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Legendre functions, table

The variation of Pn(ft) with ft for a few values of n is sliown in Fig. 5. Since, in most physical problems, the Legendre polynomial involved is usually / tl(cos 0) we have shown in Fig. fi the variation of this function with 0. Numerical values may be obtained from Tables of Associated Legendre Functions (Columbia University Press, 194-5),... [Pg.51]

Table V. gives the value of log10r(w) to four decimal places for all values of n between 1 and 2. It has been adapted from Legendre s tables to twelve decimal places in his Exercises de Calcul Integral, Paris, 2, 18, 1817. For all values of n between 1 and 2, log T(w) will be negative. Hence, as in the ordinary logarithmic tables of the trigonometrical functions, the tabular logarithm is often increased by the addition of 10 to the logarithm of T(w). This must be allowed for when arranging the final result. Table V. gives the value of log10r(w) to four decimal places for all values of n between 1 and 2. It has been adapted from Legendre s tables to twelve decimal places in his Exercises de Calcul Integral, Paris, 2, 18, 1817. For all values of n between 1 and 2, log T(w) will be negative. Hence, as in the ordinary logarithmic tables of the trigonometrical functions, the tabular logarithm is often increased by the addition of 10 to the logarithm of T(w). This must be allowed for when arranging the final result.
The functions Siyn 9) are well known in mathematics and are associated Legendre functions multiplied by a normalization constant. The associated Legendre functions are defined in Prob. 5.34. Table 5.1 gives the Siyn(O) functions for / < 3. [Pg.108]

The functions are the associated Legendre polynomials of which a few are given in Table 1.1. They are independent of Z, the nuclear charge number, and therefore are the same for all one-electron atoms. [Pg.13]

The im (9) functions are related to the associated Legendre polynomials, and the first few are listed in table 6.1. The R i(r) are the radial wave functions, known as associated Laguerre functions, the first few of which are listed in table 6.2. The quantities n, l and m in (6.8) are known as quantum numbers, and have the following allowed values ... [Pg.179]

For certain mathematical functions and operations it is necessary for the physicist to know their context, definition and mathematical properties, which we treat in the book. He does not need to know how to calculate them or to control their calculation. Numerical values of functions such as sinx have traditionally been taken from table books or slide rules. Modern computational facilities have enabled us to extend this concept, for example, to Coulomb functions, associated Legendre polynomials, Clebsch—Gordan and related coefficients, matrix inversion and diagonali-sation and Gaussian quadratures. The subroutine library has replaced the table book. We give references to suitable library subroutines. [Pg.338]

In this expression, P2 is the second Legendre polynomial and i(t) is a unit vector with the same orientation as the transition dipole at time t. The brackets indicate an ensemble average over all transition dipoles in the sample. The correlation function has a value of one at very short times when the orientation of y(t) has not changed from its initial orientation. At long times, the correlation function decays to zero because all memory of the initial orientation is lost. At intermediate times, the shape of the correlation function provides detailed information about the types of motions taking place. Table I shows the three theoretical models for the correlation function which we have compared with our experimental results. [Pg.75]

Tables 9.5 and 9.6 give some approximations for (o Xo ) and (O )(60) along with the applicable constraints. The wavelength X is that for the wave traveling in the fluid, and if nf 1, then X = X /nf, where X0 is for travel in vacuum. Table 9.6 shows the various approximations used to represent the phase function (O )(6o) in terms of Legendre polynomials. Tables 9.5 and 9.6 give some approximations for (o Xo ) and (O )(60) along with the applicable constraints. The wavelength X is that for the wave traveling in the fluid, and if nf 1, then X = X /nf, where X0 is for travel in vacuum. Table 9.6 shows the various approximations used to represent the phase function (O )(6o) in terms of Legendre polynomials.
TABLE 9.6 Phase Function in Terms of Legendre Polynomials... [Pg.678]

The 0 part of the differential in equation 11.46 does have a known solution. The solution is a set of functions known as associated Legendre polynomials. (As with the Hermite polynomials, differential equations of the form in equation 11.46 had been previously studied, by the French mathematician Adrien Legendre, but for different reasons.) These polynomials, listed in Table 11.3, are functions of 0 only, but have two indices labeling the functions. One of the indices, an integer denoted , indicates the maximum power, or order, of 0 terms. (It also indicates the total order of the combination of cos 0 and sin 0 terms.) The second index, m, specifies which... [Pg.358]


See other pages where Legendre functions, table is mentioned: [Pg.61]    [Pg.345]    [Pg.137]    [Pg.424]    [Pg.505]    [Pg.194]    [Pg.40]    [Pg.294]    [Pg.353]    [Pg.369]    [Pg.365]    [Pg.74]    [Pg.114]    [Pg.469]    [Pg.458]    [Pg.84]    [Pg.414]    [Pg.116]    [Pg.220]    [Pg.453]   
See also in sourсe #XX -- [ Pg.506 ]




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