4.7 Article

Slow decay of magnetic fields in open Friedmann universes

期刊

PHYSICAL REVIEW D
卷 77, 期 10, 页码 -

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AMER PHYSICAL SOC
DOI: 10.1103/PhysRevD.77.107302

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  1. STFC [ST/F002998/1, ST/G000581/1] Funding Source: UKRI
  2. Science and Technology Facilities Council [ST/G000581/1, ST/F002998/1] Funding Source: researchfish

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Magnetic fields in Friedmann universes can experience superadiabatic growth without departing from conventional electromagnetism. The reason is the relativistic coupling between vector fields and space-time geometry, which slows down the decay of large-scale magnetic fields in open universes, compared to that seen in perfectly flat models. The result is a large relative gain in magnetic strength that can lead to astrophysically interesting B fields, even if our Universe is only marginally open today.

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