scholarly journals Improved STEREO simulation with a new gamma ray spectrum of excited gadolinium isotopes using FIFRELIN

2019 ◽  
Vol 55 (10) ◽  
Author(s):  
H. Almazán ◽  
L. Bernard ◽  
A. Blanchet ◽  
A. Bonhomme ◽  
C. Buck ◽  
...  

Abstract. The STEREO experiment measures the electron antineutrino spectrum emitted in a research reactor using the inverse beta decay reaction on H nuclei in a gadolinium loaded liquid scintillator. The detection is based on a signal coincidence of a prompt positron and a delayed neutron capture event. The simulated response of the neutron capture on gadolinium is crucial for the comparison with data, in particular in the case of the detection efficiency. Among all stable isotopes, 155Gd and 157Gd have the highest cross sections for thermal neutron capture. The excited nuclei after the neutron capture emit gamma rays with a total energy of about 8MeV. The complex level schemes of 156Gd and 158Gd are a challenge for the modeling and prediction of the deexcitation spectrum, especially for compact detectors where gamma rays can escape the active volume. With a new description of the Gd (n,$ \gamma$γ) cascades obtained using the FIFRELIN code, the agreement between simulation and measurements with a neutron calibration source was significantly improved in the STEREO experiment. A database of ten millions of deexcitation cascades for each isotope has been generated and is now available for the user.

2002 ◽  
Vol 90 (8) ◽  
Author(s):  
G. L. Molnár ◽  
T. Belgya ◽  
Zs. Révay ◽  
Syed M. Qaim

SummaryAccurate partial gamma-ray production cross sections were determined for the prompt and radioactive product decay gamma rays following cold neutron capture in


1985 ◽  
Vol 25 (1) ◽  
pp. 265
Author(s):  
Sami O. Ajam ◽  
V.E. Rahal

The Thermal Multigate Decay (TMD) logging system utilizes a pulsed 14 Mev generator and two gamma ray detectors to obtain measurements of the capture cross sections of downhole formations. The composite decay curve from both formation and borehole capture gamma rays is detected, and is separated into the two individual components : sigma formation and sigma borehole. The resulting sigma formation measurement is only minimally affected by borehole conditions, especially in cased wells.In addition to sigma formation and sigma borehole, the TMD system generates a dual-spaced porosity ratio and several other parameters which provide information on log quality, borehole parameters, and tool stability. These features can be used to assist the log analyst in understanding the down- hole borehole environment as well as formation characteristics. Under appropriate conditions, the TMD log can also provide production logging information relating to fluid movement in or near the wellbore.The paper briefly reviews the TMD logging system, after which it concentrates on log examples in unusual borehole conditions : logs run across intervals where borehole conditions change; logs run in air filled boreholes; logs run in badly washed out boreholes; logs run through stuck drill pipe/ collars; logs run in flowing wells. The supplemental TMD curves in these situations identify the presence of gravel packs and packers, changes in borehole fluid salinity, possible communication between zones, and water and oil producing perforations. Gas in the borehole can also be clearly differentiated from gas in the formation.


