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Institute
The experimental area 2 (EAR-2) at CERNs neutron time-of-flight facility (n_TOF), which is operational since 2014, is designed and built as a short-distance complement to the experimental area 1 (EAR-1). The Parallel Plate Avalanche Counter (PPAC) monitor experiment was performed to characterize the beam pro↓le and the shape of the neutron 'ux at EAR-2. The prompt γ-flash which is used for calibrating the time-of-flight at EAR-1 is not seen by PPAC at EAR-2, shedding light on the physical origin of this γ-flash.
Monte Carlo (MC) simulations are an essential tool to determine fundamental features of a neutron beam, such as the neutron flux or the γ-ray background, that sometimes can not be measured or at least not in every position or energy range. Until recently, the most widely used MC codes in this field had been MCNPX and FLUKA. However, the Geant4 toolkit has also become a competitive code for the transport of neutrons after the development of the native Geant4 format for neutron data libraries, G4NDL. In this context, we present the Geant4 simulations of the neutron spallation target of the n_TOF facility at CERN, done with version 10.1.1 of the toolkit. The first goal was the validation of the intra-nuclear cascade models implemented in the code using, as benchmark, the characteristics of the neutron beam measured at the first experimental area (EAR1), especially the neutron flux and energy distribution, and the time distribution of neutrons of equal kinetic energy, the so-called Resolution Function. The second goal was the development of a Monte Carlo tool aimed to provide useful calculations for both the analysis and planning of the upcoming measurements at the new experimental area (EAR2) of the facility.
The transition from the marine to the terrestrial realm is one of the most fascinating issues in evolutionary biology for it required the appearance, in different organisms, of several novel adaptations to deal with the demands of the new realm. Adaptations include, for instance, modifications in different metabolic pathways, development of body structures to facilitate movement and respiration, or tolerance to new conditions of stress. The transition to the land also gives an extraordinary opportunity to study whether evolution used similar changes at the genomic level to produce parallel adaptations in different taxa. Mollusks are among taxa that were successful in the conquest of the land. For instance, several lineages of the molluscan clade Panpulmonata (Gastropoda, Heterobranchia) invaded the intertidal, freshwater and land zones from the marine realm. In my dissertation, using tools from bioinformatics, phylogenetics, and molecular evolution, I used panpulmonates as a suitable model group to study the independent invasions into the terrestrial realm and the adaptive signatures in genes that may have favored the realm transitions. My work includes two peer-reviewed published papers and one manuscript under review. In Publication 1 (Romero et al., 2016a), I used mitochondrial and nuclear molecular markers to resolve the phylogeny of the Ellobiidae, a family that possesses intertidal and terrestrial species. The phylogeny provided an improved resolution of the relationships within inner clades and a framework to study the tempo and mode of the land transitions. I showed that the terrestrialization events occurred independently, in different lineages (Carychiinae, Pythiinae) and in different geological periods (Mesozoic, Cenozoic). In addition, the diversification in this group may not have been affected by past geological or climate changes as the Cretaceous-Paleogene (K-Pg) event or the sea-level decrease during the Oligocene. In Publication 2 (Romero et al., 2016b), I generated new mitochondrial genomes from terrestrial species and compared them with other panpulmonates. I used the branch-site test of positive selection and detected significant nonsynonymous changes in the terrestrial lineages from Ellobioidea and Stylommatophora. Two genes appeared under positive selection: cob (Cytochrome b) and nad5 (NADH dehydrogenase 5). Surprisingly, I found that the same amino acid positions in the proteins encoded by these genes were also under positive selection in several vertebrate lineages that transitioned between different habitats (whales, bats and subterranean rodents). This result suggested an adaptation pattern that required parallel genetic modifications to cope with novel metabolic demands in the new realms. In Manuscript 1 (Romero et al., under review), I de novo assembled transcriptomes from several panpulmonate specimens resulting in thousands of genes that were clustered in 702 orthologous groups. Again, I applied the branch-site test of positive selection in the terrestrial lineages from Ellobioidea and Stylommatophora and in the freshwater lineages from Hygrophila and Acochlidia. Different sets of genes appeared under positive selection in land and freshwater snails, supporting independent adaptation events. I identified adaptive signatures in genes involved in gas-exchange surface development and energy metabolism in land snails, and genes involved in the response to abiotic stress factors (radiation, desiccation, xenobiotics) in freshwater snails. My work provided evidence that supported multiple land invasions within Panpulmonata and provided new insights towards understanding the genomic basis of the adaptation during sea-to-land transitions. The results of my work are the first reports on the adaptive signatures at the codon level in genes that may have facilitated metabolic and developmental changes during the terrestrialization in the phylum Mollusca. Moreover, they contribute to the current debate on the conquest of land from the marine habitat, a discussion that has been only based in vertebrate taxa. Future comparative genome-wide analyses would increase the number of genes that may have played a key role during the realm transitions.
