Relevant bibliographies by topics / AlMn Binary Alloy

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  1. Journal articles
  2. Dissertations / Theses
  3. Book chapters

Academic literature on the topic 'AlMn Binary Alloy'

Author: Grafiati
Published: 6 September 2023

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Journal articles on the topic "AlMn Binary Alloy"

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Snitovsky, Yuri P. "Changes in the physical and mechanical properties of aluminum depending on the composition of the alloying elements." Yugra State University Bulletin 18, no. 4 (2023): 68–76. http://dx.doi.org/10.18822/byusu20220468-76.

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Subject of research: the influence of the concentration and composition of alloying elements Mn, Ti, Cr, Y, Mo, W, V on the change in the aluminum recrystallization temperature.
 Purpose of research: to find the optimal concentration of alloying additives, at which the recrystallization temperature reaches its maximum value.
 Methods and objects of research: using the methods of thermodynamic analysis of binary state diagrams of aluminum with alloying additives, it has been established that the nature of the change in the recrystallization temperature depends on what type of eutectic
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Mollaamin, Fatemeh. "Increasing corrosion resistance of binary Al-Alloy through implanting with some transition elements and heteroatom organic compounds." Acta Chimica Asiana 6, no. 2 (2023): 328–42. http://dx.doi.org/10.29303/aca.v6i2.166.

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Decorating of Transition metals (TMs) on the "AlMg" nanoalloy has been studied on the basis of Langmuir adsorption applying "ONIOM" model with three levels of «high, medium and low» by using "LANL2DZ /6-31+G(d,p)/EPR-III", "semi-empirical" and "MM2" functions. The fluctuation of "NQR" has estimated the inhibiting role of pyridine and alkylpyridines containing 2-picoline (2Pic), 3-picoline (3Pic) ,4-picoline (4Pic), and 2,4-lutidine (24Lut) for (Sc, Ti, Cr, Ni, Cu, Zn)-doped AlMg alloy nanosheet due to "N" atom in the benzene cycle of heterocyclic carbenes being near the monolayer surface of te
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Kowalski, W., B. Grushko, Włodzimierz Bogdanowicz, and M. Surowiec. "Complex Intermetallics in the Al-Rich Part of Al-Pd-Cr System." Solid State Phenomena 163 (June 2010): 272–77. http://dx.doi.org/10.4028/www.scientific.net/ssp.163.272.

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The Al-Pd-Cr alloy system was investigated at 680 to 990°C in the compositional range above 60 at.% Al. The binary Al-Cr , μ and phases dissolves up to 1 at.% of Al, the η-phase extends up to 2 at.% of Pd and the 2-phase extends up to 3 at.% of Pd, respectively. The binary Al-Pd -phases dissolves up to 3 at.% of Cr and -phase up to 4 at.% Cr. Close to the high-Pd limit of the -range a ternary phase is formed between about Al78Pd4Cr18, Al77Pd10Cr13 and Al74Pd7Cr19. Its structure is orthorhombic with lattice parameters: a = 1.47, b = 1.24 and c = 1.25 nm, resembling the lattice parameters
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Wang, Tian, Dmytro Kevorkov, Ahmad Mostafa, and Mamoun Medraj. "Experimental Investigation of the Phase Equilibria in the Al-Mn-Zn System at 400°C." Journal of Materials 2014 (July 17, 2014): 1–13. http://dx.doi.org/10.1155/2014/451587.

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Al-Mn-Zn ternary system is experimentally investigated at 400°C using diffusion couples and key alloys. Phase relationships and homogeneity ranges are determined for binary and ternary compounds using EPMA, SEM/EDS, and XRD. Reported ternary compound T3 (Al11Mn3Zn2) is confirmed in this study and is denoted as τ2 in this paper. Two new ternary compounds (τ1 and τ3) are observed in this system at 400°C. τ1 is determined as a stoichiometric compound with the composition of Al31Mn8Zn11. τ3 has been found to have homogeneity range of AlxMnyZnz (x=9–13 at%; y=11–15 at%; z=75–77 at%). The binary com
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Gallardo Cava, Iván, Valentín Bujarrabal, Javier Alcolea, et al. "Rotating and Expanding Gas in Binary Post-AGB Stars." Astronomy 1, no. 2 (2022): 84–92. http://dx.doi.org/10.3390/astronomy1020008.

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There is a class of binary post-AGB stars (binary system including a post-AGB star) that are surrounded by Keplerian disks and outflows resulting from gas escaping from the disk. To date, there are seven sources that have been studied in detail through interferometric millimeter-wave maps of CO lines (ALMA/NOEMA). For the cases of the Red Rectangle, IW Carinae, IRAS 08544-4431, and AC Herculis, it is found that around ≥85% of the total nebular mass is located in the disk with Keplerian dynamics. The remainder of the nebular mass is located in an expanding component. This outflow is probably a
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Graver, Brit, Antonius van Helvoort, John Charles Walmsley, and Kemal Nisancioglu. "Surface Segregation of Indium by Heat Treatment of Aluminium." Materials Science Forum 519-521 (July 2006): 673–78. http://dx.doi.org/10.4028/www.scientific.net/msf.519-521.673.

