When solving the equation for the geometry in spherical coordinates, the following equation for the radius arises
where γ \gamma is the eigenvalue, k k is a nonnegative integer.
Let us make the substitution R ( r ) R(r) = 1 r ⋅ R ^ ( r ) = \frac{\displaystyle 1}{\displaystyle \sqrt r} \cdot \widehat{R}(r) and carry out the transformations
d R ( r ) d r \displaystyle \frac{\displaystyle d R(r)}{\displaystyle dr} = d d r ( 1 r ⋅ R ^ ( r ) ) \displaystyle = \frac{\displaystyle d}{\displaystyle dr} \left( \frac{\displaystyle 1}{\displaystyle \sqrt r} \cdot \widehat{R}(r) \right) = − 1 2 ⋅ r ⋅ r ⋅ R ^ ( r ) \displaystyle = - \frac{\displaystyle 1}{\displaystyle 2 \cdot r \cdot \sqrt r} \cdot \widehat{R}(r) + 1 r ⋅ d R ^ ( r ) d r , \displaystyle + \frac{\displaystyle 1}{\displaystyle \sqrt r} \cdot \frac{\displaystyle d \widehat{R}(r)}{\displaystyle dr}, d 2 R ( r ) d r 2 \displaystyle \frac{\displaystyle d^2 R(r)}{\displaystyle dr^2} = − 1 2 ⋅ d d r ( 1 r ⋅ r ⋅ R ^ ( r ) ) \displaystyle = - \frac{\displaystyle 1}{\displaystyle 2} \cdot \frac{\displaystyle d}{\displaystyle dr} \left( \frac{\displaystyle 1}{\displaystyle r \cdot \sqrt r} \cdot \widehat{R}(r) \right) + d d r ( 1 r ⋅ d R ^ ( r ) d r ) , \displaystyle + \frac{\displaystyle d}{\displaystyle dr} \left( \frac{\displaystyle 1}{\displaystyle \sqrt r} \cdot \frac{\displaystyle d \widehat{R}(r)}{\displaystyle dr} \right), − 1 2 ⋅ d d r ( 1 r ⋅ r ⋅ R ^ ( r ) ) \displaystyle - \frac{\displaystyle 1}{\displaystyle 2} \cdot \frac{\displaystyle d}{\displaystyle dr} \left( \frac{\displaystyle 1}{\displaystyle r \cdot \sqrt r} \cdot \widehat{R}(r) \right) = 3 4 ⋅ 1 r 2 ⋅ r ⋅ R ^ ( r ) \displaystyle = \frac{\displaystyle 3}{\displaystyle 4} \cdot \frac{\displaystyle 1}{\displaystyle r^2 \cdot \sqrt r} \cdot \widehat{R}(r) − 1 2 ⋅ 1 r ⋅ r ⋅ d R ^ ( r ) d r , \displaystyle - \frac{\displaystyle 1}{\displaystyle 2} \cdot \frac{\displaystyle 1}{\displaystyle r \cdot \sqrt r} \cdot \frac{\displaystyle d \widehat{R}(r)}{\displaystyle dr}, d d r ( 1 r ⋅ d R ^ ( r ) d r ) \displaystyle \frac{\displaystyle d}{\displaystyle dr} \left( \frac{\displaystyle 1}{\displaystyle \sqrt r} \cdot \frac{\displaystyle d \widehat{R}(r)}{\displaystyle dr} \right) = − 1 2 ⋅ r ⋅ r ⋅ d R ^ ( r ) d r \displaystyle = - \frac{\displaystyle 1}{\displaystyle 2 \cdot r \cdot \sqrt r} \cdot \frac{\displaystyle d \widehat{R}(r)}{\displaystyle dr} + 1 r ⋅ d 2 R ^ ( r ) d r 2 , \displaystyle + \frac{\displaystyle 1}{\displaystyle \sqrt r} \cdot \frac{\displaystyle d^2 \widehat{R}(r)}{\displaystyle dr^2}, d 2 R ( r ) d r 2 \displaystyle \frac{\displaystyle d^2 R(r)}{\displaystyle dr^2} = 1 r ⋅ d 2 R ^ ( r ) d r 2 \displaystyle = \frac{\displaystyle 1}{\displaystyle \sqrt r} \cdot \frac{\displaystyle d^2 \widehat{R}(r)}{\displaystyle dr^2} − 1 r ⋅ r ⋅ d R ^ ( r ) d r \displaystyle - \frac{\displaystyle 1}{\displaystyle r \cdot \sqrt r} \cdot \frac{\displaystyle d \widehat{R}(r)}{\displaystyle dr} + 3 4 ⋅ 1 r 2 ⋅ r ⋅ R ^ ( r ) , \displaystyle + \frac{\displaystyle 3}{\displaystyle 4} \cdot \frac{\displaystyle 1}{\displaystyle r^2 \cdot \sqrt r} \cdot \widehat{R}(r), r 2 ⋅ d 2 R ( r ) d r 2 \displaystyle r^2 \cdot \frac{\displaystyle d^2 R(r)}{\displaystyle dr^2} = r ⋅ r ⋅ d 2 R ^ ( r ) d r 2 \displaystyle = r \cdot \sqrt r \cdot \frac{\displaystyle d^2 \widehat{R}(r)}{\displaystyle dr^2} − r ⋅ d R ^ ( r ) d r \displaystyle - \sqrt r \cdot \frac{\displaystyle d \widehat{R}(r)}{\displaystyle dr} + 3 4 ⋅ 1 r ⋅ R ^ ( r ) , \displaystyle + \frac{\displaystyle 3}{\displaystyle 4} \cdot \frac{\displaystyle 1}{\displaystyle \sqrt r} \cdot \widehat{R}(r), r 2 ⋅ d 2 R ( r ) d r 2 \displaystyle r^2 \cdot \frac{\displaystyle d^2 R(r)}{\displaystyle dr^2} + 2 ⋅ r ⋅ d R ( r ) d r \displaystyle + 2 \cdot r \cdot \frac{\displaystyle d R(r)}{\displaystyle dr} = r ⋅ r ⋅ d 2 R ^ ( r ) d r 2 \displaystyle = r \cdot \sqrt r \cdot \frac{\displaystyle d^2 \widehat{R}(r)}{\displaystyle dr^2} + r ⋅ d R ^ ( r ) d r \displaystyle + \sqrt r \cdot \frac{\displaystyle d \widehat{R}(r)}{\displaystyle dr} − 1 4 ⋅ 1 r ⋅ R ^ ( r ) , \displaystyle - \frac{\displaystyle 1}{\displaystyle 4} \cdot \frac{\displaystyle 1}{\displaystyle \sqrt r} \cdot \widehat{R}(r), we divide by r ⋅ r r \cdot \sqrt r and write equation (G.1 r 2 ⋅ d 2 R ( r ) d r 2 \displaystyle r^2 \cdot \frac{\displaystyle d^2 R(r)}{\displaystyle dr^2} + 2 ⋅ r ⋅ d R ( r ) d r \displaystyle + 2 \cdot r \cdot \frac{\displaystyle d R(r)}{\displaystyle dr} + ( r 2 ⋅ γ 2 − k ⋅ ( k + 1 ) ) ⋅ R ( r ) \displaystyle + \left( r^2 \cdot \gamma^2 - k \cdot (k + 1) \right) \cdot R(r) = 0 , \displaystyle = 0, ) in terms of the coefficients
ζ 1 ⋅ d 2 R ^ ( r ) d r 2 \displaystyle \zeta_1 \cdot \frac{\displaystyle d^2 \widehat{R}(r)}{\displaystyle dr^2} + ζ 2 ⋅ d R ^ ( r ) d r \displaystyle + \zeta_2 \cdot \frac{\displaystyle d \widehat{R}(r)}{\displaystyle dr} + ζ 3 ⋅ R ^ ( r ) \displaystyle + \zeta_3 \cdot \widehat{R}(r) = 0 , \displaystyle = 0, and now let us determine the coefficients, first transforming the free term
