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2021 Fiscal Year Research-status Report

Combined Spectrum and Anisotropy Study of Cosmic Rays from the Vela SNR with CALET

Research Project

Project/Area Number 21K03604
Research InstitutionWaseda University

Principal Investigator

Motz Holger  早稲田大学, 理工学術院, 准教授(任期付) (30647904)

Project Period (FY) 2021-04-01 – 2024-03-31
KeywordsHigh Energy Cosmic Rays / Vela Supernova Remnant / Cosmic Ray Anisotropy / Cosmic Ray Propagation
Outline of Annual Research Achievements

Initially, as a benchmark point for the further studies, limits and best-fit values for the total energy of electron cosmic ray emission from the Vela supernova remnant have been calculated based on a standard binned analysis method and for generic emission scenarios (delayed instantaneous release, constant release for a duration). These results were shown at ICRC2021 and published in the proceedings.
Noticing the dependence of the predictions on the cosmic-ray propagation conditions, the underlying propagation models were improved by optimizing the parameters used in the numerical DRAGON calculation of the nuclei spectra in a random walk, until a model explaining the measured nuclei spectra up to oxygen with a common injection spectrum for all nuclei was found. This model explains the differences in the measured nuclei spectra by propagation effects only, without the need for species-specific acceleration mechanisms. Focusing on such well supported propagation conditions allows for more concrete predictions of the spectral and anisotropy signal from Vela, but the model is also useful in other areas such as indirect dark matter search with CALET, and has been first presented in this context.
As planned, an unbinned likelihood analysis method for the electron spectrum has been developed, which can identify a potential spectral hardening in the TeV-region based on the few expected events with high significance, according to simulations. Such a hardening could be considered a spectral signature from the Vela SNR, which would be further supported by an anisotropy signature.

Current Status of Research Progress
Current Status of Research Progress

2: Research has progressed on the whole more than it was originally planned.

Reason

Compared to the schedule in the research plan, more focus was put on and more progress made in improving the underlying propagation model, delaying further study of more detailed emission scenarios for the Vela SNR. However, by reducing the number of propagation scenarios that have to be studied, more concrete predictions and faster progress is expected in the future.

Strategy for Future Research Activity

It is planned to combine the unbinned likelihood analysis method for anisotropy (explained in the research plan) with the newly developed unbinned likelihood method for the spectrum. The sensitivity of the combined likelihood method to the different scenarios of cosmic-ray flux from Vela is then to be studied through extensive simulations. In this process, also the study of more sophisticated emission scenarios is foreseen.
Still, further improvement and validation of the propagation model, in order to explain also the antiproton spectrum data, and that of nuclei up to iron and nickel, will also be undertaken.

Causes of Carryover

30 yen is a too small amount to buy any items meaningful to the project. Merged with the next fiscal year's budget it can be spent according to the plan.

  • Research Products

    (6 results)

All 2022 2021

All Journal Article (1 results) (of which Int'l Joint Research: 1 results,  Open Access: 1 results) Presentation (5 results) (of which Int'l Joint Research: 2 results)

  • [Journal Article] Investigating the Vela SNR's Emission of Electron Cosmic Rays with CALET at the International Space Station2021

    • Author(s)
      Holger Motz on behalf of the CALET collaboration
    • Journal Title

      Proceedings of Science

      Volume: ICRC2021 Pages: 100

    • DOI

      10.22323/1.395.0100

    • Open Access / Int'l Joint Research
  • [Presentation] Indirect Search for Heavy Dark Matter with CALET2022

    • Author(s)
      Holger Motz
    • Organizer
      The Physical Society of Japan 2022 Annual Meeting
  • [Presentation] Search for TeV-Range Dark Matter with Electron and Positron Cosmic Rays2022

    • Author(s)
      Holger Motz
    • Organizer
      FY2021 学術変革領域研究「ダークマター」シンポジウム
  • [Presentation] Investigating the Vela SNR's Emission of Electron Cosmic Rays with CALET at the International Space Station2021

    • Author(s)
      Holger Motz on behalf of the CALET collaboration
    • Organizer
      37th International Cosmic Ray Conference (ICRC 2021)
    • Int'l Joint Research
  • [Presentation] Search for Signatures of Nearby Supernova Remnants with CALET2021

    • Author(s)
      Holger Motz for the CALET Collaboration
    • Organizer
      The Physical Society of Japan 2021 Autumn Meeting
  • [Presentation] Extending Dark Matter Limits from Electron and Positron Cosmic Rays to the TeV-region2021

    • Author(s)
      Holger Motz
    • Organizer
      Kashiwa Dark Matter Symposium
    • Int'l Joint Research

URL: 

Published: 2022-12-28  

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