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  • 1
    In: Journal of Nanomaterials, Hindawi Limited, Vol. 2023 ( 2023-4-29), p. 1-10
    Abstract: Our work was devoted to studying the effect of different concentrations of Mentha spicata aqueous extract on the green synthesis of silver nanoparticles (AgNPs) in order to obtain the most effective of these concentrations for bacteria inhibitory activity. Different concentrations of the aqueous M. spicata extract (0.25, 0.50, 0.75, and 1.00 mM) were used as biological solvent to synthesize AgNPs by means of the reduction method. The crystal structure and morphology of the NPs were characterized UV–vis spectra, X-ray diffraction (XRD), and scanning electron microscopy (SEM). The inhibition effect of AgNPs on Escherichia coli was studied to determine the minimum inhibitory concentration (MIC). The dark yellow color of the M. spicata extract aqueous solution indicates the successful synthesis of the AgNPs. UV spectra of the NPs show a gradual increase in absorption with increasing concentration of aqueous M. spicata extract solution from 0.25 to 1.00 mM, accompanied by a shift in the wavelength from 455 to 479 nm along with a change in the nanoparticle size from 31 to 9 nm. The tests also showed a high activity of the particles against bacteria (E. coli) ranging between 15.6 and 62.5 µg/ml. From the AgNPs, it was confirmed that aqueous M. spicata extract is an effective biosolvent for the synthesis of different sizes of AgNPs according to the solvent concentration. The AgNPs also proved effectual for the killing of bacteria.
    Type of Medium: Online Resource
    ISSN: 1687-4129 , 1687-4110
    Language: English
    Publisher: Hindawi Limited
    Publication Date: 2023
    detail.hit.zdb_id: 2229480-6
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  • 2
    Online Resource
    Online Resource
    IOP Publishing ; 2022
    In:  Research in Astronomy and Astrophysics Vol. 22, No. 8 ( 2022-08-01), p. 085013-
    In: Research in Astronomy and Astrophysics, IOP Publishing, Vol. 22, No. 8 ( 2022-08-01), p. 085013-
    Abstract: The present work aims to build a new statistical distance scale for planetary nebulae (PNe) based on a rigorous calibration sample. The distances of the calibration sample are derived from the trigonometric parallax method using the recent measurements of Gaia Early Data Release 3 (Gaia EDR3). The new distance scale is created by applying the well-known linear relationship between the radio surface brightness temperature and the nebular radius. The calibration sample is made up of 96 PNe of accurately computed distances with uncertainties less than 20%. Earlier ground- and space-based trigonometric parallaxes of PNe display inconsistency with those of Gaia, particularly the Hipparcos results. In addition, these measurements have appreciably lower precision than those of Gaia. When compared to the trigonometric technique, the expansion and kinematic methods exhibited more consistency than the spectroscopic, extinction, gravity, and photoionization methods. Furthermore, contrary to earlier results in the literature, the extinction and gravity methods, on average, underestimate and slightly overestimate the PN distances respectively. As a byproduct of extracting the Gaia parallaxes, we detect the radial velocity and variability for 14 and 3 PN central stars (CSs), respectively. To our knowledge, the variability of Hen 2-447 CS has been determined for the first time.
    Type of Medium: Online Resource
    ISSN: 1674-4527
    Language: Unknown
    Publisher: IOP Publishing
    Publication Date: 2022
    detail.hit.zdb_id: 2511247-8
    SSG: 6,25
    SSG: 16,12
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  • 3
    In: Scientific Reports, Springer Science and Business Media LLC, Vol. 13, No. 1 ( 2023-04-11)
    Abstract: This study examined the effect of varying concentrations of Ocimum basilicum aqueous extract, which was done via the green synthesis of Silver nanoparticles (AgNPs), on the identification of the most effective concentration for bacteria inhibitory activity. Different concentrations of the aqueous Ocimum basilicum extract (0.25, 0.50, 0.75 and 1.00 mM) were used as reducing and stabilizing agent to synthesize AgNPs by means of the reduction method. The crystal structure and morphology of the NPs were characterized UV–Vis spectra, X-ray diffraction (XRD) and scanning electron microscopy (SEM). The antibacterial efficacy of AgNPs was studied against E. coli ATCC 35218 using well diffusion, MIC, MBC, and time-kill curve. The dark yellow color of the Ocimum basilicum aqueous solution indicates the successful synthesis process of the AgNPs. UV-spectra of the AgNPs display a gradual increase of absorption in sequence with concentration increase of aqueous Ocimum basilicum extract solution from 0.25 to 1.00 mM. This, in turn, led to a shift in the wavelength from 488 to 497 nm, along with a change in the nanoparticle size from 52 to 8 nm. The tests also showed a high activity of the particles against bacteria ( E. coli ), ranging between 15.6 and 62.5 µg/ml. Based on AgNPs, it was confirmed that an aqueous Ocimum basilicum extract can be used as an effective, reducing and stabilizing agent for the synthesis of different sizes of AgNPs based on the solvent concentration. The AgNPs also proved to be effective in inhibiting and killing bacteria.
