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Livres sur le sujet « Hard magnetic materials »

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Auteur : Grafiati

Publié le 14 mars 2023

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1

Long, Gary J., et Fernande Grandjean, dir. Supermagnets, Hard Magnetic Materials. Dordrecht : Springer Netherlands, 1991. http://dx.doi.org/10.1007/978-94-011-3324-1.

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2

Long, Gary J. Supermagnets, Hard Magnetic Materials. Dordrecht : Springer Netherlands, 1991.

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3

1941-, Long Gary J., et Grandjean Fernande 1947-, dir. Supermagnets, hard magnetic materials. Dordrecht : Kluwer Academic Publishers, 1991.

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4

Betancourt, Israel. Magnetic materials : Current topics in amorphous wires, hard magnetic alloys, ceramics, characterization and modelling 2007. Trivandrum : Research Signpost, 2007.

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5

A, Salsgiver J., American Society for Metals. Transformer Steels Committee., American Society for Metals. Permanent Magnet Committee., Symposium on Soft and Hard Magnetic Materials with Applications (2nd : 1986 : Lake Buena Vista, Fla.) et ASM's Materials Week '86 (1986 : Lake Buena Vista, Fla.), dir. Soft and hard magnetic materials with applications : Proceedings of a symposium held in conjunction with ASM's Materials Week '86, Lake Buena Vista, Florida, 4-9 October 1986. [Metals Park, Ohio] : American Society for Metals, 1986.

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6

Men, Boris. Russian advances in atomic structure theory and applications : Solid solutions properties, hard alloys and magnetic materials. [Alexandria, Va.] : Global Consultants, 1992.

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7

National Register of Foreign Collaborations (India) et India. Dept. of Scientific & Industrial Research., dir. Technology in Indian hard ferrite industry : A status report prepared under the National Register of Foreign Collaborations. New Delhi : Govt. of India, Dept. of Scientific & Industrial Research, Ministry of Science and Technology, 1991.

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8

Coey, Michael, Laura H. Lewis, Bao-Min Ma, Thomas Schrefl et Ludwig Schultz. Advanced Hard and Soft Magnetic Materials : Volume 577. University of Cambridge ESOL Examinations, 2014.

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9

Solymar, L., D. Walsh et R. R. A. Syms. Magnetic materials. Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780198829942.003.0011.

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Macroscopic and microscopic theories of magnetic polarization are discussed. The origin of domains, domain walls, and of the hysteresis curve and the contrast between soft and hard magnetic materials are explained. The more important elements of the quantum theory of magnetism are discussed. The principles of the alignments in antiferromagnetic and ferromagnetic materials are explained. Magnetic resonance phenomena are discussed. Magnetoresistance and spintronics and their device prospects are also discussed at some length.

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10

(Editor), G. J. Long, et F. Grandjean (Editor), dir. Supermagnets, Hard Magnetic Materials (NATO Science Series C:). Springer, 2007.

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11

J. M. D. Coey (Editor), B.-M. Ma (Editor), T. Schrefl (Editor), L. Schultz (Editor), M. E. McHenry (Editor), V. G. Harris (Editor), J. Fidler (Editor), R. Hasegawa (Editor), A. Inoue (Editor) et Linda H. Lewis (Editor), dir. Advanced Hard and Soft Magnetic Materials : Symposium Held April 5-8, 1999, San Francisco, California, U.S.A (Materials Research Society Symposium Proceedings). Materials Research Society, 1999.

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12

Hard and soft magnetic materials with applications including superconductivity : Proceedings of a conference on hard and soft magnetic materials held in conjunction with ASM's Materials Week '87, Cincinnati, Ohio, 10-15 October 1987. [Metals Park, Ohio] : ASM International, 1987.

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13

Bouchez, Jean-Luc, et Adolphe Nicolas. Principles of Rock Deformation and Tectonics. Oxford University Press, 2021. http://dx.doi.org/10.1093/oso/9780192843876.001.0001.

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This book, based on laboratory, teaching and field experience, has a strong focus towards hard rocks and magmatic rocks, from both the continental crust worldwide, where quartz and granites are dominant, and the mantle dominated by olivine in peridotites. With more than 250 figures, most of them original, the book develops, in addition to classical structural geology objects, the fundamentals of brittle fracturing of materials, plastic deformation of ice, quartz and olivine, and fabric acquisition in rocks and magmas. Measurement and orientation of stress axes, bases of neotectonics and geophysics, and practical tools such as magnetic fabrics not commonly treated in geological books, are also provided. Emblematic tectonic and geodynamic sites are presented, both from the oceanic and continental crust, for instance the Oman ophiolites, and the India-Eurasia collision and its associated shear zones. Since the targeted readers are present-day young students, a few structural geology exercises are also included in order to improve their abilities.

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14

Horing, Norman J. Morgenstern. Quantum Statistical Field Theory. Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780198791942.001.0001.

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The methods of coupled quantum field theory, which had great initial success in relativistic elementary particle physics and have subsequently played a major role in the extensive development of non-relativistic quantum many-particle theory and condensed matter physics, are at the core of this book. As an introduction to the subject, this presentation is intended to facilitate delivery of the material in an easily digestible form to students at a relatively early stage of their scientific development, specifically advanced undergraduates (rather than second or third year graduate students), who are mathematically strong physics majors. The mechanism to accomplish this is the early introduction of variational calculus with particle sources and the Schwinger Action Principle, accompanied by Green’s functions, and, in addition, a brief derivation of quantum mechanical ensemble theory introducing statistical thermodynamics. Important achievements of the theory in condensed matter and quantum statistical physics are reviewed in detail to help develop research capability. These include the derivation of coupled field Green’s function equations of motion for a model electron-hole-phonon system, extensive discussions of retarded, thermodynamic and non-equilibrium Green’s functions, and their associated spectral representations and approximation procedures. Phenomenology emerging in these discussions includes quantum plasma dynamic, nonlocal screening, plasmons, polaritons, linear electromagnetic response, excitons, polarons, phonons, magnetic Landau quantization, van der Waals interactions, chemisorption, etc. Considerable attention is also given to low-dimensional and nanostructured systems, including quantum wells, wires, dots and superlattices, as well as materials having exceptional conduction properties such as superconductors, superfluids and graphene.

