000 | 03242nam a22004575i 4500 | ||
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001 | 978-3-642-27985-0 | ||
003 | DE-He213 | ||
005 | 20140220083310.0 | ||
007 | cr nn 008mamaa | ||
008 | 120507s2012 gw | s |||| 0|eng d | ||
020 |
_a9783642279850 _9978-3-642-27985-0 |
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024 | 7 |
_a10.1007/978-3-642-27985-0 _2doi |
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050 | 4 | _aQC19.2-20.85 | |
072 | 7 |
_aPHU _2bicssc |
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072 | 7 |
_aSCI040000 _2bisacsh |
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082 | 0 | 4 |
_a530.1 _223 |
100 | 1 |
_aScheck, Florian. _eauthor. |
|
245 | 1 | 0 |
_aClassical Field Theory _h[electronic resource] : _bOn Electrodynamics, Non-Abelian Gauge Theories and Gravitation / _cby Florian Scheck. |
264 | 1 |
_aBerlin, Heidelberg : _bSpringer Berlin Heidelberg : _bImprint: Springer, _c2012. |
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300 |
_aXII, 433p. 59 illus. _bonline resource. |
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336 |
_atext _btxt _2rdacontent |
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337 |
_acomputer _bc _2rdamedia |
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338 |
_aonline resource _bcr _2rdacarrier |
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347 |
_atext file _bPDF _2rda |
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490 | 1 |
_aGraduate Texts in Physics, _x1868-4513 |
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505 | 0 | _aMaxwell's Equations -- Symmetries and Covariance of Maxwell's Equations -- Maxwell Theory as a Classical Field Theory -- Some Applications of Maxwell Theory -- Local Gauge Theories -- Classical Field Theory of Gravitation. | |
520 | _aThe book describes Maxwell's equations first in their integral, directly testable form, then moves on to their local formulation. The first two chapters cover all essential properties of Maxwell's equations, including their symmetries and their covariance in a modern notation. Chapter 3 is devoted to Maxwell theory as a classical field theory and to solutions of the wave equation. Chapter 4 deals with important applications of Maxwell theory. It includes topical subjects such as metamaterials with negative refraction index and solutions of Helmholtz' equation in paraxial approximation relevant for the description of laser beams. Chapter 5 describes non-Abelian gauge theories from a classical, geometric point of view, in analogy to Maxwell theory as a prototype, and culminates in an application to the U(2) theory relevant for electroweak interactions. The last chapter 6 gives a concise summary of semi-Riemannian geometry as the framework for the classical field theory of gravitation. The chapter concludes with a discussion of the Schwarzschild solution of Einstein's equations and the classical tests of general relativity (perihelion precession of Mercury, and light deflection by the sun). ------ Textbook features: detailed figures, worked examples, problems and solutions, boxed inserts, highlighted special topics, highlighted important math etc., helpful summaries, appendix, index. | ||
650 | 0 | _aPhysics. | |
650 | 0 | _aMathematical physics. | |
650 | 1 | 4 | _aPhysics. |
650 | 2 | 4 | _aTheoretical, Mathematical and Computational Physics. |
650 | 2 | 4 | _aClassical and Quantum Gravitation, Relativity Theory. |
650 | 2 | 4 | _aMathematical Methods in Physics. |
710 | 2 | _aSpringerLink (Online service) | |
773 | 0 | _tSpringer eBooks | |
776 | 0 | 8 |
_iPrinted edition: _z9783642279843 |
830 | 0 |
_aGraduate Texts in Physics, _x1868-4513 |
|
856 | 4 | 0 | _uhttp://dx.doi.org/10.1007/978-3-642-27985-0 |
912 | _aZDB-2-PHA | ||
999 |
_c102696 _d102696 |