Search for dark photon dark matter: Dark E field radio pilot experiment
| العنوان: | Search for dark photon dark matter: Dark E field radio pilot experiment |
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| المؤلفون: | S. Mani Tripathi, Seth Hillbrand, Daniel A. Polin, J. Anthony Tyson, Molly R. Smith, Paul A. Stucky, Kent D. Irwin, Joseph Levine, Arran Phipps, Benjamin Godfrey, Shelby Klomp, J. Balajthy, Brian H. Kolner, Peter W. Graham, Nate MacFadden |
| المصدر: | Physical Review D. 104 |
| بيانات النشر: | American Physical Society (APS), 2021. |
| سنة النشر: | 2021 |
| مصطلحات موضوعية: | Physics, Noise temperature, Physics - Instrumentation and Detectors, Photon, Dark matter, FOS: Physical sciences, Instrumentation and Detectors (physics.ins-det), Magnetic detector, Coupling (probability), Dark field microscopy, Dark photon, High Energy Physics - Experiment, Computational physics, High Energy Physics - Experiment (hep-ex), Sensitivity (control systems) |
| الوصف: | We are building an experiment to search for dark matter in the form of dark photons in the nano- to milli-eV mass range. This experiment is the electromagnetic dual of magnetic detector dark radio experiments. It is also a frequency-time dual experiment in two ways: We search for a high-Q signal in wide-band data rather than tuning a high-$Q$ resonator, and we measure electric rather than magnetic fields. In this paper we describe a pilot experiment using room temperature electronics which demonstrates feasibility and sets useful limits to the kinetic coupling $\epsilon \sim 10^{-12}$ over 50--300 MHz. With a factor of 2000 increase in real-time spectral coverage, and lower system noise temperature, it will soon be possible to search a wide range of masses at 100 times this sensitivity. We describe the planned experiment in two phases: Phase-I will implement a wide band, 5-million channel, real-time FFT processor over the 30--300 MHz range with a back-end time-domain optimal filter to search for the predicted $Q\sim 10^6$ line using low-noise amplifiers. We have completed spot frequency calibrations using a biconical dipole antenna in a shielded room that extrapolate to a $5 \sigma$ limit of $\epsilon\sim 10^{-13}$ for the coupling from the dark field, per month of integration. Phase-II will extend the search to 20 GHz using cryogenic preamplifiers and new antennas. Comment: 11 pages, 13 figures. Updated to published version. Corrected minor error in Fig 12 x-axis; results unchanged |
| تدمد: | 2470-0029 2470-0010 |
| URL الوصول: | https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d1c11b1f724ce7930f209e6ae2fcf346 https://doi.org/10.1103/physrevd.104.012013 |
| حقوق: | OPEN |
| رقم الأكسشن: | edsair.doi.dedup.....d1c11b1f724ce7930f209e6ae2fcf346 |
| قاعدة البيانات: | OpenAIRE |
| تدمد: | 24700029 24700010 |
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