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15_01_2025
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ds50
gagg-nd
gssi-cryogroup
gagg-nd
01_07_2024
02_09_2024
08_10_2024
9be_gamma_n_8be_reaction
15_01_2025
15_07_2024
18_12_2024
23_10_2024
25_09_2024
29_07_2024
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gssi-cryogroup:gagg-nd:15_01_2025
(γ,n) reaction
compare neutron flux with different gamma sources (Th or U? for U, 2.4 MeV is close to the resonance energy)
increase the neutron flux by increasing source activity or Be target thickness
measurements with varying thicknesses of the PE moderator for MC validations
GAGG detector
Delayed coincidences and contamination values shall be finalized and inserted into the paper
thermal neutron Am-Be data processed
LaBr3 detector
measure the half-life of the
215
Po's mother nucleus,
219
Rn
systematic uncertainties need to be considered
producing fake data and process them with the same procedures as with the real data
consider a linear background model, instead of a flat one
adjust the time binning
check the fit method, use least square fitting (For ROOT: try “IEL” fit option)
adjust the energy window
Simulating the Am-Be neutron spectrum
Setup optimization (regarding crystal size, quality(cleaner than now) etc.)
deadline for the funding expense is this summer
Detector's possible application on the surface
surrounded by plastic scintialltors as muon veto and moderator
SIPM instead of photomultiplier
gssi-cryogroup/gagg-nd/15_01_2025.txt
· Last modified:
2026/06/09 12:05
by
127.0.0.1
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