauge framework, exact energy spectra are obtained without expanding in the deformation parameter 1/κ. On the positive-energy branch in bicrossproduct momentum coordinates, identifying these coordinates with the physical momenta entering the gauge coupling imposes an upper bound on their spatial magnitude. This bound leads to a finite number of admissible Landau-level indices and hence to a Highest Landau Level (HLL). In the fermionic case, the truncation is spin dependent for the factorization adopted here, resulting in a polarized HLL. Possible implications of this ultraviolet truncation and the limitations of the framework are briefly discussed.

Versions

Related

  1. Circular acceleration in Minkowski spacetime: thermality versus finite size
    Cameron R D Bunney, Jorma Louko
    arXivPreprintarXiv licenceFull textGravitation & general relativityarXiv
  2. Harvesting magic resource in curved spacetime
    Jiayue Yang, Dyuman Bhattacharya, Ming Zhang +1
    Communications PhysicsPeer-reviewedCC BY 4.0Atomic, molecular & optical physicsCrossrefNature
  3. Energy balance of a boson gas at zero temperature in curved spacetime
    Jorge Meza-Domínguez, Tonatiuh Matos, Pierre-Henri Chavanis
    Physical Review DPeer-reviewedLicence not statedFull textGravitation & general relativityHAL
  4. Influence of dark matter on quantum entanglement and coherence in curved spacetime
    Shu-Min Wu, Yuxuan Wang, Si-Han Shang +1
    Chinese Journal of PhysicsPeer-reviewedLicence not statedFull text8 citedHigh-energy & particle physicsOpenAlex
  5. Fermion quantum field theory on curved and non-inertial backgrounds in standard-Minkowski form
    Fabio Di Pumpo, Tobias Asano, Alexander Friedrich +2
    arXivPreprintarXiv licenceFull textGravitation & general relativityHigh-energy & particle physicsarXiv
BibTeX
@misc{vargas2026curved,
  title = {{Curved momentum space and finite Landau spectrum in $κ$-Minkowski spacetime}},
  author = {Adrián Huamán Vargas and Vladislav Kupriyanov},
  howpublished = {arXiv},
  year = {2026},
  month = sep,
  doi = {10.48550/arxiv.2607.25833},
  eprint = {2607.25833},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2607.25833},
  note = {CC BY 4.0},
}
RIS
TY  - UNPB
TI  - Curved momentum space and finite Landau spectrum in κ-Minkowski spacetime
AU  - Adrián Huamán Vargas
AU  - Vladislav Kupriyanov
PY  - 2026
DA  - 2026/09/15
PB  - arXiv
DO  - 10.48550/arxiv.2607.25833
UR  - https://arxiv.org/abs/2607.25833
AB  - We derive the κ-Poincaré Casimir from the de Sitter geometry of momentum space and employ it as the dynamical constraint governing charged particles within the framework of Poisson gauge theory. The resulting formalism is applied to scalar and spin-1/2 particles in a constant magnetic field. Within the semiclassical Poisson-gauge framework, exact energy spectra are obtained without expanding in the deformation parameter 1/κ. On the positive-energy branch in bicrossproduct momentum coordinates, identifying these coordinates with the physical momenta entering the gauge coupling imposes an upper bound on their spatial magnitude. This bound leads to a finite number of admissible Landau-level indices and hence to a Highest Landau Level (HLL). In the fermionic case, the truncation is spin dependent for the factorization adopted here, resulting in a polarized HLL. Possible implications of this ultraviolet truncation and the limitations of the framework are briefly discussed.
ER  -