REVIEW 4 cited by
Analysis of single-photon and linear amplifier detectors for microwave cavity dark matter axion searches
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
abstract
We show that at higher frequencies, and thus higher axion masses, single-photon detectors become competitive and ultimately favored, when compared to quantum-limited linear amplifiers, as the detector technology in microwave cavity experimental searches for galactic halo dark matter axions. The cross-over point in this comparison is of order 10 GHz ($\sim 40\ \mu$eV), not far above the frequencies of current searches.
Forward citations
Cited by 4 Pith papers
-
Design of ALPHA Phase I: A Plasma Haloscope for 10--20 GHz Post-Inflation Axions
ALPHA Phase I is designed to probe axion dark matter at 40 to 80 micro-eV mass with projected KSVZ-level sensitivity using tunable wire-array plasma resonators.
-
Coherent collective response in many-qubit systems for dark matter detection
Ramsey interferometry on large arrays of unentangled qubits achieves dark-matter sensitivity scaling as 1/sqrt(N), enabling projected bounds competitive with or better than existing limits for N greater than or equal ...
-
Axion Quark Nugget Dark Matter: Time Modulations and Amplifications
Simulated AQN dark matter crossing Earth produces relativistic axions at around 10^14 eV/cm2/s with about 10% daily and annual modulations and rare 100 to 10,000 times local flash amplifications.
-
Experiments to test the hypothesis for solar and dark matter axions
This is a pedagogical review of haloscope and helioscope experiments searching for dark matter and solar axions, with an overview of near-future technological developments.
Discussion (0). Continue with ORCID to comment.