Bessel's Special Function (Part - 5) - Mathematical Methods of Physics, UGC - NET Physics Physics Notes | EduRev

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Physics : Bessel's Special Function (Part - 5) - Mathematical Methods of Physics, UGC - NET Physics Physics Notes | EduRev

The document Bessel's Special Function (Part - 5) - Mathematical Methods of Physics, UGC - NET Physics Physics Notes | EduRev is a part of the Physics Course Physics for IIT JAM, UGC - NET, CSIR NET.
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SPHERICAL BESSEL FUNCTIONS

When the Helmholtz equation is separated in spherical coordinates, the radial equation has the form

Bessel`s Special Function (Part - 5) - Mathematical Methods of Physics, UGC - NET Physics Physics Notes | EduRev

This is Eq. (9.65) of Section 9.3. The parameter k enters from the original Helmholtz equation, while n(n + 1) is a separation constant. From the behavior of the polar angle function (Legendre’s equation, Sections 9.5 and 12.5), the separation constant must have this form, with n a nonnegative integer. Equation (11.139) has the virtue of being selfadjoint, but clearly it is not Bessel’s equation. However, if we substitute

Bessel`s Special Function (Part - 5) - Mathematical Methods of Physics, UGC - NET Physics Physics Notes | EduRev

Equation (11.139) becomes

Bessel`s Special Function (Part - 5) - Mathematical Methods of Physics, UGC - NET Physics Physics Notes | EduRev

which is Bessel’s equation. Z is a Bessel function of order Bessel`s Special Function (Part - 5) - Mathematical Methods of Physics, UGC - NET Physics Physics Notes | EduRev (n an integer). Because of the importance of spherical coordinates, this combination, that is,

Bessel`s Special Function (Part - 5) - Mathematical Methods of Physics, UGC - NET Physics Physics Notes | EduRev

occurs quite often.

 

Definitions

It is convenient to label these functions spherical Bessel functions with the following defining equations:

Bessel`s Special Function (Part - 5) - Mathematical Methods of Physics, UGC - NET Physics Physics Notes | EduRev

These spherical Bessel functions (Figs. 11.13 and 11.14) can be expressed in series form by using the series (Eq. (11.5)) for Jn , replacing n with Bessel`s Special Function (Part - 5) - Mathematical Methods of Physics, UGC - NET Physics Physics Notes | EduRev

Bessel`s Special Function (Part - 5) - Mathematical Methods of Physics, UGC - NET Physics Physics Notes | EduRev         (11.142)

Using the Legendre duplication formula,

Bessel`s Special Function (Part - 5) - Mathematical Methods of Physics, UGC - NET Physics Physics Notes | EduRev              (11.143)

we have

Bessel`s Special Function (Part - 5) - Mathematical Methods of Physics, UGC - NET Physics Physics Notes | EduRev

Bessel`s Special Function (Part - 5) - Mathematical Methods of Physics, UGC - NET Physics Physics Notes | EduRev

This yields

Bessel`s Special Function (Part - 5) - Mathematical Methods of Physics, UGC - NET Physics Physics Notes | EduRev

Bessel`s Special Function (Part - 5) - Mathematical Methods of Physics, UGC - NET Physics Physics Notes | EduRev

Bessel`s Special Function (Part - 5) - Mathematical Methods of Physics, UGC - NET Physics Physics Notes | EduRev

The Legendre duplication formula can be used again to give

Bessel`s Special Function (Part - 5) - Mathematical Methods of Physics, UGC - NET Physics Physics Notes | EduRev              (11.147)

These series forms, Eqs. (11.144) and (11.147), are useful in three ways: (1) limiting values as x → 0, (2) closed-form representations for n = 0, and, as an extension of this, (3) an indication that the spherical Bessel functions are closely related to sine and cosine.
For the special case n = 0 we find from Eq. (11.144) that

Bessel`s Special Function (Part - 5) - Mathematical Methods of Physics, UGC - NET Physics Physics Notes | EduRev            (11.148)

whereas for n0 , Eq. (11.147) yields

Bessel`s Special Function (Part - 5) - Mathematical Methods of Physics, UGC - NET Physics Physics Notes | EduRev          (11.149)

