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Positional correction of a 3D position-sensitive virtual Frisch-grid CZT detector for gamma spectroscopy and imaging based on a theoretical assumption

  • Younghak Kim ;Kichang Shin ;Aleksey Bolotnikov;Wonho Lee
    • Nuclear Engineering and Technology
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    • v.55 no.5
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    • pp.1718-1733
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    • 2023
  • The virtual Frisch-grid method for room-temperature radiation detectors has been widely used because of its simplicity and high performance. Recently, side electrodes were separately attached to each surface of the detectors instead of covering the entire detector surface with a single electrode. The side-electrode structure enables the measurement of the three-dimensional (3D) gamma-ray interaction in the detector. The positional information of the interaction can then be utilized to precisely calibrate the response of the detector for gamma-ray spectroscopy and imaging. In this study, we developed a 3D position-sensitive 5 × 5 × 12 mm3 cadmium-zinc-telluride (CZT) detector and applied a flattening method to correct detector responses. Collimated gamma-rays incident on the surface of the detector were scanned to evaluate the positional accuracy of the detection system. Positional distributions of the radiation interactions with the detector were imaged for quantitative and qualitative evaluation. The energy spectra of various radioisotopes were measured and improved by the detector response calibration according to the calculated positional information. The energy spectra ranged from 59.5 keV (emitted by 241Am) to 1332 keV (emitted by 60Co). The best energy resolution was 1.06% at 662 keV when the CZT detector was voxelized to 20 × 20 × 10.

Impacts of the calcination temperature on the structural and radiation shielding properties of the NASICON compound synthesized from zircon minerals

  • Islam G. Alhindawy;Hany Gamal;Aljawhara.H. Almuqrin;M.I. Sayyed;K.A. Mahmoud
    • Nuclear Engineering and Technology
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    • v.55 no.5
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    • pp.1885-1891
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    • 2023
  • The present work aims to fabricate Na1+xZr2SixP3-xO12 compound at various calcination temperatures based on the zircon mineral. The fabricated compound was calcinated at 250, 500, and 1000℃. The effect of calcination temperature on the structure, crystal phase, and radiation shielding properties was studied for the fabricated compound. The X-ray diffraction diffractometer demonstrates that, the monoclinic crystal phase appeared at a calcination temperature of 250℃ and 500℃ is totally transformed to a high-symmetry hexagonal crystal phase under a calcination temperature of 1000℃. The radiation shielding capacity was also qualified for the fabricated compounds using the Monte Carlo N-Particle transport code in the g-photons energy interval between 15keV and 122keV. The impacts of calcination temperature on the g-ray shielding behavior were clarified in the present study, where the linear attenuation coefficient was enhanced by 218% at energy of 122keV, when the calcination temperature increased from 250 to 1000℃, respectively.

A Study on the Apron Shielding Ratio According to Electromagnetic Radiation Energy (감마선 에너지에 따른 납치마의 차폐효과 분석)

  • Jang, Dong-Gun;Lee, Sang-Ho;Choi, Hyung-Seok;Son, Joo-Chul;Yoon, Chang-Yong;Ji, Yung-Sik;Cho, Yong-In;Lee, Hong Je;Yang, Seoung-Oh
    • Journal of radiological science and technology
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    • v.37 no.4
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    • pp.247-252
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    • 2014
  • The medical institution has been used electromagnetic radiation of various energy. But researchers are divided on whether using apron for radiation shielding will be effective or not. The purpose of present study was to analyze electromagnetic radiation shielding effect of apron by using Monte carlo simulation. 1 MBq electromagnetic radiation was emitted from 10-500 keV at 10 keV increments in Monte carlo simulation. Then shielded radiation dose difference was confirmed, when 0.25 mmPb shield use for shielding. As a results, shielding ratio was markedly decreased in high energy electromagnetic radiation. The radiation dose was inversely increased with 0.25 mmPb shielding.

A Study on the Comparison of HPGe Detector Response Data for Low Energy Photons Using MCNP, EGS, and ITS Codes (MCNP, EGS, ITS코드를 이용한 고순도 게르마늄 검출기의 저에너지 광자에 대한 반응 비교연구)

  • Kim, Soon-Young;Kim, Jong-Kyung;Kim, Jong-Oh;Kim, Bong-Hwan
    • Journal of Radiation Protection and Research
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    • v.21 no.2
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    • pp.125-129
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    • 1996
  • The energy response of HPGe detector for low energy Photons was determined by using three Monte Carlo codes. MCNP4A. EGS4, and CYLTRAN in ITS3. In this study. bare HPGe detector$(100 mm^2{\times}10mm)$ was used and a pencil beam was incident perpendicularly on the center of the detector surface. The photopeak efficiency, $K_{\alpha}$ and $K_{\beta}$ escape fractions were calculated as a function of incident X-ray energies ranging from 12 to 60 keV in 2-keV increments. Since the Compton. elastic. ana penetration fraction were negligible in this energy range. they were ignored in the calculation. Although MCNP. EGS, and CYLTRAN codes calculated slightly different energy response of HPGe detector for low energy Photons, it appears that the three Monte Carlo codes can Predict the low energy Photon scattering Processes accurately. The MCNP results, which are generally known as to be less accurate at low energy ranges than the EGS and ITS results. are comparable to the results of EGS and ITS and are applicable to the calculation of the low energy response data of a detector.

