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Titlebook: Microwave Cavities and Detectors for Axion Research; Proceedings of the 3 Gianpaolo Carosi,Gray Rybka Conference proceedings 2020 This is a

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樓主: risky-drinking
51#
發(fā)表于 2025-3-30 11:30:14 | 只看該作者
52#
發(fā)表于 2025-3-30 15:13:37 | 只看該作者
53#
發(fā)表于 2025-3-30 18:05:45 | 只看該作者
54#
發(fā)表于 2025-3-30 22:49:46 | 只看該作者
55#
發(fā)表于 2025-3-31 04:14:46 | 只看該作者
56#
發(fā)表于 2025-3-31 08:29:23 | 只看該作者
Overview of the Cosmic Axion Spin Precession Experiment (CASPEr),des of ALP parameter space beyond the current astrophysical and laboratory bounds. It is anticipated that future versions of the experiments will be sensitive to the axions associated with quantum chromodynamics (QCD) having masses ..
57#
發(fā)表于 2025-3-31 13:14:30 | 只看該作者
Exclusion Limits on Hidden-Photon Dark Matter Near 2 neV from a Fixed-Frequency Superconducting Lum and set a simple exclusion limit on ~2 neV hidden photons with kinetic mixing angle .???1.5?×?10. based on 5.14 h of integrated noise. This test device informs the development of the Dark Matter Radio, a tunable superconducting lumped-element resonator which will search for axions and hidden photons over the 100 Hz to 300 MHz frequency range.
58#
發(fā)表于 2025-3-31 17:02:52 | 只看該作者
Recent Results with the ADMX Experiment, results marked the first time a haloscope experiment achieved sensitivity to the well-motivated DFSZ axion. In addition, I will provide updates on the search for axions in the 2.82–3.31 .eV madss range with the ADMX experiment.
59#
發(fā)表于 2025-3-31 20:10:19 | 只看該作者
60#
發(fā)表于 2025-3-31 23:42:28 | 只看該作者
The ORGAN Experiment,ric materials) higher order modes present solutions to some of these issues. We discuss a few schemes for implementing higher order modes in haloscope searches, with a particular focus on cavity design for the ORGAN Experiment.
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