An accurate measurement of the 140Ce(n,γ) energy-dependent cross-section was performed at the n_TOF facility at CERN. This cross-section is of great importance because it represents a bottleneck for the s-process nucleosynthesis and determines to a large extent the cerium abundance in stars. The measurement was motivated by the significant difference between the cerium abundance measured in globular clusters and the value predicted by theoretical stellar models. This discrepancy can be ascribed to an overestimation of the 140Ce capture cross-section due to a lack of accurate nuclear data. For this measurement, we used a sample of cerium oxide enriched in 140Ce to 99.4%. The experimental apparatus consisted of four deuterated benzene liquid scintillator detectors, which allowed us to overcome the difficulties present in the previous measurements, thanks to their very low neutron sensitivity. The accurate analysis of the p-wave resonances and the calculation of their average parameters are fundamental to improve the evaluation of the 140Ce Maxwellian-averaged cross-section.
Neutron capture on 241Am plays an important role in the nuclear energy production and also provides valuable information for the improvement of nuclear models and the statistical interpretation of the nuclear properties. A new experiment to measure the 241Am(n, γ) cross section in the thermal region and the first few resonances below 10 eV has been carried out at EAR2 of the n_TOF facility at CERN. Three neutron-insensitive C6D6 detectors have been used to measure the neutron-capture gamma cascade as a function of the neutron time of flight, and then deduce the neutron capture yield. Preliminary results will be presented and compared with previously obtained results at the same facility in EAR1. In EAR1 the gamma-ray background at thermal energies was about 90% of the signal while in EAR2 is up to a 25 factor much more favorable signal to noise ratio. We also extended the low energy limit down to subthermal energies. This measurement will allow a comparison with neutron capture measurements conducted at reactors and using a different experimental technique.
Although the 12C(n,p)12B and 12C(n,d)11B reactions are of interest in several fields of basic and applied Nuclear Physics the present knowledge of these two cross-sections is far from being accurate and reliable, with both evaluations and data showing sizable discrepancies. As part of the challenging n_TOF program on (n,cp) nuclear reactions study, the energy differential cross-sections of the 12C(n,p)12B and 12C(n,d)11 B reactions have been measured at CERN from the reaction thresholds up to 30 MeV neutron energy. Both measurements have been recently performed at the long flight-path (185 m) experimental area of the n_TOF facility at CERN using a pure (99.95%) rigid graphite target and two silicon telescopes. In this paper an overview of the experiment is presented together with a few preliminary results.
The study of neutron-induced reactions is of high relevance in a wide variety of fields, ranging from stellar nucleosynthesis and fundamental nuclear physics to applications of nuclear technology. In nuclear energy, high accuracy neutron data are needed for the development of Generation IV fast reactors and accelerator driven systems, these last aimed specifically at nuclear waste incineration, as well as for research on innovative fuel cycles. In this context, a high luminosity Neutron Time Of Flight facility, n_TOF, is operating at CERN since more than a decade, with the aim of providing new, high accuracy and high resolution neutron cross-sections. Thanks to the features of the neutron beam, a rich experimental program relevant to nuclear technology has been carried out so far. The program will be further expanded in the near future, thanks in particular to a new high-flux experimental area, now under construction.
High precision measurement of the radiative capture cross section of 238U at the n_TOF CERN facility
(2017)
The importance of improving the accuracy on the capture cross-section of 238U has been addressed by the Nuclear Energy Agency, since its uncertainty significantly affects the uncertainties of key design parameters for both fast and thermal nuclear reactors. Within the 7th framework programme ANDES of the European Commission three different measurements have been carried out with the aim of providing the 238U(n,γ) cross-section with an accuracy which varies from 1 to 5%, depending on the energy range. Hereby the final results of the measurement performed at the n_TOF CERN facility in a wide energy range from 1 eV to 700 keV will be presented.
Neutron-induced fission cross sections of 238U and 235U are used as standards in the fast neutron region up to 200 MeV. A high accuracy of the standards is relevant to experimentally determine other neutron reaction cross sections. Therefore, the detection effciency should be corrected by using the angular distribution of the fission fragments (FFAD), which are barely known above 20 MeV. In addition, the angular distribution of the fragments produced in the fission of highly excited and deformed nuclei is an important observable to investigate the nuclear fission process.
In order to measure the FFAD of neutron-induced reactions, a fission detection setup based on parallel-plate avalanche counters (PPACs) has been developed and successfully used at the CERN-n_TOF facility. In this work, we present the preliminary results on the analysis of new 235U(n,f) and 238U(n,f) data in the extended energy range up to 200 MeV compared to the existing experimental data.