Pith. sign in

REVIEW 1 cited by

Design and Operational Experience of a Microwave Cavity Axion Detector for the 20-100 micro-eV Range

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 1611.07123 v2 pith:DA4WJTUX submitted 2016-11-22 physics.ins-det astro-ph.IM

S. Al Kenany , M. A. Anil , K. M. Backes , B. M. Brubaker , S. B. Cahn , G. Carosi , Y. V. Gurevich , W. F. Kindel
show 12 more authors
S. K. Lamoreaux K. W. Lehnert S. M. Lewis M. Malnou D. A. Palken N. M. Rapidis J. R. Root M. Simanovskaia T. M. Shokair I. Urdinaran K. A. van Bibber L. Zhong
This is my paper · ORCID
classification physics.ins-detastro-ph.IM
keywords cavityamplifieraxionmicrowavedatadetectorfirstoperational
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
abstract

We describe a dark matter axion detector designed, constructed, and operated both as an innovation platform for new cavity and amplifier technologies and as a data pathfinder in the $5 - 25$ GHz range ($\sim20-100\: \mu$eV). The platform is small but flexible to facilitate the development of new microwave cavity and amplifier concepts in an operational environment. The experiment has recently completed its first data production; it is the first microwave cavity axion search to deploy a Josephson parametric amplifier and a dilution refrigerator to achieve near-quantum limited performance.

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. Indirect detection of the QCD axion

    astro-ph.CO 2024-11 unverdicted

    A GBT X-band search for axion minicluster-neutron star radio transients in M31 found no 5-sigma candidates, yielding sensitivity to QCD axions in the 33-42 micro-eV mass range.

Pith tools