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A Theoretical Calculation of Photon Dose Equivalent Conversion Factor For Extremity Dosimeter (말단선량계의 광자선량당량환산인자에 대한 이론적 계산)

  • Kim, Kwang-Pyo;Lee, Won-Keun;Kim, Jong-Su;Yoon, Yeo-Chang;Yoon, Suk-Chul
    • Journal of Radiation Protection and Research
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    • v.21 no.1
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    • pp.41-50
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    • 1996
  • In this study, the theoretical calculation of the air kerma-to-dose equivalent conversion factors was performed with a Monte Carlo N-Particle transport code for the two types of extremity phantom of the ANSI and the KAERI, respectively. Considering the distribution of absorbed dose due to the interaction of homogeneous Parallel broad beam of monoenergetic primary photons in the range between 15keV and 1.5MeV, the air kerma-to-dose equivalent conversion factors based on the kerma approximation were calculated. It is showed that all the theoretical conversion factors of the two types of the extremity phantom for the ANSI and the KAERI agree well with the experimental values of the ANSI N13.32 draft(1995) for each energy within 5.7%, maximum difference ratio, except for 13.6%, difference ratio in the case for the energy of less than 40keV. It is due to uncertainties of experiment occurred in the low X-ray energy range and geometry considered in the MCNP code.

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Radiological Characterization of the High-sensitivity MOSFET Dosimeter (고감도 MOSFET 선량계 방사선학적 특성 연구)

  • Cho Sung Koo;Kim Chan-Hyeong
    • Progress in Medical Physics
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    • v.15 no.4
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    • pp.215-219
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    • 2004
  • Due to their excellence for the high-energy therapy range of photon beams, researchers show increasing interest in applying MOSFET dosimeters to low- and medium-energy applications. In this energy range, however, MOSFET dosimeter is complicated by the fact that the interaction probability of photons shows significant dependence on the atomic number, Z, due to photoelectric effect. The objective of this study is to develop a very detailed 3-dimensional Monte Carlo simulation model of a MOSFET dosimeter for radiological characterizations and calibrations. The sensitive volume of the High-Sensitivity MOSFET dosimeter is very thin (1 ${\mu}{\textrm}{m}$) and the standard MCNP tallies do not accurately determine absorbed dose to the sensitive volume. Therefore, we need to score the energy deposition directly from electrons. The developed model was then used to study various radiological characteristics of the MOSFET dosimeter. the energy dependence was quantified for the energy range 15 keV to 6 MeV; finding maximum dependence of 6.6 at about 40 keV. A commercial computer code, Sabrina, was used to read the particle track information from an MCNP simulation and count the tracks of simulated electrons. The MOSFET dosimeter estimated the calibration factor by 1.16 when the dosimeter was at 15 cm depth in tissue phantom for 662 keV incident photons. Our results showed that the MOSFET dosimeter estimated by 1.11 for 1.25 MeV photons for the same condition.

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An aspect of Gagok enjoyment in the early 19th century (19세기 초반, 가곡 향유의 한 단면 - 『영언』과『청륙』의 ‘이삭대엽 우ㆍ계면 배분방식’을 대상으로 -)

  • 성무경
    • Sijohaknonchong
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    • v.19 no.1
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    • pp.235-260
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    • 2003
  • Recently, I presented Gagok(歌曲) Collection Yeong-eon永言 to learned circles. Yeong-eon is very similar to Yukdang-version六堂本 CheongGuYeongeon靑丘永言. Compared with Cheong- Yuk, it is the same age or little bit early time of Cheong-Yuk in culture Icon. This paper paid attention to the considerable difference between Yeong-eon and Cheong-Yuk in the way of the distribution of Yisakdaeyap二數大 葉's Woo mode羽調 and Ke-myeon mode界面調. There was the way of gathering ‘real name’+‘namelessness’ in Yisakdaeyap, which is the feature of the 18th century Gagok Collection. I found this way just put on the 19th century Gagok Collection way which is the distribution of Yisakdaeyap's 'Woo mode and Ke-myeon mode' in CheongYuk. Then I proved in this paper that the way of gathering Yisakdaeyap in Cheong Yuk didn't correspond to an actual singing in the early 19th century when 'Woo mode and Ke-myeon mode' was fixed. In case of Yeong-eon, however, it was not written any writers' names at all, when it was researched retroactively, I knew it was distributed evenly both the works of 'real name' and 'namelessness' in Yisakdaeyaps 'Woo mode and Ke-myeon mode'. Consequently, I found Yeong-eon is the good Gagok Collection for an actual singing at that time. In addition, there was discord in the mode or key distribution among many Gagok Collections. I found this issue of the application had kept on make Gagok Collections edit during 2 centuries. Because the actual Gagok enjoyment in the specific time is connected the way of the mode application directly.

