Lecture 17 Hydrogenic atom (c) So Hirata, Department of Chemistry, University of Illinois at Urbana-Champaign. This material has been developed and made available online by work supported jointly by University of Illinois, the National Science Foundation under Grant CHE-1118616 (CAREER), and the Camille & Henry Dreyfus Foundation, Inc. through the Camille Dreyfus Teacher-Scholar program. Any opinions, findings, and conclusions or recommendations expressed in this material are those of the author(s) and do not necessarily reflect the views of the sponsoring agencies. Hydrogenic atom We study the Schrödinger equation of the hydrogenic atom, of which exact, analytical solution exists. We add to our repertories another special function – associated Laguerre polynomials – solutions of the radial part of the hydrogenic atom’s Schrödinger equation. Coulomb potential The potential energy between a nucleus with atomic number Z and an electron is Proportional to nuclear charge 2 V Attractive Ze 4 0 r Inversely proportional to distance Hamiltonian of hydrogenic atom The Classical total energy in Cartesian coordinates is 1 1 Ze 2 2 E = mnx n + mex e 2 2 4pe 0 x e - x n 2 2 1 1 Ze 2 2 = MX + mx 2 2 4pe 0 x Center of mass Relative motion motion mnx n + mex e mn me M = mn + me ; X = ; m= ; x = xe - xn M mn + me The Schrödinger equation Center of mass motion Relative motion 2 2 2 æ ö Ze 2 2 ÑX Ñx ç÷ Y ( X,x ) = EY ( X,x ) 2m 4pe 0 x ø è 2M 6-dimensional equation! Separation of variables 2 2 2 æ ö Ze 2 2 ÑX Ñx ç÷ F ( X ) Q ( x ) = EF ( X ) Q ( x ) 2m 4pe 0 x ø è 2M - 2 2M QÑ 2X F - 2 2m FÑ 2x Q - Ze2 4pe 0 x FQ = EFQ 2 1 2 1 2 Ze2 ÑXF ÑxQ = E Separable into 3 + 3 dimensions 2M F 2m Q 4pe 0 x 2 Center of mass motion Relative motion The Schrödinger equation - Two Schrödinger equations 2 2M 2 2m Ñ F ( X ) = ECOM F ( X ) 2 X Ñ Q(x ) 2 x Ze2 4pe 0 x Hydrogen’s gas-phase dynamics (3D particle in a box) Q ( x ) = ErelativeQ ( x ) Hydrogen’s atomic structure In spherical coordinates centered at the nucleus 2 2 æ ö Ze 2 ç - 2m Ñ - 4pe r ÷ Y ( r,q ,j ) = EY ( r,q ,j ) è 0 ø Further separation of variables The Schrödinger eq. for atomic structure: 2 2 æ Ze ö 2 ç - 2m Ñ - 4pe r ÷ Y(r,q ,j ) = EY(r,q ,j ) è 0 ø Still 3 dimensional! Can we further separate variables? YES ( r , , ) R ( r )Y ( , ) Further separation of variables 2 æ Ze2 ö 2 ç - 2 m Ñ - 4pe r ÷ R(r)Y (q ,j ) = ER(r)Y (q ,j ) è 0 ø é ù ê ú 2 ê ¶2 2 ¶ 1 æ 1 ¶2 1 ¶ ¶ öú Ze2 + 2ç 2 + sin q ÷ ú RY RY = ERY ê 2+ 2 2 m ê ¶r r ¶r r è sin q ¶f sin q ¶q ¶q ø ú 4pe 0r ê ú êë úû 2 2 æ ¶2 2 ¶ ö L Ze2 Yç 2 + RR 2YRY = ERY ÷ 2 m è ¶r r ¶r ø 2m r 4pe r =L 0 2 æ ¶2 2 ¶ ö L Ze2 + RY=E 2 2 ç ÷ 2 m R è ¶r r ¶r ø 2 mY r 4pe 0 r 2 2 r