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High temperature heat treatment of aluminium alloys causes surface enrichment of the trace elements in Group IIIA - VA, specifically the low melting point elements Pb, Bi, In and Sn. The phenomenon has practical significance in promoting certain types of localised corrosion, such as galvanic and filiform corrosion, while mitigating other types, such as pitting corrosion of the bare surface. The purpose of this paper is to investigate the surface enrichment and microstructure of indium relative to the available data for Pb. Model binary AlIn alloys, containing 20-1000 ppm of In, were used after
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Martinez–Brunner, Rafael, Simon Casassus, Sebastián Pérez, et al. "High-resolution ALMA observations of V4046 Sgr: a circumbinary disc with a thin ring." Monthly Notices of the Royal Astronomical Society 510, no. 1 (2021): 1248–57. http://dx.doi.org/10.1093/mnras/stab3440.

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ABSTRACT The nearby V4046 Sgr spectroscopic binary hosts a gas-rich disc known for its wide cavity and dusty ring. We present high resolution (∼20 mas or 1.4 au) ALMA observations of the 1.3 mm continuum of V4046 Sgr which, combined with SPHERE–IRDIS polarised images and a well-sampled spectral energy distribution (SED), allow us to propose a physical model using radiative transfer predictions. The ALMA data reveal a thin ring at a radius of 13.15 ± 0.42 au (Ring13), with a radial width of 2.46 ± 0.56 au. Ring13 is surrounded by a ∼10 au-wide gap, and it is flanked by a mm-bright outer ring (R
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Guélin, M., N. A. Patel, M. Bremer, et al. "IRC +10 216 in 3D: morphology of a TP-AGB star envelope." Astronomy & Astrophysics 610 (February 2018): A4. http://dx.doi.org/10.1051/0004-6361/201731619.

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During their late pulsating phase, AGB stars expel most of their mass in the form of massive dusty envelopes, an event that largely controls the composition of interstellar matter. The envelopes, however, are distant and opaque to visible and NIR radiation: their structure remains poorly known and the mass-loss process poorly understood. Millimeter-wave interferometry, which combines the advantages of longer wavelength, high angular resolution and very high spectral resolution is the optimal investigative tool for this purpose. Mm waves pass through dust with almost no attenuation. Their spect
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Gu, Z., J. H. Edgar, E. A. Payzant, et al. "Sublimation Growth of Aluminum Nitride-Silicon Carbide Alloy Crystals on SiC (0001) Substrates." MRS Proceedings 831 (2004). http://dx.doi.org/10.1557/proc-831-e3.1.

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ABSTRACTThick (up to 1 mm) AlN-SiC alloy crystals were grown on off-axis Si-face 6H-SiC (0001) substrates by the sublimation-recondensation method from a mixture of AlN and SiC powders at 1860–1990 °C in a N2 atmosphere. The color of the crystals changed from clear to dark green with increasing growth temperature. Raman spectroscopy and x-ray diffraction (XRD) confirmed an AlN-SiC alloy was formed with the wurtzite structure and good homogeneity. Three broad peaks were detected in the Raman spectra, with one of those related to an AlN-like and another one to a SiC-like mode, both shifted relat
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Wood, C. M., J. C. A. Miller-Jones, A. Bahramian, et al. "Time-dependent visibility modelling of a relativistic jet in the X-ray binary MAXI J1803−298." Monthly Notices of the Royal Astronomical Society, March 30, 2023. http://dx.doi.org/10.1093/mnras/stad939.

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Abstract Tracking the motions of transient jets launched by low-mass X-ray binaries (LMXBs) is critical for determining the moment of jet ejection, and identifying any corresponding signatures in the accretion flow. However, these jets are often highly variable and can travel across the resolution element of an image within a single observation, violating a fundamental assumption of aperture synthesis. We present a novel approach in which we directly fit a single time-dependent model to the full set of interferometer visibilities, where we explicitly parameterise the motion and flux density va
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Dissertations / Theses on the topic "AlMn Binary Alloy"

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Meddour, Athmane. "Structure electronique d'alliages metalliques amorphes et quasicristallins : systemes binaires pdy et almn." Paris 6, 1988. http://www.theses.fr/1988PA066696.

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Etude realisee par spectroscopie optique et photoelectronique. Les echantillons sont prepares par pulverisation cathodique sous forme de couches minces. On obtient des echantillons amorphes et quasicristallins par melange ionique a partir de couches multiples. Discussion de l'evolution des spectres optiques des alliages al-mn lorsqu'on passe d'un etat cristallin ordonne a un etat quasi ordonne et enfin a un etat totalement desordonne
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Book chapters on the topic "AlMn Binary Alloy"

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Igor, Vurgaftman. "Binary Compound Semiconductors." In Bands and Photons in III-V Semiconductor Quantum Structures. Oxford University Press, 2020. http://dx.doi.org/10.1093/oso/9780198767275.003.0006.

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To apply the band structure models discussed in Part I (extended to structures with quantum confinement in Part III and applied to photonic devices in Part IV), a reliable set of input parameters is necessary. The chapter overviews the literature related to these parameters that has appeared since our published reviews. It also recommends specific values for all of them, including the dependence on temperature and alloy composition. If reliable experimental reports are available, they are used preferentially in the recommendations. Otherwise, it falls back to extrapolations from the existing data and theoretical estimates to fill in the gaps. It starts by reviewing and tabulating band parameters for the III–V compound semiconductors GaAs, AlAs, InAs, GaSb, AlSb, InSb, GaP, AlP, InP, GaN, AlN, and InN. The parameters include energy gaps, electron and hole mass parameters, deformation potentials, elastic constants, band offsets, and their temperature dependences.
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