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Inhomogeneous Primordial Magnetic Field Strength and Its Impact on Primordial Nucleosynthesis

  • Yudong Luo*
  • , Toshitaka Kajino
  • , Motohiko Kusakabe
  • , Grant J. Mathews
  • *此作品的通讯作者
  • National Astronomical Observatory of Japan
  • The University of Tokyo
  • Beihang University
  • University of Notre Dame

科研成果: 书/报告/会议事项章节会议稿件同行评审

摘要

We investigate the effect on the light element abundances from the presence of a primordial magnetic field (PMF) whose strength is spatially inhomogeneous. By assuming an uniform total energy density with a gaussian distribution of field strength, we find that domains of different temperatures exist in the BBN epoch due to variations in the local PMF. As a result, the effective distribution function of particle velocities averaged over domains of different temperatures deviates from the Maxwell-Boltzmann distribution. We perform BBN calculations including this effect and find that the 7Li abundance is significantly reduced. We also discuss the possibility that the baryon-to-photon ratio decreased after the BBN epoch. In this case, if the ratio during BBN was larger than the cosmic microwave background constraint, all produced light elements are consistent with observational data.

源语言英语
主期刊名Nuclei in the Cosmos XV
编辑Alba Formicola, Matthias Junker, Lucio Gialanella, Gianluca Imbriani
出版商Springer Science and Business Media, LLC
401-403
页数3
ISBN(印刷版)9783030138752
DOI
出版状态已出版 - 2019
活动15th International Symposium on Nuclei in the Cosmos, NIC 2018 - L'Aquila, 意大利
期限: 24 6月 201829 6月 2018

出版系列

姓名Springer Proceedings in Physics
219
ISSN(印刷版)0930-8989
ISSN(电子版)1867-4941

会议

会议15th International Symposium on Nuclei in the Cosmos, NIC 2018
国家/地区意大利
L'Aquila
时期24/06/1829/06/18

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