æ ¶2 2 ¶ ö Ze2 r 2 + R- Er LY = 0 2 ç ÷ 2 m R è ¶r r ¶r ø 4pe 0 2 mY 2 2 Function of just r Function of just φ and θ Particle on a sphere redux We have already encountered the angular part – this is the particle on a sphere l(l +1) LY = EY Û LY = EY Y Û EY = 2mY 2m 2m 2 2 r æ ¶2 2 ¶ ö Ze2 r 2 + R Er = - EY 2 ç ÷ 2 m R è ¶r r ¶r ø 4pe 0 2 2 r æ ¶2 2 ¶ ö Ze2 r l(l + 1) 2 + R- Er = 2 ç ÷ 2 m R è ¶r r ¶r ø 4pe 0 2m 2 2 æ ¶2 2 ¶ ö Ze2 l(l + 1) + RR+ 2 ç ÷ 2 m è ¶r r ¶r ø 4pe 0r 2 mr 2 2 2 2 R = ER 2 Radial and angular components For the radial degree of freedom, we have a new equation. æ ¶2 2 ¶ ö Ze2 l(l +1) + RR+ 2 ç ÷ 2m è ¶r r ¶r ø 4pe 0r 2 mr 2 2 This is kinetic energy in the radial motion 2 R = ER Original Coulomb potential + a new one Centrifugal force This new term partly canceling the attractive Coulomb potential can be viewed as the repulsive potential due to the centrifugal force. 2 l(l + 1) + 2 2mr V l 2 2mr 2 F The higher the angular momentum, the greater the force in the positive r direction dV dr l 2 mr 2 3 p r mr 2 3 mv r 2 The radial part Simplify the equation by scaling the variables 4pe 0 2Zr r= ; a0 = a0 m e2 2 4E me4 E ¢ = 2 ; e0 = 2 2 Z e0 32p e 0 o = 1 bohr = 0.529 A 2 = 1 Ry = 13.6 eV æ ¶2 2 ¶ ö Ze2 l(l + 1) + RR+ 2 ç ÷ 2 m è ¶r r ¶r ø 4pe 0r 2 mr 2 2 2 R = ER ¶ 2 R 2 ¶R R l(l + 1) - 2- + R = E ¢R 2 r ¶r r ¶r r The radial solutions We need a new set of orthogonal polynomials: R 2 2 2 R R The solution of this is l l ( l 1) 2 Slater-type orbital æ rö - r /2n Rnl (r) = N nl ç ÷ Lnl ( r )e è nø Normalization R E R Associated Laguerre polynomials 1 E¢ = - 2 4n The Slater-type orbital Wave functions Y ( r,q ,j ) = Rnl ( r ) Ylm (q ,j ) n = 1, 2, 3,… l = 0, 1, 2,… , n - 1 m = -l, … , l The radial solutions æZö n = 1, l = 0, Rnl = 2 ç ÷ è a0 ø 3/2 e- r /2 1 æZö n = 2, l = 0, Rnl = ç ÷ 2 2 è a0 ø 3/2 1 æZö n = 2, l = 1, Rnl = ç ÷ 4 6 è a0 ø 3/2 1 æZö n = 3, l = 0, Rnl = ç ÷ 9 3 è a0 ø 3/2 æ r ö - r /4 2 e çè ÷ 2ø re - r /4 æ r 2 ö - r /6 çè 6 - 2 r + 9 ÷ø e 1 E¢ = - 2 4n E=- Z 2 me4 32p 2e 02 2 n2 Verification Let us verify that the (n = 1, l = 0) and (n = 2, l = 1) radial solutions indeed satisfy the radial equation n = 1, l = 0 : R = Ce- r /2 n = 2, l = 1: R = C re - r /4 ¶ 2 R 2 ¶R R l(l + 1) - 2- + R = E ¢R 2 r ¶r r ¶r r 1 E¢ = - 2 4n Summary The 3-dimensional Schrödinger equation for the hydrogenic atomic structures can be solved analytically after separation of variables. The wave function is a product of the radial part involving associated Laguerre polynomials and the angular part that is the spherical harmonics. There are 3 quantum numbers n, l, and m. The discrete energy eigenvalues are negative and inversely proportional to n2.