Search for Invisible Axion Dark Matter in the 
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 Mass Range

Bartram, C.; Braine, T.; Burns, Eileen S.; Cervantes, R.; Crisosto, N.; Du, N.; Korandla, H; Leum, G.; Mohapatra, P.; Nitta, T.; Rosenberg, L.; Rybka, G.; Yang, Ji-Woon; Clarke, John; Siddiqi, Irfan; Agrawal, Ankur; Dixit, Akash; Awida, Mohamed H.; Chou, A.; Hollister, M. I.; Knirck, Stefan; Sonnenschein, A.; Wester, W.; Gleason, J.; Hipp, A. T.; Jois, S.; Sikivie, P.; Sullivan, N. S.; Tanner, D. B.; Lentz, Erik W.; Khatiwada, R.; Carosi, G.; Robertson, N. A.; Woollett, Nathan; Duffy, Leanne D.; Boutan, C.; Jones, Mark; LaRoque, B. H.; Oblath, N. S.; Taubman, Matthew S.; Daw, E. J.; Perry, M. G.; Buckley, J. H.; Gaikwad, C.; Hoffman, Joseph J.; Murch, Kater; Goryachev, Maxim; McAllister, Ben T.; Quiskamp, Aaron; Thomson, Catriona A.; Tobar, Michael E.

doi:10.1103/physrevlett.127.261803

Cited by 176 publications

(63 citation statements)

References 38 publications

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“…[43]). So far, dark matter has evaded all direct searches based on experiments on the earth, including the hunt for weakly interacting massive particles (WIMPs) [44] and axion dark matter [45]. The interest in macroscopic dark matter candidates such as PBHs has been revived in light of the discovery of black hole mergers by LIGO and Virgo [46][47][48].…”

Section: Introductionmentioning

confidence: 99%

Broad search for gravitational waves from subsolar-mass binaries through LIGO and Virgo's third observing run

Nitz,

Wang

2022

Preprint

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Section: Introductionmentioning

confidence: 99%

Broad search for gravitational waves from subsolar-mass binaries through LIGO and Virgo's third observing run

Nitz,

Wang

2022

Preprint

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“…We illustrate the median limit over 100 MC realizations of the NS population (red line), and the corresponding 68% and 95% statistical uncertainties on the population model (see text for details). We compare our upper limit to those from the CAST [15], HAYSTAC [16,17] and ADMX [18,19] experiments and the prediction from ALP-cogenesis [20]. electric (magnetic) field, a is the axion field, and g aγγ is a coupling constant (with units of inverse energy).…”

mentioning

confidence: 99%

Extraterrestrial Axion Search with the Breakthrough Listen Galactic Center Survey

Foster¹,

Witte²,

Lawson³

et al. 2022

Preprint

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“…haloscope approach introduced in Ref. [2] for ADMX [19][20][21] and SQMS (see also Ref. [22]), as well as cosmological probes of GWs [23] based on observations by the radio telescopes EDGES and ARCADE [24,25].…”

mentioning

confidence: 99%

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

Domcke,

Garcia-Cely,

Rodd

2022

Preprint

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Gravitational waves (GWs) generate oscillating electromagnetic effects in the vicinity of external electric and magnetic fields. We discuss this phenomenon with a particular focus on reinterpreting the results of axion haloscopes based on lumped-element detectors, which probe GWs in the 100 kHz -100 MHz range. Measurements from ABRACADABRA and SHAFT already place bounds on GWs, although the present strain sensitivity is weak. However, we demonstrate that the sensitivity scaling with the volume of such instruments is significant -faster than for axions -and so rapid progress will be made in the future. With no modifications, DMRadio-m 3 will have a GW strain sensitivity of h ∼ 10 −20 at 200 MHz. A simple modification of the pickup loop used to readout the induced magnetic flux can parametrically enhance the GW sensitivity, particularly at lower frequencies.

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Search for Invisible Axion Dark Matter in the 3.3–4.2 μeV Mass Range

Cited by 176 publications

References 38 publications

Broad search for gravitational waves from subsolar-mass binaries through LIGO and Virgo's third observing run

Broad search for gravitational waves from subsolar-mass binaries through LIGO and Virgo's third observing run

Extraterrestrial Axion Search with the Breakthrough Listen Galactic Center Survey

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

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