The DOI matches its Crossref record.
Cosmological 'seed' magnetic field from inflation
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.
Overview
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Integrity signals
Registry
Cites
Statistics
Verification
Claims the paper makes
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Self-check
Percentages, sums and reported differences re-computed from the paper’s own numbers.
The self-check needs the paper’s full text.
Citations
Cited by
Astrophysical magnetic fields and nonlinear dynamo theory
Brandenburg, A., & Subramanian, K. (2005) · Physics Reports · doi:10.1016/j.physrep.2005.06.005 · Cited by 1,640
The pre-big bang scenario in string cosmology
Gasperini, M., & Veneziano, G. (2003) · Physics Reports · doi:10.1016/s0370-1573(02)00389-7 · Cited by 872
Lidsey, J. E., Wands, D., & Copeland, E. J. (2000) · Physics Reports · doi:10.1016/s0370-1573(00)00064-8 · Cited by 480
Cosmological Magnetic Field Limits in an Inhomogeneous Universe
Blasi, P., Burles, S., & Olinto, A. V. (1999) · The Astrophysical Journal · doi:10.1086/311958 · Cited by 263
Primordial power spectra from anisotropic inflation
Dulaney, T. R., & Gresham, M. I. (2010) · Physical Review D · doi:10.1103/physrevd.81.103532 · Cited by 140
Metadata
- Authors
- Ratra, B.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- 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
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
Are you an author, or do you see a problem with this page? Request a review
How to cite
Cite CoChat for the checks on this page, and the paper for its own findings.
- This page
- CoChat. (2026). Citation check: Cosmological 'seed' magnetic field from inflation. https://app.cochat.ai/papers/10.1086/186384
- The paper
- Ratra, B. (1992). Cosmological 'seed' magnetic field from inflation. The Astrophysical Journal. https://doi.org/10.1086/186384
Data sources
Bibliographic data: Semantic Scholar, OpenAlex, Crossref.
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.