Primordial circular polarization in the cosmic microwave background
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Publication:1716702
DOI10.1016/j.physletb.2018.12.037zbMath1406.83002arXiv1811.05953OpenAlexW2901370203WikidataQ128719703 ScholiaQ128719703MaRDI QIDQ1716702
Evan McDonough, Stephon H. S. Alexander
Publication date: 5 February 2019
Published in: Physics Letters. B (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1811.05953
Relativistic cosmology (83F05) Observational and experimental questions in relativity and gravitational theory (83B05) Gravitational waves (83C35)
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Cites Work
- ``CMB-slow or how to determine cosmological parameters by hand?
- Magneto-optic effects of the cosmic microwave background
- Inflationary magneto-(non)genesis, increasing kinetic couplings, and the strong coupling problem
- The thermal history of the plasma and high-frequency gravitons
- Observable chiral gravitational waves from inflation in string theory
- Chiral gravitational waves and baryon superfluid dark matter