Constraints on the strength of primordial magnetic fields from big bang nucleosynthesis reexamined

Baolian Cheng, Angela V. Olinto, David N. Schramm, and James W. Truran
Phys. Rev. D 54, 4714 – Published 15 October 1996
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Abstract

In this paper, we reexamine in detail the effects of primordial magnetic fields on big bang nucleosynthesis (BBN) including a discussion of the magnetic field geometry and the anomalous magnetic moment. The presence of magnetic fields affects BBN by (1) increasing the weak reaction rates, (2) increasing the electron density due to changes to the electron phase space, and (3) increasing the expansion rate of the universe, due both to the magnetic field energy density and to the modified electron energy density. Of the effects considered, the increase in the expansion rate due to the magnetic field energy is the most significant for the interests of BBN. The allowed magnetic field intensity at the end of nucleosynthesis (0.01 MeV) is about 2×109 G and corresponds to an upper limit on the magnetic field energy density of about 28% of the neutrino energy density (ρB<~0.28ρν).

  • Received 12 April 1996

DOI:https://doi.org/10.1103/PhysRevD.54.4714

©1996 American Physical Society

Authors & Affiliations

Baolian Cheng1, Angela V. Olinto1,2, David N. Schramm2, and James W. Truran2

  • 1Los Alamos National Laboratory, NIS-2 MS D436, Los Alamos, New Mexico 87545
  • 2Department of Astronomy and Astrophysics and Enrico Fermi Institute, The University of Chicago, 5640 South Ellis Avenue, Chicago, Illinois 60637

Comments & Replies

Comment on “Constraints on the strength of primordial magnetic fields from big bang nucleosynthesis reexamined”

Peter J. Kernan, Glenn D. Starkman, and Tanmay Vachaspati
Phys. Rev. D 56, 3766 (1997)

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Vol. 54, Iss. 8 — 15 October 1996

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