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Non-extensive Solution to Cosmological Lithium Problem

  • S. Q. Hou*
  • , J. J. He
  • , A. Parikh
  • , D. Kahl
  • , C. A. Bertulani
  • , Toshitaka Kajino
  • , Grant J. Mathews
  • , G. Zhao
  • *此作品的通讯作者
  • CAS - Institute of Modern Physics
  • CAS - National Astronomical Observatories
  • Polytechnic University of Catalonia
  • Institute of Space Studies of Catalonia
  • University of Edinburgh
  • Texas A&M University-Commerce
  • The University of Tokyo
  • National Astronomical Observatory of Japan
  • 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

The standard Big-Bang model predicts the primordial abundances of H(D), He, He in excellent agreement with observations, except for Li that is overpredicted by a factor of about three. Despite many attempted solutions to this discrepancy using conventional nuclear physics over the past decades, the lithium enigma persists. Here we present an investigation of Big Bang nucleosynthesis (BBN) predictions when we adopt a non-extensive distribution to describe the velocity profile of the nuclides in the primordial plasma. We find excellent agreement between predicted and observed primordial abundances of D, He, Li for the case of, which indicates a possible new solution to the cosmological lithium problem.

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
39-43
页数5
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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