Pith. sign in

REVIEW 1 cited by

Stimulated Emission of Dark Matter Axion from Condensed Matter Excitations

Not yet reviewed by Pith; the record is open.

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 1612.05406 v2 pith:AXUQA5WK submitted 2016-12-16 hep-ph astro-ph.COcond-mat.mes-hallhep-th

classification hep-phastro-ph.COcond-mat.mes-hallhep-th
keywords matteraxionsdarkemissioncondensedpossiblestimulatedtype
verification ladder T0 review T1 audit T2 compute T3 formal

Signed reviews

No signed human review yet.

0 comments
read the original abstract

We discuss a possible principle for detecting dark matter axions in galactic halos. If axions constitute a condensate in the Milky Way, stimulated emissions of the axions from a type of excitation in condensed matter can be detectable. We provide general mechanism for the dark matter emission, and, as a concrete example, an emission of dark matter axions from magnetic vortex strings in a type II superconductor are investigated along with possible experimental signatures.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 1 Pith paper

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

  1. Abelian-Higgs vortices in the oscillating axion background

    hep-ph 2025-07 conditional novelty 7.0 of 10

    Axion oscillations can resonantly amplify electric fields inside Abelian-Higgs vortex cores and induce attractive or repulsive forces between vortices, even in the BPS limit.

Pith tools