15. Legendre Functions Legendre Polynomials Orthogonality

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Presentation transcript:

15. Legendre Functions Legendre Polynomials Orthogonality Physical Interpretation of Generating Function Associated Legendre Equation Spherical Harmonics Legendre Functions of the Second Kind

Schrodinger eq. for a central potential  Associated Legendre eq.  Legendre eq. with

1. Legendre Polynomials Legendre eq.   x = 1 & x =  are regular singular points.

Frobenius Series See § 8.3 & Mathematica  Indicial eq.  series diverges for x2 1 unless terminated Set a1 = 0  a2 j + 1 = 0 s = 0  even order : s = 1  odd order :

Generating Function    

 &  highest power of x in coeff. of tn is n.  Coeff. of xn in Pn(x) = Coeff. of xn tn  Coeff. of highest power of x in Pn(x)

Summary Power Expansion : Ex.15.1.2

Recurrence Relations   

Table 15.1. Legendre Polynomials  Mathematica

  & Eliminate x Pn1 term 

More Recurrence Relations Any set of functions satisfying these recurrence relations also satisfy the Legendre ODE. Ex.15.1.1

Upper & Lower Bounds for Pn (cos ) 

 Coeff. invariant under j   j   Coeff. invariant under j   ( j+1) 

For P2n , x = 1 are global max. For P2n+1 , x = +1 is a gloabal max, while x = 1 is a gloabal min. Mathematica

Rodrigues Formula From § 12.1 : If has self-adjoint form then Legendre eq. : Self-adjoint form :  

Coefficient of xn in Pn(x) Coefficient of xn is :  

2. Orthogonality is self-adjoint [ w(x) = 1 ]   Pn(x) are orthogonal polynomials in [ 1, 1 ].

Normalization  Let    via Rodrigues formula : Ex.15.2.1

Legendre Series Eigenfunctions of an ODE are complete  { Pn (x) } is completeness over [1,1] .  For any function f (x) in [1,1] :  unique

Solutions to Laplace Eq. in Spherical Coordinates General solution : finite  l = 0,1,2, … Solution with no azimuthal dependence ( m = 0 ) : Solution that is finite inside & outside a boundary sphere :

Example 15.2.1 Earth’s Gravitational Field Gravitational potential U in mass-free region : Neglect azimuthal dependence : Earth’s radius at equator g includes rotational effect Note: Let  al dimensionless Earth is a sphere  

Slightly distorted Earth with axial symmetry :  CM located at origin  See Mathematica for proof.  Experimental data : Data including longitudinal dependence is described by a Laplace series (§15.5).

Example 15.2.2 Sphere in a Uniform Field Grounded conducting sphere (radius r0 ) in uniform applied electric field everywhere  For :  

Surface charge density : SI units induced dipole moment Ex.15.2.11 Mathematica

Example 15.2.3 Electrostatic Potential for a Ring of Charge Thin, conducting ring of radius a, centered at origin & lying in x-y plane, has total charge q. Outside the ring, Axial symmetry  no  dependence Mathematica For r > a : On z-axis, Coulomb’s law gives :

  See Eg.15.4.2 for magnetic analog.

3. Physical Interpretation of Generating Function Leading term : (point charge)  for r > a.  for r < a.

Expansion of 1 / | r  r | Let :  either r or r on z-axis

Electric Multipoles Electric dipole : point dipole Leading term :

(Linear) Multipoles Let = 2l -pole potential with center of charge at z = r. Mono ( 20 ) -pole : Di ( 21 ) -pole : Quadru ( 22 ) –pole : ( 2l ) –pole : Quadrupole Mathematica

Multipole Expansion If all charges are on the z-axis & within the interval [zm , zm ] : for r > zm where is the (linear) 2l –pole moment. For a discrete set of charges qi at z = ai . 

If one shifts the coord origin to Z. l is independent of coord, i.e.,  Z iff Multipole expansion for a general (r) are done in terms of the spherical harmonics.