19–21 Nov 2021
美豪丽致酒店
Asia/Shanghai timezone

Session

Axion

20 Nov 2021, 10:45
美豪丽致酒店

美豪丽致酒店

上海市闵行区石坪路499号

Conveners

Axion: Session-1

  • Jing Shu (ITP, CAS)
  • Shao-Feng Ge (TDLI-SJTU)
  • Yong Yang (Shanghai Jiao Tong University)

Axion: Session-2

  • Jing Shu (ITP, CAS)
  • Yong Yang (Shanghai Jiao Tong University)
  • Shao-Feng Ge (TDLI-SJTU)

Description

https://cern.zoom.us/j/66814713888?pwd=QTJGWkpFNTVRRUxzZWFnNWozazBxdz09
Meeting ID: 668 1471 3888
Password:2021

Presentation materials

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  1. Prof. Jia Liu (Peking University)
    20/11/2021, 10:45
  2. Dr Yuan-Han Chang (Academia Sinica)
    20/11/2021, 11:05
  3. Dr Yifan Chen (ITP, CAS)
    20/11/2021, 11:25
  4. Dr Min Jiang (University of Science and Technology of China)
    20/11/2021, 11:45
  5. Nick Houston (BJUT)
    20/11/2021, 12:05

    Axions provide a natural and well-motivated dark matter candidate, with the capability to convert directly to photons in the presence of an electromagnetic field. A particularly compelling observational target is the conversion of dark matter axions into photons in the magnetospheres of highly magnetised neutron stars, which is expected to produce a narrow spectral peak centred at the...

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  6. Prof. Yannis K. Semertzidis
    20/11/2021, 15:50
  7. Dr Kanioar Karan (Cardiff University)
    20/11/2021, 16:10
  8. Xiaopeng Zhou
    20/11/2021, 16:30
  9. Prof. Fei Gao (Tsinghua University)
    20/11/2021, 16:50
  10. Dr Yun-Long Zhang (NAOC, CAS)
    20/11/2021, 17:10

    Abstract: The axion objects such as axion mini-clusters and axion clouds around spinning black holes induce parametric resonances of electromagnetic waves through the axion-photon interaction. In particular, it has been known that the resonances from the axion with the mass around mueV may explain the observed fast radio bursts (FRBs). Here we argue that similar bursts of high-frequency...

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