論文

査読有り 筆頭著者
2020年9月3日

Relativistic magnetic reconnection in laser laboratory for testing an emission mechanism of hard-state black hole system

Physical Review E
  • K. F. F. Law
  • Y. Abe
  • A. Morace
  • Y. Arikawa
  • S. Sakata
  • S. Lee
  • K. Matsuo
  • H. Morita
  • Y. Ochiai
  • C. Liu
  • A. Yogo
  • K. Okamoto
  • D. Golovin
  • M. Ehret
  • T. Ozaki
  • M. Nakai
  • Y. Sentoku
  • J. J. Santos
  • E. d{\textquotesingle}Humi{\`{e } }res
  • Ph. Korneev
  • S. Fujioka
  • 全て表示

102
3
記述言語
英語
掲載種別
研究論文(学術雑誌)
DOI
10.1103/physreve.102.033202
出版者・発行元
American Physical Society ({APS})

Magnetic reconnection in a relativistic electron magnetization regime was observed in a laboratory plasma produced by a high-intensity, large energy, picoseconds laser pulse. Magnetic reconnection conditions realized with a laser-driven several kilotesla magnetic field is comparable to that in the accretion disk corona of black hole systems, i.e., Cygnus X-1. We observed particle energy distributions of reconnection outflow jets, which possess a power-law component in a high-energy range. The hardness of the observed spectra could explain the hard-state x-ray emission from accreting black hole systems.

リンク情報
DOI
https://doi.org/10.1103/physreve.102.033202
PubMed
https://www.ncbi.nlm.nih.gov/pubmed/33075864
Scopus
https://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=85093910784&origin=inward
Scopus Citedby
https://www.scopus.com/inward/citedby.uri?partnerID=HzOxMe3b&scp=85093910784&origin=inward
ID情報
  • DOI : 10.1103/physreve.102.033202
  • ISSN : 2470-0045
  • ISSN : 2470-0053
  • eISSN : 2470-0053
  • ORCIDのPut Code : 111564702
  • PubMed ID : 33075864
  • SCOPUS ID : 85093910784

エクスポート
BibTeX RIS