10.67 Asymptotic Expansions for Large Argument10.69 Uniform Asymptotic Expansions for Large Order

§10.68 Modulus and Phase Functions

Contents

§10.68(ii) Basic Properties

10.68.3
\mathop{\mathrm{ber}_{{\nu}}\/}\nolimits x=\mathop{M_{{\nu}}\/}\nolimits\!\left(x\right)\mathop{\cos\/}\nolimits\mathop{\theta _{{\nu}}\/}\nolimits\!\left(x\right),
\mathop{\mathrm{bei}_{{\nu}}\/}\nolimits x=\mathop{M_{{\nu}}\/}\nolimits\!\left(x\right)\mathop{\sin\/}\nolimits\mathop{\theta _{{\nu}}\/}\nolimits\!\left(x\right),
10.68.4
\mathop{\mathrm{ker}_{{\nu}}\/}\nolimits x=\mathop{N_{{\nu}}\/}\nolimits\!\left(x\right)\mathop{\cos\/}\nolimits\mathop{\phi _{{\nu}}\/}\nolimits\!\left(x\right),
\mathop{\mathrm{kei}_{{\nu}}\/}\nolimits x=\mathop{N_{{\nu}}\/}\nolimits\!\left(x\right)\mathop{\sin\/}\nolimits\mathop{\phi _{{\nu}}\/}\nolimits\!\left(x\right).
10.68.5
\mathop{M_{{\nu}}\/}\nolimits\!\left(x\right)=({\mathop{\mathrm{ber}_{{\nu}}\/}\nolimits^{{2}}}x+{\mathop{\mathrm{bei}_{{\nu}}\/}\nolimits^{{2}}}x)^{{\ifrac{1}{2}}},
\mathop{N_{{\nu}}\/}\nolimits\!\left(x\right)=({\mathop{\mathrm{ker}_{{\nu}}\/}\nolimits^{{2}}}x+{\mathop{\mathrm{kei}_{{\nu}}\/}\nolimits^{{2}}}x)^{{\ifrac{1}{2}}},
10.68.6
\mathop{\theta _{{\nu}}\/}\nolimits\!\left(x\right)=\mathop{\mathrm{Arctan}\/}\nolimits\!\left(\mathop{\mathrm{bei}_{{\nu}}\/}\nolimits x/\mathop{\mathrm{ber}_{{\nu}}\/}\nolimits x\right),
\mathop{\phi _{{\nu}}\/}\nolimits\!\left(x\right)=\mathop{\mathrm{Arctan}\/}\nolimits\!\left(\mathop{\mathrm{kei}_{{\nu}}\/}\nolimits x/\mathop{\mathrm{ker}_{{\nu}}\/}\nolimits x\right).
10.68.7
\mathop{M_{{-n}}\/}\nolimits\!\left(x\right)=\mathop{M_{{n}}\/}\nolimits\!\left(x\right),
\mathop{\theta _{{-n}}\/}\nolimits\!\left(x\right)=\mathop{\theta _{{n}}\/}\nolimits\!\left(x\right)-n\pi.

