Preparation and Characterization of Silver and Gold Nanoparticles and Study Influence on Physical Properties of PVA/PVP nanocomposites

Gold nanoparticles (Au NPs) and Silver nanoparticles (Ag NPs) ware prepared by green synthesis extraction using the Chenopodium murale leaf extract, the obtained (Ag NPs and Au NPs) were investigated by UV/Vis. absorption spectroscopy, transmission electron microscopy, Zetasizer, XRD. The plant extraction leads to produce nanoparticles of spherical shape with size range from 4 to 22 nm. Polyvinyl alcohol (PVA) and polyvinyl Pyrolidone (PVP) blend with mixed silver and gold nanoparticles were prepared by casting method. Amorphous feather of doping polymers blend was characterized by X-ray diffraction. Significant changes within the polymer matrix were monitored from infrared spectroscopy which indicates the interaction between polymer blend and mixed nanoparticles. Both indirect and direct optical energy gaps are calculated and discussed

Genetic polymorphism of five genes associated with growth traits in goat

Genetic polymorphism studies in domestic animals aim at evaluating genetic variations within and across breeds mainly for conservation purposes. In this study, polymerase chain reaction-restriction fragment length polymorphism (PCR-RFLP) was used to detect polymorphisms of five candidate genes in four Egyptian and Saudi goat breeds (Barki, Zaribi, Ardi and Masri), to detect the genotype of GH, IGF1, POUIF1, MSTN and BMP15 genes in the goat breeds and their allele frequencies. Results of GH gene which encloses a Haelll endonuclease restriction site show four unique PCR-RFLP banding patterns (genotypes AA, AB, CC and CD). The frequencies of the A allele in the samples from the goat breeds varied from 0.410 to 0.620. While  IGF-1gene revealed three fragments after digestion with Haelll with genotype AA, AB and BB and the  frequencies of allele A varied from 0.432 to 0.731. Furthermore, PCR-RFLP of POUIF1 gene showed two  fragments after digestion by Pst1 endonuclease with genotype TT and CC and the frequencies of allele T varied from 0.250 to 0.840. The MSTN gene revealed three fragments after digestion with DraI with genotype AA, BB and AB and the frequencies of allele A varied from 0.240 to 0.630. Meanwhile, the BMP15 gene revealed one fragments of 112 bp for AA after digestion with Hinf1 enzyme.Key words: Goats, polymerase chain reaction-restriction fragment length polymorphism (PCR-RFLP), GH, IGF-1, POUIF1, MSTN, BMP-15

Biologically guided isolation and ADMET profile of new factor Xa inhibitors fromGlycyrrhiza glabraroots usingin vitroandin silicoapproaches

Selective factor Xa inhibitors effectively block coagulation cascade with a broader therapeutic window than multitargeted anticoagulants. They have evolved as a crucial part of prevention and treatment of thromboembolic diseases and in therapeutic protocols involved in many clinical trials in coronavirus disease 2019 (COVID-19) patients. Biologically-guided isolation of specific FXa inhibitors from licorice (Glycyrrhiza glabra) root extract furnished ten flavonoids. By detailed analysis of their1H,13C NMR and MS data, the structures of these flavonoids were established as 7,4′-dihydroxyflavone (1), formononetin (2), 3-R-glabridin (3), isoliquiritigenin (4), liquiritin (5), naringenin 5-O-glucoside (6), 3,3′,4,4′-tetrahydroxy-2-methoxychalcone (7), liquiritinapioside (8) and the two isomers isoliquiritigenin-4′-O-β-d-apiosylglucoside (9) and isoliquiritigenin-4-O-β-d-apiosylglucoside (10). All the isolated compounds were assessed for their FXa inhibitory activity usingin vitrochromogenic assay for the first time. Liquirtin (5) showed the most potent inhibitory effects with an IC50of 5.15 μM. The QikProp module was implemented to perform ADMET predictions for the screened compounds

LINEARNO PROGRAMIRANJE KAO ALAT ZA PROJEKTIRANJE SIROVINSKE SMJESE U TVORNICI CEMENTA

This study uses linear programming to develop a methodology for selecting the best raw material mix in an ASCOM cement plant in Egypt. In cement factories, this type adheres to Egyptian chemical composition criteria for raw feed (e.g. 82.5% calcium carbonate, 14.08% silica, 2.5% alumina and 0.92% iron oxide). Furthermore, the model is bound by industry-specific characteristics (e.g. lime saturation factor, silica modulus, alumina modulus and loss of ignition). The results reveal that the model is able to accurately reproduce the mixing of high-quality feed with varying constituent percentages. It is also capable of determining the combining limitations of each ingredient. Furthermore, it demonstrates optimality for additive sourcing short-term planning and capping limestone quality to meet changeable component combinations. Additionally, improving the raw mix reduces limestone feed quality from 51 to 50.6%, resulting in the inclusion of extra limestone reserves.Studija prikazuje metodu linearnoga programiranja uporabljenu sa svrhom odabira najbolje sirovinske smjese u tvornici cementa ASCOM (Egipat). Takva smjesa poštuje egipatske standarde kemijskoga sastava sirovine (npr. 82,5 % kalcijeva karbonata, 14,08 % silikata, 2,5 % aluminijeva oksida, 0,92 % željeznoga oksida). Također, model je uvjetovan industrijskim standardima (npr. faktorom zasićenja vapnom, silikatnim i aluminatnim modulom te gubitkom (oksida) žarenjem). Modelom se mogla točno izračunati visokokvalitetna mješavina različitih (postotnih) komponenti te je dokazan kao optimalan za brz izračun raznih aditiva i postizanje najveće kvalitete vapnenačke sirovine uz doziranje ostalih komponenti. Time je udjel vapnenca bilo moguće smanjiti na 50,6 – 51 %, što je otvorilo put eksploataciji dodatnih rezervi te sirovine

