中文

利用 SKAO 理解脉冲星磁层

高能天体物理现象 2026-07-03 v1
作者: L. S. Oswald , A. Basu , M. Chakraborty , B. C. Joshi , N. Lewandowska , K. Liu , M. E. Lower , A. Philippov , X. Song , P. Tarafdar , J. van Leeuwen , A. L. Watts , P. Weltevrede , G. Wright , J. Benáček , A. Beri , S. Cao , P. Esposito , F. Jankowski , J. C. Jiang , A. Karastergiou , K. J. Lee , N. Rea , D. Vohl
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摘要

SKA 望远镜将在宽射电频段带来无与伦比的灵敏度，在南天拥有广阔的视场，并具备子阵能力，所有这些都使其成为研究脉冲星磁层的理想仪器。本章描述了在过去十年中脉冲星磁层物理学取得的进展，并详细说明了这些进展是如何通过现代射电望远镜，特别是 SKA 先导和探路者望远镜的进步而实现的。它解释了 SKA 望远镜将如何通过大规模监测巡天和对独特源及新发现的深入后续观测相结合，来变革脉冲星磁层物理学领域。最后，它描述了 AA* 和 AA4 配置可用的具体观测机会将如何在未来几年内实现解决脉冲星射电发射物理问题所必需的进展。

关键词

脉冲星磁层 SKA 射电发射 监测巡天 脉冲星物理 望远镜能力

引用

@article{arxiv.2607.05432,
  title  = {Understanding Pulsar Magnetospheres with the SKAO},
  author = {L. S. Oswald and A. Basu and M. Chakraborty and B. C. Joshi and N. Lewandowska and K. Liu and M. E. Lower and A. Philippov and X. Song and P. Tarafdar and J. van Leeuwen and A. L. Watts and P. Weltevrede and G. Wright and J. Benáček and A. Beri and S. Cao and P. Esposito and F. Jankowski and J. C. Jiang and A. Karastergiou and K. J. Lee and N. Rea and D. Vohl},
  journal= {arXiv preprint arXiv:2607.05432},
  year   = {2026}
}

备注

Published in Advancing Astrophysics with the SKA II (AASKAII), 2026 (arXiv:2606.20366). Report-no:AASKAII/Oswald01. Advancing Astrophysics with the SKA II (AASKAII) outlines the transformative scientific advances that will be enabled by the SKA telescopes. N.B. a version of this article was previously published as part of a Special Issue, linked at arxiv:2512.16157