Matches in SemOpenAlex for { <https://semopenalex.org/work/W2943763858> ?p ?o ?g. }
- W2943763858 abstract "The $ensuremath{mu}mathrm{eV}$-mass axion is one of the most promising candidates for cold dark matter and remains to be a well-motivated solution to the $CP$ problem of quantum chromodynamics (QCD) via the Peccei-Quinn mechanism. In this paper, we propose a novel method to detect the dark-matter axions in our Galaxy via the resonant emission $|mathrm{e}⟩ensuremath{rightarrow}|mathrm{g}⟩+ensuremath{gamma}+{ensuremath{gamma}}^{ensuremath{'}}+a$ (or the absorption $a+|mathrm{e}⟩ensuremath{rightarrow}|mathrm{g}⟩+ensuremath{gamma}+{ensuremath{gamma}}^{ensuremath{'}}$) in an atomic system with superradiance, where $|mathrm{e}⟩$ and $|mathrm{g}⟩$ stand for the excited and ground energy levels of atoms, respectively. A similar process via $|mathrm{e}⟩ensuremath{rightarrow}|mathrm{g}⟩+ensuremath{gamma}+a$ (or $a+|mathrm{e}⟩ensuremath{rightarrow}|mathrm{g}⟩+ensuremath{gamma}$) is also put forward to probe the axion-electron coupling. For the nominal experimental setup assuming a background-free environment, most of the parameter space for typical QCD axion models can be covered with parahydrogen molecules or ytterbium atoms. However, the background in a realistic experimental setup remains to be a major issue that needs to be solved in future studies. Searching for better atomic or molecular candidates may be required for a bigger signal-to-noise ratio." @default.
- W2943763858 created "2019-05-09" @default.
- W2943763858 creator A5027224341 @default.
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- W2943763858 date "2019-08-12" @default.
- W2943763858 modified "2023-10-14" @default.
- W2943763858 title "Probing cosmic axions through resonant emission and absorption in atomic systems with superradiance" @default.
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- W2943763858 doi "https://doi.org/10.1103/physrevd.100.035010" @default.
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