The effect of auditory stimulation on pain response of preterm infants

This study aimed to evaluate the effect of auditory stimulation on preterm infants' pain responses. A quasi-experimental design was utilized in this study. Thirty preterm infants were recruited for the study. They were one group used for three days as day one (routine care), day two (music intervention) and day three (recorded mother voice intervention) before, during and after blood sample procedure (heel prick) from Cairo University hospitals (El Monira and Kasar Aini). A tool containing two parts was used for data collection: 1) socio-demographic data for the preterm infants and the mothers, 2) Premature Infant Pain Profile (PIPP) tool for physiological responses (heart rate, oxygen saturation) behavioral state, brow bulge, eye squeeze, nasolabial furrow and respiratory rate was determined. Results of the study showed that during heel prick the majority of preterm infants (96.7%) who were exposed to recorded mother voice had highly statistical significant no or minimal pain followed by music groups (66.7%). On the other hand, nearly half of the cases (46.7%) had moderate pain and (30%) had severe pain among control group. There were significant differences between the three groups in the behavioral state, brow bulge, eye squeeze and nasolabial furrow (P≤0.001) and improved oxygen saturation (P≤0.05). After heel prick, the preterm infants (100%) who were exposed to recorded mother voice had highly statistically significant no or minimal pain in the items of behavioral state, eye squeeze and nasolabial furrow (P≤0.001), brow bulge was significantly lower (P≤0.05) when comparing by control or music group. In Conclusion, exposure to recorded mother voice during heel prick of preterm infants is better than exposure to music or no intervention and this was manifested by lower pain level, decrease heart rate, improved oxygen saturation and respiration. Key words: Auditory stimulation; recorded mother voice; music; pain response; physiological responses; behavioral stat

Ionospheric Response at Conjugate Locations During the 7–8 September 2017 Geomagnetic Storm Over the Europe-African Longitude Sector

This paper focuses on unique aspects of the ionospheric response at conjugate locations over Europe and South Africa during the 7–8 September 2017 geomagnetic storm including the role of the bottomside and topside ionosphere and plasmasphere in influencing electron density changes. Analysis of total electron content (TEC) on 7 September 2017 shows that for a pair of geomagnetically conjugate locations, positive storm effect was observed reaching about 65% when benchmarked on the monthly median TEC variability in the Northern Hemisphere, while the Southern Hemisphere remained within the quiet time variability threshold of ±40%. Over the investigated locations, the Southern Hemisphere midlatitudes showed positive TEC deviations that were in most cases twice the comparative response level in the Northern Hemisphere on the 8 September 2017. During the storm main phase on 8 September 2017, we have obtained an interesting result of ionosonde maximum electron density of the F2 layer and TEC derived from Global Navigation Satellite System (GNSS) observations showing different ionospheric responses over the same midlatitude location in the Northern Hemisphere. In situ electron density measurements from SWARM satellite aided by bottomside ionosonde-derived TEC up to the maximum height of the F2 layer (hmF2) revealed that the bottomside and topside ionosphere as well as plasmasphere electron content contributions to overall GNSS-derived TEC were different in both hemispheres especially for 8 September 2017 during the storm main phase. The differences in hemispheric response at conjugate locations and on a regional scale have been explained in terms of seasonal influence on the background electron density coupled with the presence of large-scale traveling ionospheric disturbances and low-latitude-associated processes. The major highlight of this study is the simultaneous confirmation of most of the previously observed features and their underlying physical mechanisms during geomagnetic storms through a multi–data set examination of hemispheric differences. © 2020. American Geophysical Union. All Rights Reserved

Solar Flares and Coronal Mass Ejections: A Statistically Determined Flare Flux-CME Mass Correlation

In an effort to examine the relationship between flare flux and corresponding CME mass, we temporally and spatially correlate all X-ray flares and CMEs in the LASCO and GOES archives from 1996 to 2006. We cross-reference 6,733 CMEs having well-measured masses against 12,050 X-ray flares having position information as determined from their optical counterparts. For a given flare, we search in time for CMEs which occur 10-80 minutes afterward, and we further require the flare and CME to occur within +/-45 degrees in position angle on the solar disk. There are 826 CME/flare pairs which fit these criteria. Comparing the flare fluxes with CME masses of these paired events, we find CME mass increases with flare flux, following an approximately log-linear, broken relationship: in the limit of lower flare fluxes, log(CME mass)~0.68*log(flare flux), and in the limit of higher flare fluxes, log(CME mass)~0.33*log(flare flux). We show that this broken power-law, and in particular the flatter slope at higher flare fluxes, may be due to an observational bias against CMEs associated with the most energetic flares: halo CMEs. Correcting for this bias yields a single power-law relationship of the form log(CME mass)~0.70*log(flare flux). This function describes the relationship between CME mass and flare flux over at least 3 dex in flare flux, from ~10^-7 to 10^-4 W m^-2.Comment: 28 pages, 16 figures, accepted to Solar Physic