With arguments (x) suppressed,

10.68.8 {\mathop{\mathrm{ber}_{{\nu}}\/}\nolimits^{{\prime}}}x=\tfrac{1}{2}\mathop{M_{{\nu+1}}\/}\nolimits\mathop{\cos\/}\nolimits\!\left(\mathop{\theta _{{\nu+1}}\/}\nolimits-\tfrac{1}{4}\pi\right)-\tfrac{1}{2}\mathop{M_{{\nu-1}}\/}\nolimits\mathop{\cos\/}\nolimits\!\left(\mathop{\theta _{{\nu-1}}\/}\nolimits-\tfrac{1}{4}\pi\right)=(\nu/x)\mathop{M_{{\nu}}\/}\nolimits\mathop{\cos\/}\nolimits\mathop{\theta _{{\nu}}\/}\nolimits+\mathop{M_{{\nu+1}}\/}\nolimits\mathop{\cos\/}\nolimits\!\left(\mathop{\theta _{{\nu+1}}\/}\nolimits-\tfrac{1}{4}\pi\right)=-(\nu/x)\mathop{M_{{\nu}}\/}\nolimits\mathop{\cos\/}\nolimits\mathop{\theta _{{\nu}}\/}\nolimits-\mathop{M_{{\nu-1}}\/}\nolimits\mathop{\cos\/}\nolimits\!\left(\mathop{\theta _{{\nu-1}}\/}\nolimits-\tfrac{1}{4}\pi\right),
10.68.9 {\mathop{\mathrm{bei}_{{\nu}}\/}\nolimits^{{\prime}}}x=\tfrac{1}{2}\mathop{M_{{\nu+1}}\/}\nolimits\mathop{\sin\/}\nolimits\!\left(\mathop{\theta _{{\nu+1}}\/}\nolimits-\tfrac{1}{4}\pi\right)-\tfrac{1}{2}\mathop{M_{{\nu-1}}\/}\nolimits\mathop{\sin\/}\nolimits\!\left(\mathop{\theta _{{\nu-1}}\/}\nolimits-\tfrac{1}{4}\pi\right)=(\nu/x)\mathop{M_{{\nu}}\/}\nolimits\mathop{\sin\/}\nolimits\mathop{\theta _{{\nu}}\/}\nolimits+\mathop{M_{{\nu+1}}\/}\nolimits\mathop{\sin\/}\nolimits\!\left(\mathop{\theta _{{\nu+1}}\/}\nolimits-\tfrac{1}{4}\pi\right)=-(\nu/x)\mathop{M_{{\nu}}\/}\nolimits\mathop{\sin\/}\nolimits\mathop{\theta _{{\nu}}\/}\nolimits-\mathop{M_{{\nu-1}}\/}\nolimits\mathop{\sin\/}\nolimits\!\left(\mathop{\theta _{{\nu-1}}\/}\nolimits-\tfrac{1}{4}\pi\right).
10.68.10
{\mathop{\mathrm{ber}\/}\nolimits^{{\prime}}}x=\mathop{M_{{1}}\/}\nolimits\mathop{\cos\/}\nolimits\!\left(\mathop{\theta _{{1}}\/}\nolimits-\tfrac{1}{4}\pi\right),
{\mathop{\mathrm{bei}\/}\nolimits^{{\prime}}}x=\mathop{M_{{1}}\/}\nolimits\mathop{\sin\/}\nolimits\!\left(\mathop{\theta _{{1}}\/}\nolimits-\tfrac{1}{4}\pi\right).
10.68.11 {\mathop{M_{{\nu}}\/}\nolimits^{{\prime}}}=(\nu/x)\mathop{M_{{\nu}}\/}\nolimits+\mathop{M_{{\nu+1}}\/}\nolimits\mathop{\cos\/}\nolimits\!\left(\mathop{\theta _{{\nu+1}}\/}\nolimits-\mathop{\theta _{{\nu}}\/}\nolimits-\tfrac{1}{4}\pi\right)=-(\nu/x)\mathop{M_{{\nu}}\/}\nolimits-\mathop{M_{{\nu-1}}\/}\nolimits\mathop{\cos\/}\nolimits\!\left(\mathop{\theta _{{\nu-1}}\/}\nolimits-\mathop{\theta _{{\nu}}\/}\nolimits-\tfrac{1}{4}\pi\right),
10.68.12 {\mathop{\theta _{{\nu}}\/}\nolimits^{{\prime}}}=(\mathop{M_{{\nu+1}}\/}\nolimits/\mathop{M_{{\nu}}\/}\nolimits)\mathop{\sin\/}\nolimits\!\left(\mathop{\theta _{{\nu+1}}\/}\nolimits-\mathop{\theta _{{\nu}}\/}\nolimits-\tfrac{1}{4}\pi\right)=-(\mathop{M_{{\nu-1}}\/}\nolimits/\mathop{M_{{\nu}}\/}\nolimits)\mathop{\sin\/}\nolimits\!\left(\mathop{\theta _{{\nu-1}}\/}\nolimits-\mathop{\theta _{{\nu}}\/}\nolimits-\tfrac{1}{4}\pi\right).
10.68.13
{\mathop{M_{{0}}\/}\nolimits^{{\prime}}}=\mathop{M_{{1}}\/}\nolimits\mathop{\cos\/}\nolimits\!\left(\mathop{\theta _{{1}}\/}\nolimits-\mathop{\theta _{{0}}\/}\nolimits-\tfrac{1}{4}\pi\right),
{\mathop{\theta _{{0}}\/}\nolimits^{{\prime}}}=(\mathop{M_{{1}}\/}\nolimits/\mathop{M_{{0}}\/}\nolimits)\mathop{\sin\/}\nolimits\!\left(\mathop{\theta _{{1}}\/}\nolimits-\mathop{\theta _{{0}}\/}\nolimits-\tfrac{1}{4}\pi\right).
10.68.14
\ifrac{d(x{\mathop{M_{{\nu}}\/}\nolimits^{{2}}}{\mathop{\theta _{{\nu}}\/}\nolimits^{{\prime}}})}{dx}=x{\mathop{M_{{\nu}}\/}\nolimits^{{2}}},
x^{2}{\mathop{M_{{\nu}}\/}\nolimits^{{\prime\prime}}}+x{\mathop{M_{{\nu}}\/}\nolimits^{{\prime}}}-\nu^{2}\mathop{M_{{\nu}}\/}\nolimits=x^{2}\mathop{M_{{\nu}}\/}\nolimits{{\mathop{\theta _{{\nu}}\/}\nolimits^{{\prime}}}^{{2}}}.

