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Cited by 736

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Cosmological 'seed' magnetic field from inflation

Ratra, Bharat·1992·The Astrophysical Journal

Abstract

The scalar-field-inflation-modified hot big bang model (Ratra and Peebles, 1988; Ratra, 1989) is extended by adding an inflation epoch coupling term between the scalar field Phi responsible for inflation and an Abelian gauge field A(mu). It is shown that the inflation based mechanism can generate a present intergalactic magnetic field that might be as large as about 10 exp -10 G. This is an example of a primeval seed magnetic field, which might be amplified by anisotropic protogalactic collapse and galactic differential rotation to produce the present galactic magnetic fields. The paper describes the model and the derivation of the magnetic-field two-point correlation function.

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Metadata

Authors
Ratra, B.
Venue
The Astrophysical Journal
Published
1992-05
Volume
391
Pages
L1
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W2022022896
Cited by
736
References
0
FWCI
13.76
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Cosmological 'seed' magnetic field from inflation. https://app.cochat.ai/papers/10.1086/186384
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Ratra, B. (1992). Cosmological 'seed' magnetic field from inflation. The Astrophysical Journal. https://doi.org/10.1086/186384

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.