Pith. sign in

REVIEW

Search for streaming dark matter axions or other exotica

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

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 1803.08588 v2 pith:JYTEKI7J submitted 2018-03-22 astro-ph.IM

A. Gardikiotis , V. Anastassopoulos , S. Bertolucci , G. Cantatore , S. Cetin , H. Fischer , W. Funk , D.H.H. Hoffmann
show 6 more authors
S. Hofmann M. Karuza M. Maroudas Y. Semertzidis I. Tkachev K. Zioutas
This is my paper · ORCID
classification astro-ph.IM
keywords axionotheraxionsdarkexoticamattersearchstreaming
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

We suggest a new approach to search for galactic axions or other similar exotica. Streaming dark matter (DM) could have a better discovery potential because of flux enhancement, due to gravitational lensing when the Sun and/or a planet are aligned with a DM stream. Of interest are also axion miniclusters, in particular, if the solar system has trapped one during its formation. Wide-band axion antennae fit this concept, but also the proposed fast narrow band scanning. A network of detectors can provide full time coverage and a large axion mass acceptance. Other DM searches may profit from this proposal.

Discussion (0). Continue with ORCID to comment.

Pith tools