Equations (10.68.8)–(10.68.14) also hold with the symbols \mathop{\mathrm{ber}\/}\nolimits, \mathop{\mathrm{bei}\/}\nolimits, \mathop{M\/}\nolimits, and \mathop{\theta\/}\nolimits replaced throughout by \mathop{\mathrm{ker}\/}\nolimits, \mathop{\mathrm{kei}\/}\nolimits, \mathop{N\/}\nolimits, and \mathop{\phi\/}\nolimits, respectively. In place of (10.68.7),

10.68.15
\mathop{N_{{-\nu}}\/}\nolimits\!\left(x\right)=\mathop{N_{{\nu}}\/}\nolimits\!\left(x\right),
\mathop{\phi _{{-\nu}}\/}\nolimits\!\left(x\right)=\mathop{\phi _{{\nu}}\/}\nolimits\!\left(x\right)+\nu\pi.

§10.68(iii) Asymptotic Expansions for Large Argument

When \nu is fixed, \mu=4\nu^{2}, and x\to\infty

§10.68(iv) Further Properties

Additional properties of the modulus and phase functions are given in Young and Kirk (1964, pp. xi–xv). However, care needs to be exercised with the branches of the phases. Thus this reference gives \mathop{\phi _{{1}}\/}\nolimits\!\left(0\right)=\tfrac{5}{4}\pi (Eq. (6.10)), and \lim _{{x\to\infty}}(\mathop{\phi _{{1}}\/}\nolimits\!\left(x\right)+(x/\sqrt{2}))=-\tfrac{5}{8}\pi (Eqs. (10.20) and (Eqs. (10.26b)). However, numerical tabulations show that if the second of these equations applies and \mathop{\phi _{{1}}\/}\nolimits\!\left(x\right) is continuous, then \mathop{\phi _{{1}}\/}\nolimits\!\left(0\right)=-\tfrac{3}{4}\pi; compare Abramowitz and Stegun (1964, p. 433).