From the definition of the spherical Hankel functions (Eq. (11.141)),

Bessel`s Special Function (Part - 5) - Mathematical Methods of Physics, UGC - NET Physics Physics Notes | EduRev              (11.150)

Equations (11.148) and (11.149) suggest expressing all spherical Bessel functions as combinations of sine and cosine. The appropriate combinations can be developed from the power-series solutions, Eqs. (11.144) and (11.147), but this approach is awkward. Actually the trigonometric forms are already available as the asymptotic expansion of Section 11.6.
From Eqs. (11.131) and (11.129a),

Bessel`s Special Function (Part - 5) - Mathematical Methods of Physics, UGC - NET Physics Physics Notes | EduRev(11.151)

Now, Pn+1/2   and Qn+1/2 are polynomials. This means that Eq. (11.151) is mathematically exact, not simply an asymptotic approximation. We obtain

Bessel`s Special Function (Part - 5) - Mathematical Methods of Physics, UGC - NET Physics Physics Notes | EduRev(11.152)

Bessel`s Special Function (Part - 5) - Mathematical Methods of Physics, UGC - NET Physics Physics Notes | EduRev

Bessel`s Special Function (Part - 5) - Mathematical Methods of Physics, UGC - NET Physics Physics Notes | EduRev

Bessel`s Special Function (Part - 5) - Mathematical Methods of Physics, UGC - NET Physics Physics Notes | EduRev

and so on.

 

Limiting Values

For x ≪ 1,26 Eqs. (11.144) and (11.147) yield

Bessel`s Special Function (Part - 5) - Mathematical Methods of Physics, UGC - NET Physics Physics Notes | EduRev

The transformation of factorials in the expressions for nn (x ) employs Exercise 8.1.3. The limiting values of the spherical Hankel functions go as ±inn (x ).
The asymptotic values of jn ,nn ,Bessel`s Special Function (Part - 5) - Mathematical Methods of Physics, UGC - NET Physics Physics Notes | EduRev , and Bessel`s Special Function (Part - 5) - Mathematical Methods of Physics, UGC - NET Physics Physics Notes | EduRev may be obtained from the Bessel asymptotic forms, Section 11.6. We find

Bessel`s Special Function (Part - 5) - Mathematical Methods of Physics, UGC - NET Physics Physics Notes | EduRev

Bessel`s Special Function (Part - 5) - Mathematical Methods of Physics, UGC - NET Physics Physics Notes | EduRev

The condition for these spherical Bessel forms is that x ≫ n(n + 1)/2. From these asymptotic values we see that jn (x ) and nn (x ) are appropriate for a description of standing spherical waves; Bessel`s Special Function (Part - 5) - Mathematical Methods of Physics, UGC - NET Physics Physics Notes | EduRev (x ) and Bessel`s Special Function (Part - 5) - Mathematical Methods of Physics, UGC - NET Physics Physics Notes | EduRev (x ) correspond to traveling spherical waves. If the time dependence for the traveling waves is taken to be e−iωt , then Bessel`s Special Function (Part - 5) - Mathematical Methods of Physics, UGC - NET Physics Physics Notes | EduRev (x ) yields an outgoing traveling spherical wave, Bessel`s Special Function (Part - 5) - Mathematical Methods of Physics, UGC - NET Physics Physics Notes | EduRev (x ) an incoming wave. Radiation theory in electromagnetism and scattering theory in quantum mechanics provide many applications.

 

Recurrence Relations

The recurrence relations to which we now turn provide a convenient way of developing the higher-order spherical Bessel functions. These recurrence relations may be derived from the series, but, as with the modified Bessel functions, it is easier to substitute into the known recurrence relations (Eqs. (11.10) and (11.12)). This gives

Bessel`s Special Function (Part - 5) - Mathematical Methods of Physics, UGC - NET Physics Physics Notes | EduRev

Rearranging these relations (or substituting into Eqs. (11.15) and (11.17)), we obtain

Bessel`s Special Function (Part - 5) - Mathematical Methods of Physics, UGC - NET Physics Physics Notes | EduRev

Here fmay represent  Bessel`s Special Function (Part - 5) - Mathematical Methods of Physics, UGC - NET Physics Physics Notes | EduRev

The specific forms, Eqs. (11.154) and (11.155), may also be readily obtained from Eq. (11.164).
By mathematical induction we may establish the Rayleigh formulas

