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5
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84951214551
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For a very readable account of the early studies of scattering of plane waves by spheres see
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(1965)
Proc. IEEE
, vol.63
, pp. 48
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-
Logan, N.A.1
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6
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33645771791
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See also, a note by the same author published
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(1962)
the J. Opt. Soc. Am.
, vol.52
, pp. 342
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-
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7
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84951214552
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For a detailed list of references to papers on multipole expansions up to 1953 see
-
(Wiley, New York)
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(1955)
Multipole Fields
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Rose, M.E.1
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21
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0040225149
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The relationship between homogeneous plane wave expansions and angular spectrum representations is discussed, for certain classes of scalar wave fields, in
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(1973)
SIAM Rev.
, vol.15
, pp. 765
-
-
Devaney, A.J.1
Sherman, G.C.2
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23
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84951214553
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The customary term “multipole field” for the field [formula omitted] defined by Eq. (2.4) is rather inappropriate since this field is everywhere well-behaved. This terminology is undoubtedly responsible for incorrect statements in the literature about the behavior of such a field at the origin. [See, for example, W. Heitler. The Quantum Theory of Radiation (Clarendon, Oxford, 1954), 3rd ed., statement following Eq. (9) on p. 402.]
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It is the scalar field [formula omitted] defined by Eq. (3.14), and the electromagnetic fields [formula omitted] [formula omitted] and [formula omitted] [formula omitted] defined by Eqs. (4.15), that behave as fields generated by a true multipole at the origin [formula omitted] and hence have an appropriate singularity at that point.
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-
-
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24
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84951258387
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We use the same definitions of the spherical harmonics and of the spherical Bessel and Hankel functions as those given in A. Messiah, Quantum Mechanics (North-Holland, Amsterdam, third printing 1965), Vol. I, App. BII and BIV.
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-
-
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25
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0001554253
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(Paris); Because the integrand of (3.4) is an entire analytic function of a, the a integration contours [formula omitted] may be deformed in accordance with the rules of integration in the complex plane. When these contours are chosen as shown in Fig. 1, (3.4) corresponds to the following, frequently used, alternative form of the Weyl expansion: [formula omitted] Here, [formula omitted] if [formula omitted] The two forms of the Weyl expansion, and the transformations required to pass from one to the other, are discussed in A. Baños, Dipole Radiation in the Presence of a Conducting Half-Space (Pergamon, New York, 1966), sec. 2.13.
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(1919)
Ann. Phys.
, vol.60
, pp. 481
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Weyl, H.1
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26
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84951261821
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If the representation (3.4a), rather than (3.4), is employed one obtains, instead of (3.5), the following form of the angular spectrum representation, which is commonly employed in the literature: [formula omitted]where [formula omitted] is defined by (3.4b), and the positive signs are used when [formula omitted] and the negative signs when [formula omitted]
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The spectral amplitudes [formula omitted] (s) are given by [formula omitted] with [formula omitted] being the threefold Fourier transform of the source distribution, as defined by Eq. (3.7).
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27
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5644268272
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The effect of discarding all evanescent plane waves in the angular spectrum representation of the scalar dipole field [formula omitted] [see Eq. (3.14)] has been very clearly analyzed by
-
(1970)
Opt. Commun.
, vol.2
, pp. 142
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Carter, W.H.1
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28
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84951239947
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This result is, essentially, a three-dimensional analogue of a well-known theorem that the Fourier transform of a continuous function which vanishes outside a finite interval is a boundary value of an entire analytic function.
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This theorem follows at once from a well known result on analytic functions defined by definite integrals [cf., E. T. Copson, An Introduction to the Theory of Functions of a Complex Variable (Oxford U.P., London, 1962), Sec. 5.5]. The multidimensional form of the theorem is the well-known Plancherel-Pólya theorem [cf., B. A. Fuks, Introduction to the Theory of Analytic Functions of Several Complex Variables (Amer. Math. Soc. Providence, R.I., 1963), p. 352].
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32
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84951214548
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If, in addition to oscillating charges and current densities, there is a contribution from density of magnetization [formula omitted] one must replace [formula omitted] by [formula omitted] The introduction of magnetization makes it possible to take into account the effect of spin in the corresponding quantum mechanical formulation.
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-
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33
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84951214549
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Conversely, it is not difficult to show that the E and H fields that are the solutions to Eqs. (4.1) and which behave at infinity as outgoing spherical waves satisfy the full set of Maxwell equations everywhere.
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-
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34
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84951245585
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The angular spectrum representation (4.2) may, of course, be expressed in the vectorial generalization of the alternative form discussed in Footnote 21.
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37
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84951248996
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This fact may readily be deduced from the customary form of the completeness theorem (discussed, for example, in Ref. 11, pp. 798–799), which may be stated as follows: An arbitrary, well-behaved vector field [formula omitted] may be expanded in terms of three types of vector spherical harmonics [formula omitted] [formula omitted] and [formula omitted] in the form [formula omitted] where [formula omitted] [formula omitted] and [formula omitted] are functions of the radial coordinate [formula omitted] only. (The vector spherical harmonics [formula omitted] [formula omitted] and [formula omitted] correspond to [formula omitted] [formula omitted] and [formula omitted] respectively, of Ref. 11).
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The vector spherical harmonic [formula omitted] is, except for a normalization factor, the same function that we denoted by [formula omitted] more precisely [formula omitted]. Moreover, one has the relations [see Eqs. (B3) and (B9) of Ref. 31]: [formula omitted] and [formula omitted] where [formula omitted] is the unit vector in the radial direction. Since, according to these relations, the vector spherical harmonics [formula omitted] [formula omitted] and [formula omitted] are linearly independent combinations of [formula omitted] [formula omitted] and [formula omitted] it is clear that they too form a complete basis for the expansion of A(r). Moreover, [formula omitted] and [formula omitted] are tangential to the unit sphere [formula omitted] and [formula omitted] is perpendicular to it. Hence, the two types of vector spherical harmonics [formula omitted] and [formula omitted] form a complete set for arbitrary “tangential vector fields” A(r), i.e., an arbitrary, well-behaved, vector field A(r) such that [formula omitted] may be expanded in terms of them.
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38
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84951214264
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By making use of elementary vector identities and the fact that [formula omitted] one can rewrite (4.12a) in the form [formula omitted] Now, [formula omitted] is the Fourier transform [formula omitted] of the transverse part [formula omitted] of the current distribution [cf.
-
(American Elsevier, New York, 1964), Sec. 6.3]. Thus, (4.12a′) and (4.12b) show that all multipole moments, (and, consequently, the field outside the source region), depend only on those Fourier components [formula omitted] of the transverse part of the current distribution for which [formula omitted]
-
Introductory Quantum Electrodynamics
-
-
Power, E.A.1
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39
-
-
85087998592
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14.
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-
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40
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85087998430
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The decomposition (5.3) of the spectral amplitudes [formula omitted] and [formula omitted] which we obtained as a consequence of the completeness of the vector spherical harmonics [formula omitted] and [formula omitted] with respect to all well behaved fields [formula omitted] that are orthogonal to s [i.e., such that [formula omitted]], may also be obtained as a direct consequence of the so-called Hodge’s decomposition theorem [See, for example
-
14 employed this theorem in his treatment of the Debye representation, which, however, is quite different from ours.
-
(1946)
Commun. Math. Hel.
, vol.19
, pp. 1
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-
Bidal, P.1
de Rham, G.2
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41
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84951214262
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This identity follows from a well known general expression for vector spherical harmonics in terms of ordinary spherical harmonics. [See, for example, Eq. (1.5), p. 797 in Ref. 11].
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