Author: Hayakawa, Y.
Paper Title Page
THPOJO22 A Ground Experimental Approach Toward Understanding Mysterious Astrophysical Fast Radio Bursts 735
THOPA03   use link to see paper's listing under its alternate paper code  
  • Y. Sumitomo, T. Asai, D. Kobayashi, S. Kumagai, K. Kusaka, Y. Onishi, T. Seki, R. Yanagi
    Nihon University, Tokyo, Japan
  • Y. Hayakawa, T. Sakai
    LEBRA, Funabashi, Japan
  • S. Kisaka
    HU ADSE, Hiroshima, Japan
  • H. Koguchi
    AIST, Tsukuba, Japan
  Funding: Nihon University CST Project Research Grant (2021 Apr. ~), Japan Society for the Promotion of Science (JSPS), Grant-in-Aid for Scientific Research (KAKENHI), Grant Number JP19K12631
The Fast Radio Bursts are astrophysical events that get much more attentions increasing year by year, due to their mysterious properties of signals. The major properties of signals include a class of the brightest astrophysical events, short durations of emissions, and larger dispersion measures than the known short duration events. Interestingly, the large values of dispersion measures suggest the existence of abundant plasma around the parent bodies of emissions. To have a better understanding of basic mechanism of the Fast Radio Burst emissions, we initiated a ground-based research project at our 100 MeV electron LINAC facility, in combination with the high-beta plasma generation knowledge matured also at Nihon University, that mimics plasma fields in space. In this presentation, we overview our project and report on the status of the experiment for the induced enhanced emissions from integrated iterative interactions with plasma fields.
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About • Received ※ 12 August 2022 — Revised ※ 21 August 2022 — Accepted ※ 31 August 2022 — Issue date ※ 23 September 2022
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