357 research outputs found
Praesphaerammina, a new genus of Cenozoic deep-water agglutinated foraminifera from the Carpathian flysch deposits
The genus Praesphaerammina Kaminski and Filipcscu is newly described based on a revision of the type species Cystammina subgaleata Vasicek 1947. The genus differs from the Holocene genus Sphaerammina Cushman 1910 emend. Loeblich and Tappan 1964, in possessing a less embracing final chamber and in its interio-areal to areal aperture that lacks any tooth. The definition of the subfamily Sphaeramminae is accordingly emended as well. The genus is common in the Eocene of the Carpathian flysch deposits, but the type species Praesphaerammina subgaleata (Vasicek 1947) is also observed in the Caribbean region and West Africa, where it ranges into the Miocene
The response of modern benthic foraminiferal assemblages to water mass properties along the southern shelf of the Marmara Sea.
Dietary supplementation of Yerba Mate (Ilex paraguariensis) during the dry period improves redox balance in lactating dairy cows
Thirty-six pregnant Holstein–Friesian cows were used to study the effect of Yerba Mate (YM) supplementation during the dry period on redox balance. The treatments groups were Control (no YM), YM 250 (250 g/cow/day), and YM 500 (500 g/cow/day). Blood samples were obtained 30 days prepartum, at calving, and monthly postpartum until four months post calving. Liveweight (LW) and body condition score (BCS) were assessed prepartum, at calving, and then postpartum monthly until the end of the trial. Plasma was analyzed for hydroperoxides (d-ROMs), advanced oxidation protein products (AOPP), and biological antioxidant potential (BAP). The oxidative stress index (OSI) was calculated as OSI = ROMs/BAP 100. Cows were milked twice daily, and milk yield data were recorded daily. Redox balance was improved by YM supplementation, as reflected in the lower OSI values observed in the YM groups. Yerba Mate supplementation significantly affected LW, but did not affect BCS. Milk yield averaged 28.1 0.40, 29.0 0.48, and 29.9 0.46 L/cow/day in the Control, YM 250, and YM 500 groups, respectively, but was not significant. Nutritional manipulation during the dry period with Yerba Mate has demonstrated the potential to improve redox balance and milk yiel
Growth and characterizations of nanostructured tungsten oxides
Tungsten oxide (WO3) as nanostructured thin film is an attractive compound to be used for sensors applications. We report on WO3 nanostructured thin films deposited by radio-frequency plasma assisted laser ablation technique. A tungsten oxide ceramic target was irradiated at 193 nm wavelength; the depositions have been carried out in a gas mixture of oxygen and argon on heated substrates (corning glass and silicon) up to 600°C. The gas pressure varied between 1 Pa and 10 Pa. The influence of the substrate temperature, gas pressure and RF power on properties of the obtained nanostructures was investigated by Atomic Force Microscopy, Raman spectroscopy, Secondary Ion Mass Spectrometry and spectro-ellipsometry
Aspects Regarding the Determination of the Law Applicable for Natural Persons
Determining the law applicable for natural persons has special importance in the private international law, considering the way in which this legal institution is regulated and influences other institutions of private international law, like: law embezzlement, renvoi, public order, legal document with a foreign element, civil offence, etc. National law systems include various regulations regarding the determination of the law applicable to natural persons, consequently the international private law had to find solutions for achieving a compatibility between these systems.natural person, citizenship, domicile, personal law, national law, capacity
Future prospects of nuclear reactions induced by gamma-ray beams at ELI-NP
The future prospects of photonuclear reactions studies at the new Extreme Light Infrastructure—Nuclear Physics (ELI-NP) facility are discussed in view of the pursuit of investigating the electromagnetic response of nuclei using γ-ray beams of unprecedented energy resolution and intensity characteristics. We present here the features of the γ-ray beam source, the emerging ELI-NP experimental program involving photonuclear reactions cross section measurements and spectroscopy and angular measurements of γ-rays and neutrons along with the detection arrays currently under implementation
E1 moments from a coherent set of measured photoneutron cross sections
info:eu-repo/semantics/publishe
Simulation of the ELIGANT-GN array performances at ELI-NP for gamma beam energies larger than neutron threshold
Performance of the ELIGANT-GN array being developed at ELI-NP was evaluated using dedicated GEANT4 simulation code. The array is designed to consist of 17 LaBr3:Ce and 17 CeBr3 detectors as well as 33 BC501A and 29 6Li-glass detectors. The energy and time responses of the detectors were studied giving information on gamma and neutron absolute detection efficiencies of the array. A planned day-one experiment regarding the gamma and neutron decay from GDR in 208Pb is discussed and, based on simulations, the data analysis procedure is proposed. The detection efficiencies as well as the count rates estimations are presented
Response function and linearity for high energy Î3-rays in large volume LaBr3:Ce detectors
The response function to high energy γ-rays of two large volume LaBr3:Ce crystals (3.5”x8”) and the linearity of the coupled PMT's were investigated at the NewSUBARU facility, where γ-rays in the energy range 6–38 MeV were produced and sent into the detectors. Monte Carlo simulations were performed to reproduce the experimental spectra. The photopeak and interaction efficiencies were also evaluated both in case of a collimated beam and an isotropic sourc
Response function and linearity for high energy γ-rays in large volume LaBr3:Ce detectors
The response function to high energy γ-rays of two large volume LaBr3:Ce crystals (3.5”x8”) and the linearity of the coupled PMT's were investigated at the NewSUBARU facility, where γ-rays in the energy range 6–38 MeV were produced and sent into the detectors. Monte Carlo simulations were performed to reproduce the experimental spectra. The photopeak and interaction efficiencies were also evaluated both in case of a collimated beam and an isotropic source
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