English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

Gravitational waves (GWs) generate oscillating electromagnetic effects in thevicinity of external electric and magnetic fields. We discuss this phenomenonwith a particular focus on reinterpreting the results of axion haloscopes basedon lumped-element detectors, which probe GWs in the 100 kHz-100 MHz range.Measurements from ABRACADABRA and SHAFT already place bounds on GWs, althoughthe present strain sensitivity is weak. However, we demonstrate that thesensitivity scaling with the volume of such instruments is significant - fasterthan for axions - and so rapid progress will be made in the future. With nomodifications, DMRadio-m$^3$ will have a GW strain sensitivity of $h \sim10^{-20}$ at 200 MHz. A simple modification of the pickup loop used to readoutthe induced magnetic flux can parametrically enhance the GW sensitivity,particularly at lower frequencies.

A novel search for high-frequency gravitational waves with low-mass axion haloscopes