Bessel`s Special Function (Part - 5) - Mathematical Methods of Physics, UGC - NET Physics Physics Notes | EduRev

Bessel`s Special Function (Part - 5) - Mathematical Methods of Physics, UGC - NET Physics Physics Notes | EduRev

 

Orthogonality

We may take the orthogonality integral for the ordinary Bessel functions (Eqs. (11.49) and (11.50)),

Bessel`s Special Function (Part - 5) - Mathematical Methods of Physics, UGC - NET Physics Physics Notes | EduRev

and substitute in the expression for jn to obtain

Bessel`s Special Function (Part - 5) - Mathematical Methods of Physics, UGC - NET Physics Physics Notes | EduRev

Here αnp and αnq are roots of jn .
This represents orthogonality with respect to the roots of the Bessel functions. An illustration of this sort of orthogonality is provided in Example 11.7.1, the problem of a particle in a sphere. Equation (11.169) guarantees orthogonality of the wave functions jn (r ) for fixed n. (If n varies, the accompanying spherical harmonic will provide orthogonality.)

 

Example 11.7.1 PARTICLE IN A SPHERE

An illustration of the use of the spherical Bessel functions is provided by the problem of a quantum mechanical particle in a sphere of radius a . Quantum theory requires that the wave function ψ , describing our particle, satisfy
Bessel`s Special Function (Part - 5) - Mathematical Methods of Physics, UGC - NET Physics Physics Notes | EduRev

and the boundary conditions (1) ψ(r ≤ a) remains finite, (2) ψ(a ) = 0. This corresponds to a square-well potential V = 0, r ≤ a , and V =∞, r> a .Here h¯ is Planck’s constant divided by 2π, m is the mass of our particle, and E is, its energy. Let us determine the minimum value of the energy for which our wave equation has an acceptable solution.
Equation (11.170) is Helmholtz’s equation with a radial part (compare Section 9.3 for separation of variables):

Bessel`s Special Function (Part - 5) - Mathematical Methods of Physics, UGC - NET Physics Physics Notes | EduRev

We choose the orbital angular momentum index n = 0, for any angular dependence would raise the energy. The spherical Neumann function is rejected because of its divergent behavior at the origin. To satisfy the second boundary condition (for all angles), we require

Bessel`s Special Function (Part - 5) - Mathematical Methods of Physics, UGC - NET Physics Physics Notes | EduRev            (11.172)

where α is a root of j, that is, j0 (α) = 0. This has the effect of limiting the allowable energies to a certain discrete set, or, in other words, application of boundary condition (2) quantizes the energy E . The smallest α is the first zero of j0 ,

α = π,

and

Bessel`s Special Function (Part - 5) - Mathematical Methods of Physics, UGC - NET Physics Physics Notes | EduRev      (11.173)

which means that for any finite sphere the particle energy will have a positive minimum or zero-point energy. This is an illustration of the Heisenberg uncertainty principle for Δp with Δr ≤ a .
In solid-state physics, astrophysics, and other areas of physics, we may wish to know how many different solutions (energy states) correspond to energies less than or equal to some fixed energy E0 . For a cubic volume (Exercise 9.3.5) the problem is fairly simple.
The considerably more difficult spherical case is worked out by R. H. Lambert, Am. J.
Phys. 36: 417, 1169 (1968).
The relevant orthogonality relation for the jn (kr ) can be derived from the integral given in Exercise 11.7.23.

Another form, orthogonality with respect to the indices, may be written as

Bessel`s Special Function (Part - 5) - Mathematical Methods of Physics, UGC - NET Physics Physics Notes | EduRev

The proof is left as Exercise 11.7.10. If m = n (compare Exercise 11.7.11), we have 

Bessel`s Special Function (Part - 5) - Mathematical Methods of Physics, UGC - NET Physics Physics Notes | EduRev

Most physical applications of orthogonal Bessel and spherical Bessel functions involve orthogonality with varying roots and an interval [0,a ] and Eqs. (11.168) and (11.169) and Exercise 11.7.23 for continuous-energy eigenvalues.
The spherical Bessel functions will enter again in connection with spherical waves, but further consideration is postponed until the corresponding angular functions, the Legendre functions, have been introduced.

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