Non-linearity effects on the light-output calibration of light charged particles in CsI(Tl) scintillator crystals

Dell’Aquila, D.; Sweany, S.; Brown, K. W.; Chajęcki, Z.; Lynch, W. G.; Teh, F. C. E.; Tsang, C. Y.; Tsang, M.B.; Zhu, K.; Anderson, Carl E.; Anthony, A.; Barlini, S.; Barney, J.; Camaiani, A.; Jhang, G.; Crosby, Javier; Estee, J.; Ghazali, Mohd Sabri Mohd; Guan, Fenhai; Khanal, O.B.; Kodali, S.; Lombardo, I.; Manfredi, J.; Morelli, L.; Morfouace, P.; Niu, C. Y.; Verde, G.

doi:10.1016/j.nima.2019.03.065

Cited by 31 publications

(20 citation statements)

References 29 publications

(71 reference statements)

Supporting

Mentioning

Contrasting

Order By: Relevance

“…5, the energy response for Z = 1 isotopes exhibits insignificant non-linearity and slight difference among the isotopes in the energy range of 0 − 100 MeV in accordance with the results in Ref. [19]. For the heavy isotopes from He to Boron, however, the non-linearity is increasingly pronounced depending on the species.…”

Section: Energy Calibration Of the Csi(tl) Crystalssupporting

confidence: 90%

“…6. The trends of the fitting curves are consistent with the results of HiRA10 detectors [19], and a detailed discussion on the energy calibration of CsI(Tl) crystals can be found therein.…”

Section: Energy Calibration Of the Csi(tl) Crystalssupporting

confidence: 84%

“…With the set of data points for each isotope, the energy response of the CsI(Tl) can be calibrated. For Z = 1 isotopes, the calibration function is written as [19],…”

Section: Energy Calibration Of the Csi(tl) Crystalsmentioning

confidence: 99%

See 2 more Smart Citations

Track Recognition for the $ΔE-E$ Telescopes with Silicon Strip Detectors

Guan,

Wang,

Diao

et al. 2021

Preprint

View full text Add to dashboard Cite

For the high granularity and high energy resolution, Silicon Strip Detector (SSD) is widely applied in assembling telescopes to measure the charged particles in heavy ion reactions. In this paper, we present a novel method to achieve the track recognition in the SSD telescopes of the Compact Spectrometer for Heavy Ion Experiment (CSHINE). Each telescope consists of a singlesided silicon strip detector (SSSSD) and a double-sided silicon strip detector (DSSSD) backed by 3 × 3 CsI(Tl) crystals. Detector calibration, track reconstruction and coordinate transformation are implemented. Special decoding algorithm is developed for the multi track recognition procedure to deal with the multi-hit effect convoluted by charge sharing and the missing signals with certain probability. It is demonstrated that the track recognition efficiency of the method is ∼90% and ∼80% for the DSSSD-CsI and SSSSD-DSSSD events, respectively.

show abstract

Section: Energy Calibration Of the Csi(tl) Crystalssupporting

confidence: 90%

“…6. The trends of the fitting curves are consistent with the results of HiRA10 detectors [19], and a detailed discussion on the energy calibration of CsI(Tl) crystals can be found therein.…”

Section: Energy Calibration Of the Csi(tl) Crystalssupporting

confidence: 84%

See 1 more Smart Citation

Track Recognition for the $ΔE-E$ Telescopes with Silicon Strip Detectors

Guan,

Wang,

Diao

et al. 2021

Preprint

View full text Add to dashboard Cite

show abstract

“…Two types of wedge-shaped CsI(Tl)s were designed to be placed behind the annular double-sided silicon detectors (ADSSDs) to identify the light charged particles with the Δ − method. The properties of CsI(Tl)s with different shapes and sizes, such as energy resolution, light output nonuniformity and particle identification capability, were compared by using a -source and a radioactive beam of 15 C. The big-size CsI(Tl) was finally adopted to form the Δ − telescope due to better properties. The property differences of these two types of CsI(Tl)s can be interpreted based on the Geant4 simulation results.…”

Section: Introductionmentioning

confidence: 99%

“…[8,9,10,11], which decreases the energy resolution of crystals and further affects the particle-identification (PID) capability of the Δ − method. In this paper, we designed two types of wedgeshaped CsI(Tl)s to match the ADSSD size, then tested and compared their energy resolution, PID capability, and light output non-uniformity by using a -source and a radioactive beam of 15 C. Finally, we chose one shape with better properties as the detector of the telescope TA.…”

Section: Introductionmentioning

confidence: 99%