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Sheet Resistance of Ion Implanted Si(100) at Various Doses, Energies and Beam Currents (Si(100)에 이온 주입 시 에너지, 조사량과 빔 전류에 따른 면저항의 변화)

  • Kim, Hyung-In;Jeong, Young-Wan;Lee, Myeung-Hee;Kang, Suk-Tai
    • Journal of the Korean Vacuum Society
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    • v.20 no.2
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    • pp.100-105
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    • 2011
  • Simulations were performed using Crystal TRIM software under the same conditions used by previous researchers in order to clarify the mechanism that determines sheet resistance various doses, energies and beam currents. The results showed that the peak of the depth profile (Rp) in the same sample gradually shifts inward and damage increases near the surface as the energy increases for $As^+$ equal dose of $1{\times}10^{15}/cm^2$ implanted into Si(100) energies of 5, 10, and 15 keV. From a theoretical calculation of B+ ion implantation processes at energy of 20 keV using parameters that correspond to 1 mA and 7 mA beam currents with the same dose of $5{\times}10^{15}/cm^2$, it was found that the higher beam currents resulted in more damage near the surface (<100 nm). Likewise, In the simulations employing sets of doses ($1{\times}10^{15}$, $3{\times}10^{15}/cm^2$) and beam currents (0.8 mA, 8 mA), more damage was produced at larger doses and higher current. Thus, sheet resistance at the surface was reduced by the intensified damage from increases in beam energy, dose and beam currents.

A Study on the Energy and Time Characteristics of $BaF_2$ Scintillation Detector ($BaF_2$ 검출기의 시간과 에너지 특성연구)

  • Ju, Gwan-Sik;Park, Il-Jin;Kim, Jong-Ho;Nam, Gi-Yong;Baek, Seung-Hwa
    • Journal of Biomedical Engineering Research
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    • v.18 no.3
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    • pp.267-272
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    • 1997
  • he scintillation detector having $BaF^2$ crystal with 3.6cm dia${\times}$2.0 cm thick was provided. The energy and timing characteristics were measured and compared with NaI(Tl) scintillation detectors, which widely used in unclear medicine. In order to measure the energy spectrum, the radioactive sources used were $^{22}Na,\;^{54}Mn,\;^{57}Co,\;^{137}Cs$ and the source to detector distance was 7cm. For the timing characteristic, NaI(Tl)(1" ${\times}$ 1")-$BaF^2$ and NaI(Tl)(3" ${\times}$ 3")-$BaF^2$ timing coincidence systems were prepared and the used source was $^{22}Na$ emitting 511keV annihilation photons. For the 511keV gamma-ray emitted from $^{22}Na$, It was revealed that the timing response of the $BaF^2$ detector was faster than NaI(Tl)(1" ${\times}$ 1") and NaI(Tl)(3" ${\times}$ 3") detector used in this experimental investigation. The energy characteristics of the $BaF^2$ detector had a good values for about 500keV energy range.

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A Comparative Study of Branching Ratio of 167Yb Radioactive Isotope from Gamma-ray Spectrum Produced by 169Tm(p,3n)167Yb Reaction with 100-MeV Proton Beam (100-MeV 양성자 빔을 이용하여 169Tm(p,3n)167Yb 반응에 의해 생성된 167Yb 방사성동위원소에서 방출되는 감마선 스펙트럼 비교 연구)

  • Sam-Yol, Lee
    • Journal of the Korean Society of Radiology
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    • v.16 no.7
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    • pp.953-960
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    • 2022
  • The measurement of branching ratio of 167Yb radioactive isotopes from gamma-ray spectrum of 169Tm(p,3n)167Yb reaction were performed by using a 100-MeV proton linear accelerator of the Korea Multi-purpose Accelerator Complex (KOMAC). The 167Yb isotope has a half-life of 17.5 minutes and decays to 169Tm. The gamma rays generated from the 167Yb isotope were measured using an HPGe detector gamma ray spectroscopy system. The energy calibration of the detector and the efficiency measurement of the detector were determined using a standard source. The gamma rays of known main energy (62.9, 106.2, 113.3, 143.5 and 176.3 keV) were measured. On the other hand, information about the intensity of the generated gamma rays is very inaccurate. Therefore, in this study, the decay strength of the main gamma rays was accurately measured. Overall, it was different from the previously known results, and in particular, it was found that the intensity of the main decay gamma ray, such as the 113.3 and 106.2 keV gamma ray, was overestimated, and it was found that the gamma ray, such as 62.9, 116.7 and 143.5 keV was underestimated. The present results are considered to be important information in the fields of nuclear fusion, astrophysics and nuclear physics in the future.