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Primordial magnetic fields from a non-singular bouncing cosmology

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Publication:748663
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DOI10.1016/J.NUCLPHYSB.2014.05.018zbMath1323.83038arXiv1312.2162OpenAlexW1974917473MaRDI QIDQ748663

Federico Agustín Membiela

Publication date: 29 October 2015

Published in: Nuclear Physics. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1312.2162


zbMATH Keywords

inflationmagnetogenesis


Mathematics Subject Classification ID

Relativistic cosmology (83F05) Electromagnetic fields in general relativity and gravitational theory (83C50)


Related Items (4)

Enhance primordial black hole abundance through the non-linear processes around bounce point ⋮ Inflationary magneto-(non)genesis, increasing kinetic couplings, and the strong coupling problem ⋮ Inflationary magnetogenesis with reheating phase from higher curvature coupling ⋮ Effective theory of inflationary magnetogenesis and constraints on reheating




Cites Work

  • Starting the universe: stable violation of the null energy condition and non-standard cosmologies
  • Anisotropy in a non-singular bounce




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