    Type of Medium: Online Resource
    ISSN: 2045-2322
    Language: English
    Publisher: Springer Science and Business Media LLC
    Publication Date: 2023
    detail.hit.zdb_id: 2615211-3
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  • 4
    In: Physica Scripta, IOP Publishing, Vol. 98, No. 9 ( 2023-09-01), p. 095914-
    Abstract: Due to their unique structure, the metal sulfides are mechanically stable, have higher conductivities, and are frequently used in energy storage devices. Here, binder-free electrodes were designed by depositing the nickel zinc sulfide (NiZnS) incorporated with carbon nanotubes (CNTs) on the nickel foam (NF). X-ray diffraction (XRD) was used to describe the crystallinity of produced CNTs-NiZnS nanostructures, and morphological investigations were performed using field emission scanning electron microscopy (FESEM). According to the electrochemical measurements, the heating of electrolyte at 80 °C resulted in considerably enhanced specific capacitance of 1475 Cg −1 (50.85 F m −2 ) and 666 Cg −1 (13.77 F m −2 ) at 1 and 2 Ag −1 current density, correspondingly. Thus demonstrating a good capacity retention of 47% at 2 Ag −1 . The supercapattery (CNTs-NiZnS//AC) was designed with CNTs-NiZnS and AC, providing a specific charge capacity of 212 Cg −1 (at 2.0 Ag −1 ) along with energy density of 51 Wh-kg −1 at 820 W kg −1 power density. The stability of CNTs-NiZnS//AC was tested by subjecting it to 5000 successive cycles.
    Type of Medium: Online Resource
    ISSN: 0031-8949 , 1402-4896
    Language: Unknown
    Publisher: IOP Publishing
    Publication Date: 2023
    detail.hit.zdb_id: 1477351-X
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  • 5
    Online Resource
    Online Resource
    Virtual Company of Physics ; 2023
    In:  Journal of Ovonic Research Vol. 19, No. 1 ( 2023-01), p. 1-14
    In: Journal of Ovonic Research, Virtual Company of Physics, Vol. 19, No. 1 ( 2023-01), p. 1-14
    Abstract: This research presents a simulation study to achieve an optimized homojunction GaAs solar cell using SILVACO TCAD. A solar cell with configuration of p+ -AlGaAs as window, p-GaAs as emitter, n-GaAs as base and n+ -AlGaInP as BSF layer is proposed. The AlGaInP is selected as BSF layer due to high bandgap as compared to AlGaAs that is usually used in literature. Large scale of variation for doping concentration and thickness for all layers of cell have been simulated. The results show an improvement for solar cell parameters for the optimized cell as compared with the proposed one, where Jsc increases from 40.03 mA/cm2 to 52.58 mA/cm2 , Voc slightly increases from 0.94 V to 1 V, Pmax increases from 30.8 mW/cm2 to 46.86 mW/cm2 , FF increases from 82.19% to 88.54% and η increases from 22.29% to 33.94%. Which confirms the effectiveness of the doping concentration and thickness on solar cell performance.
    Type of Medium: Online Resource
    ISSN: 1584-9953
    URL: Issue
    Language: Unknown
    Publisher: Virtual Company of Physics
    Publication Date: 2023
    detail.hit.zdb_id: 2563541-4
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  • 6
    Online Resource
    Online Resource
    Springer Science and Business Media LLC ; 2022
    In:  Astrophysics and Space Science Vol. 367, No. 6 ( 2022-06)
    In: Astrophysics and Space Science, Springer Science and Business Media LLC, Vol. 367, No. 6 ( 2022-06)
    Type of Medium: Online Resource
    ISSN: 0004-640X , 1572-946X
    Language: English
    Publisher: Springer Science and Business Media LLC
    Publication Date: 2022
    detail.hit.zdb_id: 1472548-4
    detail.hit.zdb_id: 2207653-0
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  • 7
    In: Journal of Nanomaterials, Hindawi Limited, Vol. 2023 ( 2023-4-26), p. 1-11
    Abstract: Despite several attempts to enhance the electrical and charge carrier transport characteristics of porous silicon (PSi), the requisite conditions for optimally synthesizing n-PSi with appealing optoelectronic properties are yet to be achieved. Therefore, this research explores the effect of the chemical ratio of precursor materials (HF:C2H6O:H2O2) on the surface morphology, crystalline structure, and optical and electric properties of PSi. The PSi was produced by photoelectrochemical etching followed by anodization of the n-type Si under light illumination. The properties of the as-prepared PSi were studied by means of microscopic and spectroscopic techniques. The HF:C2H6O:H2O2 chemical ratio was optimized at 2 : 1 : 1. A metal–semiconductor–metal (MSM) ultraviolet photodetector (Pt/n-PSi/Pt) was fabricated, which exhibited high performances under UV light (365 nm) illumination. The photodetector was shown to be highly stable and reliable with a rapid rise time of 0.56 s at a bias voltage of +5 V. The MSM photodetector displayed responsivity (Rp) of 9.17 A/m at 365 nm, which significantly exceeds the values reported for TiC/porous Si/Si in some contemporary research. The photodetector fabricated from n-PSi, synthesized at an optimum chemical ratio (2 : 1 : 1) exhibited the best photodetection performance, possibly due to the high porosity and defect-free state of the n-PSi thin films.
