19–24 May 2024
Music City Center
US/Central timezone

The gamma activation measurements at Shanghai Laser Electron Gamma Source

THPR86
23 May 2024, 16:00
2h
Rock 'n Roll (MCC Exhibit Hall A)

Rock 'n Roll

MCC Exhibit Hall A

Poster Presentation MC8.U09 Other Applications Thursday Poster Session

Speaker

Yuxuan Yang (Shanghai Institute of Applied Physics)

Description

SLEGS is a Laser Compton Scattering gamma source. The gamma energy is 0.66 to 21.7 MeV, and the gamma flux is approximately 4.8e+5 to 1.5e+7 phs/s. Gamma activation method is used in beam flux monitor, medical isotpoe production and nuclear astrophysics in SLEGS. Gamma beam flux under different collimated apertures has been checked by gamma activation method by using various half-life nuclide targets with an online activation and offline measurement platform. It is consistent with the flux measured with direct method by the LaBr3 detector. The activation method will be uniquely advantageous for monitoring gamma beam with short-life nuclide in a short time.A series of potential medical isotopes giant resonance production cross sections are measured by gamma activation method, which will provide key data for medical isotopes production by photonuclear reactions. The p-nuclei’s photonuclear cross sections*, for example Ru, are measured by photoneutron and gamma activation, which can provide favorable data on the much larger abundance of 98Ru, 96Ru. The activation experiment of SLEGS provides a reliable option for different experimental research objectives in photonuclear physics.

Footnotes

  • Wang H W, Fan G T, Liu L X, et al., Commissioning of Laser Electron Gamma Beamline SLEGS at SSRF[J], Nuclear Science and Techniques, 2022, 33, 87.
    **Gy. Gyürky, Zs. Fülöp, F. Käppeler, G. G. Kiss, and A. Wallner, The Activation Method for Cross Section Measurements in Nuclear Astrophysics[J], Eur. Phys. J. A 55, 41 (2019).
Region represented Asia
Paper preparation format LaTeX

Primary author

Yuxuan Yang (Shanghai Institute of Applied Physics)

Co-authors

Hongwei Wang (Shanghai Synchrotron Radiation Facility) Gongtao Fan (Shanghai Synchrotron Radiation Facility) Hanghua Xu (Shanghai Advanced Research Institute) Longxiang Liu (Shanghai Advanced Research Institute) Yue Zhang (Shanghai Advanced Research Institute) Xiguang Cao (Shanghai Advanced Research Institute) Zirui Hao (Shanghai Institute of Applied Physics)

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