Abstract
Abstract
The accurate information regarding the β-decay
half-life, feeding pattern from the neutron-rich nuclei have utmost
importance in the field of nuclear waste management from the fission
reactors as well as correct understanding about the r-process
nucleosynthesis in stellar sites. The low capture cross-section
measurements are also considered as major task by experimental
nuclear astrophysicists. These kinds of measurements are really
difficult with conventional high-resolution gamma spectroscopy
techniques due to less efficiency of the detectors. For this
purpose, we have an almost 4π γ-summing NaI(Tl)
spectrometer at SINP, Kolkata. It is basically a cylindrical shaped
detector with six sectors of NaI(Tl) crystals read by 6
photomultiplier tubes (PMT) at one end. The detailed
characterization of the spectrometer via experiment using laboratory
standard sources and GEANT4 simulation model to interpret all the
interesting properties will be presented here in this paper.
Subject
Mathematical Physics,Instrumentation