1980 ◽  
Vol 20 (05) ◽  
pp. 341-348 ◽  
Author(s):  
William C. Pritchett

Introduction Laboratory and borehole measurements of shale properties may be unreliable because of modification during or after drilling or coring. The borehole gravimeter is an ideal tool for measuring the bulk density of thick shale units because of its great depth of investigation and negligible sensitivity to shale in the vicinity of the borehole, which may have been modified in drilling. By contrast, the scatter gamma ray density log has an extremely shallow depth of investigation and its response may be dominated by modified shale surrounding a borehole. A comparison of bulk densities measured by these two methods in both sands and shales was made in three U.S. gulf coast wells. In all three wells the two methods yielded comparable densities for the sands. But in two wells, which were drilled with fresh muds, the density log yielded shale bulk densities significantly less than those shown by the borehole gravimeter. These data indicate that shale adjacent to the borehole in these two wells had been modified by drilling and the modified shale densities had been reduced significantly. In the well drilled with a saline mud, bulk densities from the two methods were in close agreement in both sands and shales, which indicates that shales adjacent to the borehole in this well were not modified significantly. High-pressure shales are particularly susceptible to modification during drilling since they are relatively permeabble and soft. Sometimes they even flow. Density log data in high-pressure shales are unreliable due to probable shale modification. Unfortunately, we have no borehole gravimeter data in high. pressure shales and, therefore, no reliable measurements of bulk densities in their natural state. The best data available for studying high-pressure shales are some neutron lifetime logs. The effective depth of investigation of the neutron lifetime log is considerably greater than that of the scatter gamma ray density log.1,2 Therefore, neutron lifetime log measurements should be affected much less by any modified shale near the borehole than would measurements made with a density log. Neutron lifetime logs show a progressive decrease in macroscopic neutron capture cross section with increasing depth for U.S. gulf coast shales with normal pore pressures. This decrease in neutron capture cross section is the result of increased compaction of shales with depth. If high-pressure shales are shales that were not compacted normally with increasing depth of burial, then they should have physical properties comparable with relatively uncompacted shales at much shallower depths of a few thousand feet (1000 to 1500 m). In particular, they should have high neutron capture cross sections as compared with normally pressured shales at slightly shallower depths. However, our logs show neutron capture cross sections for U.S. gulf coast high-pressure shales that range from normal to less than normal for their depths. These data indicate that these high-pressure shales are not shales that were never compacted. The data are consistent with an alternate hypothesis for the generation of high pore pressures in shales.


1999 ◽  
Vol 36 (10) ◽  
pp. 855-864 ◽  
Author(s):  
Teerasak VEERAPASPONG ◽  
Masayuki IGASHIRA ◽  
Satoshi MIZUNO ◽  
Jun-ichi HORI ◽  
Toshiro OHSAKI

1957 ◽  
Vol 35 (12) ◽  
pp. 1347-1360 ◽  
Author(s):  
G. A. Bartholomew ◽  
P. J. Campion

The neutron capture γ-rays from Li7, B11, and N15 have been studied. In Li7 γ-rays are observed at 7.26 ± 0.03 Mev. and 6.78 ± 0.05 Mev. In B11 six γ-rays are detected. The spectrum is consistent with J = 7/2 + for the capturing state. In N15 six previously unreported γ-rays are detected. Estimates of thermal neutron radiative capture cross sections are: Li6, 0.028 ± 0.008 b.; B10, 0.5 ± 0.2 b.; and N14, 0.08 ± 0.02 b.


2014 ◽  
Vol 51 (5) ◽  
pp. 671-680
Author(s):  
Kazushi Terada ◽  
Taihei Matsuhashi ◽  
Masayuki Igashira ◽  
Tatsuya Katabuchi

2000 ◽  
Vol 37 (9) ◽  
pp. 740-749 ◽  
Author(s):  
Suhe HARNOOD ◽  
Masayuki IGASHIRA ◽  
Tetsuro MATSUMOTO ◽  
Satoshi MIZUNO ◽  
Toshiro OHSAKI

Author(s):  
Dong Wang ◽  
Bin He ◽  
Quanhu Zhang

Boron loaded plastic scintillator could detect both fast neutrons (thanks to hydrogen) and slow neutrons (thanks to 10B). The large cross sections of both reactions lead to high detection efficiency of incident neutrons. However, gamma rays must be rejected first as the scintillator is also sensitive to them. In the present research zero crossing method was used to test neutron-gamma discrimination performance of BC454 boron loaded plastic scintillator. Three contrast experiments were carried out and different thermalization degrees lead to different time spectra in the MCA. Further analysis proved that three Gaussian curves could be used to fit the spectra; they corresponded to gamma rays, fast neutrons and slow neutrons respectively. The slow neutron curve could be clearly separated from the gamma curve. Discrimination performance for fast neutrons became poor, but their peaks could also be separated.


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