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The Magnetized Universe

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arxiv astro-ph/0312614 v2 pith:6WL7NA2S submitted 2003-12-24 astro-ph gr-qchep-exhep-phhep-th

classification astro-phgr-qchep-exhep-phhep-th
keywords large-scaleexistencefieldsmagneticastrophysicsclusterscompellingconverging
verification ladder T0 review T1 audit T2 compute T3 formal
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Cosmology, high-energy physics and astrophysics are converging on the study of large-scale magnetic fields. While the experimental evidence for the existence of large-scale magnetization in galaxies, clusters and superclusters is rather compelling, the origin of the phenomenon remains puzzling especially in light of the most recent observations. The purpose of the present review is to describe the physical motivations and some of the open theoretical problems related to the existence of large-scale magnetic fields.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Probing Axion-Photon conversion via circular polarization imprints in the CMB $V$-mode observations

    astro-ph.CO 2025-10 unverdicted novelty 6.0 of 10

    Proposes that axion-photon conversion in pre-CMB helical magnetic fields imprints detectable V-mode polarization in the CMB, allowing CLASS 40 GHz observations to constrain ALP masses 10^{-10} to 10^{-8} eV and their ...

  2. Magnetogenesis from Sawtooth Coupling: Gravitational Wave Probe of Reheating

    astro-ph.CO 2025-06 conditional novelty 5.0 of 10

    A sawtooth coupling active during reheating can generate blue-tilted magnetic fields whose secondary gravitational waves peak at nanohertz to millihertz frequencies.

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