First experimental determination of the [13C II] hyperfine-structure constants A1/2=810.71(11) MHz and A3/2=162.18(5) MHz from astronomical spectra.
27 3D Fields Tahani et al
5 Pith papers cite this work, alongside 160 external citations. Polarity classification is still indexing.
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astro-ph.GA 5representative citing papers
Subradiance from entangled Dicke states in atomic hydrogen renders galactic halo gas dark in emission and transparent, matching dark matter properties at observed temperatures near 100 K.
Low-energy cosmic ray ionization rates in the Orion region scale with star formation rate as log10 ζ = (1.4±0.70)log10 SFR + (-10.5±2.9), supporting local generation by star formation.
SKA will enable Zeeman measurements of magnetic fields from cometary comas through Galactic structures and starburst galaxies to damped Ly-alpha systems at cosmological redshifts, with achievability tied to array assembly stages.
Reviews SKA techniques for reconstructing 3D magnetic field vectors in the ISM but presents no new data or derivations.
citing papers explorer
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Space as a spectroscopic laboratory: High-resolution spectroscopy of the [$^{13}$C II] hyperfine structure with SOFIA/upGREAT
First experimental determination of the [13C II] hyperfine-structure constants A1/2=810.71(11) MHz and A3/2=162.18(5) MHz from astronomical spectra.
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Quantum coherence and the invisible Universe: Subradiance as a dark matter mechanism
Subradiance from entangled Dicke states in atomic hydrogen renders galactic halo gas dark in emission and transparent, matching dark matter properties at observed temperatures near 100 K.
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Star Formation Drives Production of Low Energy Cosmic Rays
Low-energy cosmic ray ionization rates in the Orion region scale with star formation rate as log10 ζ = (1.4±0.70)log10 SFR + (-10.5±2.9), supporting local generation by star formation.
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Measuring Magnetic Fields Near and Far with the SKA via the Zeeman Effect
SKA will enable Zeeman measurements of magnetic fields from cometary comas through Galactic structures and starburst galaxies to damped Ly-alpha systems at cosmological redshifts, with achievability tied to array assembly stages.
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3D Magnetic Field Vectors in Space: Bubbles, Clouds, and Filaments
Reviews SKA techniques for reconstructing 3D magnetic field vectors in the ISM but presents no new data or derivations.