pith. sign in

arxiv: 1205.6260 · v2 · pith:3GHUOUCVnew · submitted 2012-05-29 · ✦ hep-ph · astro-ph.CO· physics.atom-ph

How do you know if you ran through a wall?

classification ✦ hep-ph astro-ph.COphysics.atom-ph
keywords currentlydarkexperimentsgravitationalnetworkwallwallsaimed
0
0 comments X
read the original abstract

Stable topological defects of light (pseudo)scalar fields can contribute to the Universe's dark energy and dark matter. Currently the combination of gravitational and cosmological constraints provides the best limits on such a possibility. We take an example of domain walls generated by an axion-like field with a coupling to the spins of standard-model particles, and show that if the galactic environment contains a network of such walls, terrestrial experiments aimed at detection of wall-crossing events are realistic. In particular, a geographically separated but time-synchronized network of sensitive atomic magnetometers can detect a wall crossing and probe a range of model parameters currently unconstrained by astrophysical observations and gravitational experiments.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Highly Excited Electron Cyclotron for QCD Axion and Dark-Photon Detection

    hep-ph 2024-10 unverdicted novelty 6.0

    Proposes resonant detection of QCD axions (0.1-2.3 meV) and dark photons (down to epsilon ~2e-16) via highly excited electron cyclotron states in an open-endcap Penning trap compatible with large cavities.