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15

Finlayson, James Gordon. Hegel and the Frankfurt School. Sous la direction de Dean Moyar. Oxford University Press, 2017. http://dx.doi.org/10.1093/oxfordhb/9780199355228.013.34.

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Hegel’s philosophy exerted a magnetic attraction on the various thinkers that comprise the Frankfurt school. This chapter aims to gauge and specify the relation that three members of the ‘inner circle’ of the Frankfurt school (Horkheimer, Adorno, and Marcuse) have to Hegel. It concludes that the young Horkheimer is a Hegelian-Marxist who endorses a qualified Hegelianism, while claiming that Hegel’s idealist metaphysics had become obsolete and superseded by a combination of sociology, psychology, and materialist historiography. Adorno remains a more committed Hegelian (and a Marxist-Hegelian) who sees his own dialectical approach to philosophy as emerging from and consistent with an immanent criticism of Hegel. Both, however, tend to reject Hegel’s philosophy of objective spirit as conservative apology for the Prussian state. Marcuse, by contrast, is a Hegelian-Marxist who has a more scholarly, nuanced, and charitable approach to Hegel, placing more emphasis on the critical moment in Hegel’s conception of reason.

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Glazov, M. M. Electron & ; Nuclear Spin Dynamics in Semiconductor Nanostructures. Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780198807308.001.0001.

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In recent years, the physics community has experienced a revival of interest in spin effects in solid state systems. On one hand, solid state systems, particularly semicon- ductors and semiconductor nanosystems, allow one to perform benchtop studies of quantum and relativistic phenomena. On the other hand, interest is supported by the prospects of realizing spin-based electronics where the electron or nuclear spins can play a role of quantum or classical information carriers. This book aims at rather detailed presentation of multifaceted physics of interacting electron and nuclear spins in semiconductors and, particularly, in semiconductor-based low-dimensional structures. The hyperfine interaction of the charge carrier and nuclear spins increases in nanosystems compared with bulk materials due to localization of electrons and holes and results in the spin exchange between these two systems. It gives rise to beautiful and complex physics occurring in the manybody and nonlinear system of electrons and nuclei in semiconductor nanosystems. As a result, an understanding of the intertwined spin systems of electrons and nuclei is crucial for in-depth studying and control of spin phenomena in semiconductors. The book addresses a number of the most prominent effects taking place in semiconductor nanosystems including hyperfine interaction, nuclear magnetic resonance, dynamical nuclear polarization, spin-Faraday and -Kerr effects, processes of electron spin decoherence and relaxation, effects of electron spin precession mode-locking and frequency focusing, as well as fluctuations of electron and nuclear spins.

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17

Bridges, John C. Evolution of the Martian Crust. Oxford University Press, 2017. http://dx.doi.org/10.1093/acrefore/9780190647926.013.18.

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This is an advance summary of a forthcoming article in the Oxford Encyclopedia of Planetary Science. Please check back later for the full article.Mars, which has a tenth of the mass of Earth, has cooled as a single lithospheric plate. Current topography gravity maps and magnetic maps do not show signs of the plate tectonics processes that have shaped the Earth’s surface. Instead, Mars has been shaped by the effects of meteorite bombardment, igneous activity, and sedimentary—including aqueous—processes. Mars also contains enormous igneous centers—Tharsis and Elysium, with other shield volcanoes in the ancient highlands. In fact, the planet has been volcanically active for nearly all of its 4.5 Gyr history, and crater counts in the Northern Lowlands suggest that may have extended to within the last tens of millions of years. Our knowledge of the composition of the igneous rocks on Mars is informed by over 100 Martian meteorites and the results from landers and orbiters. These show dominantly tholeiitic basaltic compositions derived by melting of a relatively K, Fe-rich mantle compared to that of the Earth. However, recent meteorite and lander results reveal considerable diversity, including more silica-rich and alkaline igneous activity. These show the importance of a range of processes including crystal fractionation, partial melting, and possibly mantle metasomatism and crustal contamination of magmas. The figures and plots of compositional data from meteorites and landers show the range of compositions with comparisons to other planetary basalts (Earth, Moon, Venus). A notable feature of Martian igneous rocks is the apparent absence of amphibole. This is one of the clues that the Martian mantle had a very low water content when compared to that of Earth.The Martian crust, however, has undergone hydrothermal alteration, with impact as an important heat source. This is shown by SNC analyses of secondary minerals and Near Infra-Red analyses from orbit. The associated water may be endogenous.Our view of the Martian crust has changed since Viking landers touched down on the planet in 1976: from one almost entirely dominated by basaltic flows to one where much of the ancient highlands, particularly in ancient craters, is covered by km deep sedimentary deposits that record changing environmental conditions from ancient to recent Mars. The composition of these sediments—including, notably, the MSL Curiosity Rover results—reveal an ancient Mars where physical weathering of basaltic and fractionated igneous source material has dominated over extensive chemical weathering.

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