γ 2 \displaystyle \gamma^2 − k ⋅ ( k + 1 ) r 2 \displaystyle - \frac{\displaystyle k \cdot (k + 1)}{\displaystyle r^2} − 1 4 ⋅ r 2 \displaystyle - \frac{\displaystyle 1}{\displaystyle 4 \cdot r^2} = γ 2 \displaystyle = \gamma^2 − ( k + 1 / 2 ) 2 r 2 , \displaystyle - \frac{\displaystyle (k + 1/2)^2}{\displaystyle r^2}, ζ 1 \displaystyle \zeta_1 = 1 , ζ 2 \displaystyle = 1, \quad \zeta_2 = 1 r , ζ 3 \displaystyle = \frac{\displaystyle 1}{\displaystyle r}, \quad \zeta_3 = γ 2 \displaystyle = \gamma^2 − ( k + 1 / 2 ) 2 r 2 , \displaystyle - \frac{\displaystyle (k + 1/2)^2}{\displaystyle r^2}, thus, equation (G.1 r 2 ⋅ d 2 R ( r ) d r 2 \displaystyle r^2 \cdot \frac{\displaystyle d^2 R(r)}{\displaystyle dr^2} + 2 ⋅ r ⋅ d R ( r ) d r \displaystyle + 2 \cdot r \cdot \frac{\displaystyle d R(r)}{\displaystyle dr} + ( r 2 ⋅ γ 2 − k ⋅ ( k + 1 ) ) ⋅ R ( r ) \displaystyle + \left( r^2 \cdot \gamma^2 - k \cdot (k + 1) \right) \cdot R(r) = 0 , \displaystyle = 0, ) takes the form
d 2 R ^ ( r ) d r 2 \displaystyle \frac{\displaystyle d^2 \widehat{R}(r)}{\displaystyle dr^2} + 1 r ⋅ d R ^ ( r ) d r \displaystyle + \frac{\displaystyle 1}{\displaystyle r} \cdot \frac{\displaystyle d \widehat{R}(r)}{\displaystyle dr} + ( γ 2 − ( k + 1 / 2 ) 2 r 2 ) ⋅ R ^ ( r ) \displaystyle + \left( \gamma^2 - \frac{\displaystyle (k + 1/2)^2}{\displaystyle r^2} \right) \cdot \widehat{R}(r) = 0. \displaystyle = 0. We have obtained the Bessel equation with half-integer index k k + 1 / 2 + 1/2 . Its solutions bounded at zero are the Bessel functions of the first kind R ^ ( r ) \widehat{R}(r) = J k + 1 / 2 ( γ ⋅ r ) = J_{k + 1/2}(\gamma \cdot r) , k k ∈ ( 0.. ∞ ) \in (0..\infty) ; the solutions of the second kind Y k + 1 / 2 ( γ ⋅ r ) Y_{k + 1/2}(\gamma \cdot r) are infinite at zero, as seen in figure (B.2) , and are discarded by the boundedness condition. Thus, the solution of the original equation (G.1 r 2 ⋅ d 2 R ( r ) d r 2 \displaystyle r^2 \cdot \frac{\displaystyle d^2 R(r)}{\displaystyle dr^2} + 2 ⋅ r ⋅ d R ( r ) d r \displaystyle + 2 \cdot r \cdot \frac{\displaystyle d R(r)}{\displaystyle dr} + ( r 2 ⋅ γ 2 − k ⋅ ( k + 1 ) ) ⋅ R ( r ) \displaystyle + \left( r^2 \cdot \gamma^2 - k \cdot (k + 1) \right) \cdot R(r) = 0 , \displaystyle = 0, ) has the form
where J k + 1 / 2 ( γ ⋅ r ) J_{k + 1/2}(\gamma \cdot r) is the Bessel function of the first kind with half-integer index. Up to a constant factor it is the spherical Bessel function: j k ( γ ⋅ r ) j_k(\gamma \cdot r) = π 2 ⋅ γ ⋅ r ⋅ J k + 1 / 2 ( γ ⋅ r ) = \sqrt{\frac{\displaystyle \pi}{\displaystyle 2 \cdot \gamma \cdot r}} \cdot J_{k + 1/2}(\gamma \cdot r) .
F. Norm of the Legendre polynomials H. Spherical Bessel function norm (Neumann)