    Type of Medium: Online Resource
    ISSN: 1687-4129 , 1687-4110
    Language: English
    Publisher: Hindawi Limited
    Publication Date: 2023
    detail.hit.zdb_id: 2229480-6
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  • 8
    Online Resource
    Online Resource
    World Scientific Pub Co Pte Ltd ; 2022
    In:  International Journal of Modern Physics E Vol. 31, No. 03 ( 2022-03)
    In: International Journal of Modern Physics E, World Scientific Pub Co Pte Ltd, Vol. 31, No. 03 ( 2022-03)
    Abstract: Spin correlation coefficients in elastic scattering of leptons on the deuteron are studied in the one-photon-exchange Born approximation within the limit of zero lepton mass. Numerical estimations for the spin correlation coefficients caused by a polarized beam and a vector polarized target are presented and analyzed at various beam energies and scattering angles in two coordinate systems which are relevant for experiment. The influence of the obtained results on the nucleon structure is investigated, and a considerable dependence at incident beam energies greater than 1[Formula: see text]fm[Formula: see text] and backward scattering angles is found. The estimated results are of particular interest for encouragement of experimental measurements of lepton-deuteron scattering which aim for accurate calculation of the charge radius of the proton to a high degree of precision. These results may also stimulate new generation of measurements of different physical observables very sensitive to the spin structure of the nucleon and light nuclei.
    Type of Medium: Online Resource
    ISSN: 0218-3013 , 1793-6608
    Language: English
    Publisher: World Scientific Pub Co Pte Ltd
    Publication Date: 2022
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  • 9
    Online Resource
    Online Resource
    Institute of Electrical and Electronics Engineers (IEEE) ; 2020
    In:  IEEE Transactions on Electron Devices Vol. 67, No. 1 ( 2020-1), p. 53-56
    In: IEEE Transactions on Electron Devices, Institute of Electrical and Electronics Engineers (IEEE), Vol. 67, No. 1 ( 2020-1), p. 53-56
    Type of Medium: Online Resource
    ISSN: 0018-9383 , 1557-9646
    Language: Unknown
    Publisher: Institute of Electrical and Electronics Engineers (IEEE)
    Publication Date: 2020
    detail.hit.zdb_id: 2028088-9
    detail.hit.zdb_id: 241634-7
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  • 10
    Online Resource
    Online Resource
    IOP Publishing ; 2023
    In:  Research in Astronomy and Astrophysics Vol. 23, No. 4 ( 2023-04-01), p. 045006-
    In: Research in Astronomy and Astrophysics, IOP Publishing, Vol. 23, No. 4 ( 2023-04-01), p. 045006-
    Abstract: The extremely accurate estimates of stellar variability and radial velocity in the Gaia Data Release 3 (Gaia DR3) have enabled us to examine the close binarity and radial velocity (RV) of central stars (CSs) of planetary nebulae (PNe). This study is twofold: (1) searching for new close binary CS candidates to better understand how binarity affects the formation and evolution of PNe; and (2) extending the sample size of known RVs of PNe in order to understand their kinematics and the dynamics of the Milky Way. As a target sample, we used all true, possible, and likely PNe available in the literature. Then, we looked for their matched Gaia DR3 sources that provide measurements of variability and RV. As a result, we detected the first large collection of trustworthy photometric variability of 26 symbiotic stars and 82 CSs. In this CS group, there are 24 sources already classified as true close binary CSs in the literature. Hence, we discovered 58 new close binary CS candidates. This close binary (CB) sample represents more than half of what is currently available in the literature. In addition, we identified the radial velocities for 51 PNe. To our knowledge, 24 of these were measured for the first time. The RV measurements predicted by Gaia, based on the Doppler shift of the CS absorption lines, and those derived from nebular emission lines, show satisfactory agreement except for a few extremely high-velocity PNe.
    Type of Medium: Online Resource
    ISSN: 1674-4527
    Language: Unknown
    Publisher: IOP Publishing
    Publication Date: 2023
    detail.hit.zdb_id: 2511247-8
    SSG: 6,25
    SSG: 16,12
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