MCNPX simulation of influence of cosmic rays on low-activity spectrometric measurements
Identifikátory výsledku
Kód výsledku v IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00177016%3A_____%2F12%3A%230000784" target="_blank" >RIV/00177016:_____/12:#0000784 - isvavai.cz</a>
Nalezeny alternativní kódy
RIV/00177016:_____/14:#0000866
Výsledek na webu
<a href="http://dx.doi.org/10.1016/j.radphyschem.2012.12.034" target="_blank" >http://dx.doi.org/10.1016/j.radphyschem.2012.12.034</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1016/j.radphyschem.2012.12.034" target="_blank" >10.1016/j.radphyschem.2012.12.034</a>
Alternativní jazyky
Jazyk výsledku
angličtina
Název v původním jazyce
MCNPX simulation of influence of cosmic rays on low-activity spectrometric measurements
Popis výsledku v původním jazyce
Germanium gamma spectrometers are effective instruments for low-activity measurement of a mixture of radionuclides in environmental samples, food samples, in materials released from nuclear facilities to the environment, etc. In such measurements cosmicrays have a signi?cant contribution to the background signal. A Monte Carlo code MCNPX was used to calculate coaxial high-purity germanium (HPGe) detector pulse-height spectra caused by cosmic rays penetrating through shielding made of concrete and lead.Simulations were compared to two different measurements, one performed inside a 10 cm thick lead shielding and another done inside a larger chamber made of low-activity concrete and with several ceiling thicknesses. In the ?rst experiment, a discrepancywas found between simulated and measured spectra by up to the factor of 4 at 2.62 MeV and slowly decreasing to unity at 13 MeV. It is assumed that the discrepancy between the measured and simulated spectra is caused by the simpli?cation
Název v anglickém jazyce
MCNPX simulation of influence of cosmic rays on low-activity spectrometric measurements
Popis výsledku anglicky
Germanium gamma spectrometers are effective instruments for low-activity measurement of a mixture of radionuclides in environmental samples, food samples, in materials released from nuclear facilities to the environment, etc. In such measurements cosmicrays have a signi?cant contribution to the background signal. A Monte Carlo code MCNPX was used to calculate coaxial high-purity germanium (HPGe) detector pulse-height spectra caused by cosmic rays penetrating through shielding made of concrete and lead.Simulations were compared to two different measurements, one performed inside a 10 cm thick lead shielding and another done inside a larger chamber made of low-activity concrete and with several ceiling thicknesses. In the ?rst experiment, a discrepancywas found between simulated and measured spectra by up to the factor of 4 at 2.62 MeV and slowly decreasing to unity at 13 MeV. It is assumed that the discrepancy between the measured and simulated spectra is caused by the simpli?cation
Klasifikace
Druh
J<sub>x</sub> - Nezařazeno - Článek v odborném periodiku (Jimp, Jsc a Jost)
CEP obor
BG - Jaderná, atomová a molekulová fyzika, urychlovače
OECD FORD obor
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Návaznosti výsledku
Projekt
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Návaznosti
R - Projekt Ramcoveho programu EK
Ostatní
Rok uplatnění
2014
Kód důvěrnosti údajů
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Údaje specifické pro druh výsledku
Název periodika
Radiation Physics and Chemistry
ISSN
0969-806X
e-ISSN
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Svazek periodika
2014
Číslo periodika v rámci svazku
95
Stát vydavatele periodika
GB - Spojené království Velké Británie a Severního Irska
Počet stran výsledku
4
Strana od-do
181-184
Kód UT WoS článku
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EID výsledku v databázi Scopus
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