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Field Theory Handbook

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Abstract

Let us first state exactly what this book is and what it is not. It is a compendium of equations for the physicist and the engineer working with electrostatics, magne­ tostatics, electric currents, electromagnetic fields, heat flow, gravitation, diffusion, optics, or acoustics. It tabulates the properties of 40 coordinate systems, states the Laplace and Helmholtz equations in each coordinate system, and gives the separation equations and their solutions. But it is not a textbook and it does not cover relativistic and quantum phenomena. The history of classical physics may be regarded as an interplay between two ideas, the concept of action-at-a-distance and the concept of a field. Newton's equation of universal gravitation, for instance, implies action-at-a-distance. The same form of equation was employed by COULOMB to express the force between charged particles. AMPERE and GAUSS extended this idea to the phenomenological action between currents. In 1867, LUDVIG LORENZ formulated electrodynamics as retarded action-at-a-distance. At almost the same time, MAXWELL presented the alternative formulation in terms of fields. In most cases, the field approach has shown itself to be the more powerful.

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... In the case where h = ε, from Eq. (14) we see that the 2 × 2 block at the upper left corner of the matrix (a j i ) represents an ordinary rotation about the origin on the plane R 3 = 0, hence, under these transformations (R 1 ) 2 + (R 2 ) 2 is invariant and one finds that ...
... and l, m are separation constants. This equation appears in the solution by separation of variables of the Laplace equation in the three-dimensional Euclidean space in prolate spheroidal equations (with l being an integer) (see, e.g., Ref. [13], Eq. (8.6.7) or Ref. [14], Table 1.06) and in toroidal coordinates (where l is a half-integer) (see, e.g, Ref. [13], Eq. (8.10.11) or Ref. [14], Sec. IV). ...
... and l, m are separation constants. This equation appears in the solution by separation of variables of the Laplace equation in the three-dimensional Euclidean space in prolate spheroidal equations (with l being an integer) (see, e.g., Ref. [13], Eq. (8.6.7) or Ref. [14], Table 1.06) and in toroidal coordinates (where l is a half-integer) (see, e.g, Ref. [13], Eq. (8.10.11) or Ref. [14], Sec. IV). ...
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... Substituting (46) and (47) into (8) and (9) (taking into account the azimuthal independence), while attaching (21) and (22) Thus, the initial conditions (7) or equivalently (20), by virtue of (48) and (49) , they also depend upon the physical and geometrical characteristics of the system under consideration. ...
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... Toroidal coordinates (η, θ, ϕ) for a point x = (x 0 , x 1 , x 2 ) in three-dimensional Euclidean space are defined [17,30] by the relations x 0 = sin θ cosh η − cos θ , x 1 = sinh η cos ϕ cosh η − cos θ , x 2 = sinh η sin ϕ cosh η − cos θ (1) in the range η ∈ (0, ∞), θ ∈ [−π, π], ϕ ∈ (−π, π]. For any fixed η 0 > 0, these coordinates define the interior domain η 0 = {x : η 0 < η ≤ ∞} ∪ S 1 where the limiting value η = ∞ corresponds respectively to the singular subset S 1 = {x ∈ R 3 : x 0 = 0, x 2 1 + x 2 2 = 1}. ...
... Proof Take a +,+ 0,0 = ( √ 2/π )q 0,0 , which gives f +,+ 0 = 1 identically. Then apply (30) to evaluate α(η 0 ) ...
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The Fourier method approach to the Neumann problem for the Laplacian operator in the case of a solid torus contrasts in many respects with the much more straight forward situation of a ball in 3-space. Although the Dirichlet-to-Neumann map can be readily expressed in terms of series expansions with toroidal harmonics, we show that the resulting equations contain undetermined parameters which cannot be calculated algebraically. A method for rapidly computing numerical solutions of the Neumann problem is presented with numerical illustrations. The results for interior and exterior domains combine to provide a solution for the Neumann problem for the case of a shell between two tori.
... Finally, by virtue of the representation theory, it is obvious that spherical geometry approximates sufficiently well most basic problems in linear isotropic elasticity. Nevertheless, the extension to spheroidal, ellipsoidal or even more complicated geometries [21,41] provides a challenging area for future investigation. ...
... comprise a complete set of eigenfunctions for harmonic functions and belong to the kernel space of the Laplace's operator from (10), i.e.  and mn  , while they are obtained once the classical method of separation of variables[21,22] is applied.Adopting the above mathematical analysis, the harmonic function A in differential representation (3) admits series expansion in terms of functions (13), i.e. ...
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... The spherical coordinate system is a way of representing a vector position that lies in a 3-dimensional space with three values, see Fig. 2a, one for the radius r of a sphere centered at the origin, one for the polar angle φ and the other for the azimuthal angle θ, in order to determine a position on such sphere's surface [15]. This coordinate system is used for representing vectors in problems that mainly deal with rotation operations, and therefore is appropriate for representing the W vectors in a version space bounded by a unit radius hypersphere, see Fig. 2b. ...
... Equation (17) is related to the property of complementary slackness and is satisfied because multiplying Eq. (18) by W T we obtain 2 · λ · ||W || 2 ≈ m , which implies that ||W || 2 = 1 because λ > 0. Consequently, Eqs. (15) and (16) are fulfilled. Therefore, considering λ = m/2, the KKT conditions can be simplified to the vector equation: ...
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... When ε dd = 0.3, the trajectory of the vortex is almost perfectly circular and is characterised by only a small ellipticity with a semi-major axis alongŷ. A larger degree of ellipticity is seen for ε dd = 0.6, though, and for ε dd = 0.9 the vortex trajectories are clearly no longer elliptical but are instead reminiscent of Cassini ovals [65]. ...
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... The types of potential problems defined by (19) to (21) have been discussed in connection with problems in electrostatic potential theory, fluid mechanics and elasticity and authoritative treatises covering these areas are given by [48][49][50][51][52][53][54][55][56] and others. It can be shown that the harmonic function that satisfies the boundary condition (20) and the regularity condition (21) takes the form ...
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... Let n = (γ 2 , −γ 1 ) be the unit exterior normal to Ω and κ = det γ , γ : T L → R be the signed curvature. We define the open tubular neighborhood, see Moon & Spencer (1988), by ...
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Chapter
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Chapter
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