Skip to content
DraconiticResearch
Search Sources API
194,161 studies31 sourcesUpdated 42 min ago
PreprintCC BY 4.0arXiv

The phenomenology of Axion Relic Pockets

Abstract

Axion relic pockets are phase-transition remnants consisting of regions of false vacuum stabilised from collapse by a hot axion gas. Axion relic pockets can comprise dark matter, but little is known about their phenomenology. We consider trapped axions coupled to electromagnetism and derive the axion to photon conversion rate accounting for the pocket's compactness and spherical geometry. As a case study, we show that axion-photon conversion occurs in atomic electric fields, leading to high-energy electromagnetic cascades that may be detectable by neutrino, cosmic-ray, and dark-matter experiments. The distribution of electromagnetic showers is inherently isotropic, and upward-going showers provide a smoking-gun signal for the model. Using recent data from the IceCube neutrino telescope, we derive the first limits from terrestrial experiments on axion relic pockets as dark matter. However, for the simplest realisation of the model, only a small part of the parameter space can give signals strong enough to be constrained by current data. We also comment on the prospects for discovering axion relic pockets using fluorescence and radio Cherenkov detection by atmospheric instruments and balloon-borne payloads, as well as traditional dark matter direct detection experiments. These results provide the necessary tools to initiate phenomenological studies of axion relic pockets across different environments.

Related

  1. At the EDGES of MADness: phenomenology of relic millicharged atomic dark matter
    Eleonora Vanzan, Kimberly K. Boddy, Ely D. Kovetz
    arXivPreprintCC BY 4.0Full textCosmologyHigh-energy & particle physicsarXiv
  2. Phenomenology of axion-meson mixing and scattering processes
    Noé Duarte-González
    arXivPreprintCC BY 4.0Full textCosmologyHigh-energy & particle physicsarXiv
  3. Relic Neutrinos Probing Small Scale Primordial Non-Gaussianity
    Suraj Gavhale, Shin'ichi Nojiri, Sergei D. Odintsov +1
    arXivPreprintCC BY 4.0Full textGravitation & general relativityHigh-energy & particle physicsarXiv
  4. Inelastic Dark Matter from a Higher-Dimensional Operator: The LUX-ZEPLIN High-Recoil Event and Thermal Relic
    Debajyoti Choudhury, Jaydeb Das, Divya Sachdeva
    arXivPreprintCC BY 4.0Full textHigh-energy & particle physicsarXiv
  5. Constraining U(1)Lμ−Lτ Model with Dark Matter Using Relic Density and Neff Bounds
    Shivam Gola
    arXivPreprintCC BY 4.0Full textHigh-energy & particle physicsarXiv
BibTeX
@misc{khater2026phenomenology,
  title = {{The phenomenology of Axion Relic Pockets}},
  author = {Wafaa Khater and M. C. David Marsh and Charalampos Nikolis},
  howpublished = {arXiv},
  year = {2026},
  month = sep,
  doi = {10.48550/arxiv.2609.24714},
  eprint = {2609.24714},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2609.24714},
  note = {CC BY 4.0},
}
RIS
TY  - UNPB
TI  - The phenomenology of Axion Relic Pockets
AU  - Wafaa Khater
AU  - M. C. David Marsh
AU  - Charalampos Nikolis
PY  - 2026
DA  - 2026/09/21
PB  - arXiv
DO  - 10.48550/arxiv.2609.24714
UR  - https://arxiv.org/abs/2609.24714
AB  - Axion relic pockets are phase-transition remnants consisting of regions of false vacuum stabilised from collapse by a hot axion gas. Axion relic pockets can comprise dark matter, but little is known about their phenomenology. We consider trapped axions coupled to electromagnetism and derive the axion to photon conversion rate accounting for the pocket's compactness and spherical geometry. As a case study, we show that axion-photon conversion occurs in atomic electric fields, leading to high-energy electromagnetic cascades that may be detectable by neutrino, cosmic-ray, and dark-matter experiments. The distribution of electromagnetic showers is inherently isotropic, and upward-going showers provide a smoking-gun signal for the model. Using recent data from the IceCube neutrino telescope, we derive the first limits from terrestrial experiments on axion relic pockets as dark matter. However, for the simplest realisation of the model, only a small part of the parameter space can give signals strong enough to be constrained by current data. We also comment on the prospects for discovering axion relic pockets using fluorescence and radio Cherenkov detection by atmospheric instruments and balloon-borne payloads, as well as traditional dark matter direct detection experiments. These results provide the necessary tools to initiate phenomenological studies of axion relic pockets across different environments.
ER  -