physical chemistry ii quantum chemistry lecture 18 many
play

Physical Chemistry II: Quantum Chemistry Lecture 18:Many-electron - PowerPoint PPT Presentation

Physical Chemistry II: Quantum Chemistry Lecture 18:Many-electron Atoms & Atomic Term Symbols Yuan-Chung Cheng yuanchung@ntu.edu.tw 5/7/2019 Courtesy of Prof. Jerry Chen He: Two-Electron Atom - Attraction Repulsion 2+ - He:


  1. Physical Chemistry II: Quantum Chemistry Lecture 18:Many-electron Atoms & Atomic Term Symbols Yuan-Chung Cheng yuanchung@ntu.edu.tw 5/7/2019 Courtesy of Prof. Jerry Chen

  2. He: Two-Electron Atom - Attraction Repulsion 2+ -

  3. He: Two-Electron Atom - Z eff Attraction Repulsion 2+ 1 < Z eff < 2 - Z eff : Effective Nuclear Charge By the variation method, Z eff is calculated as 1.69

  4. Atomic Orbitals for Many-Electron Atoms ˆ Y = Y H E No analytical solutions even for He because of electron repulsion He and Li atoms can be handled by variation methods Need more practical approach for other atoms!

  5. Hartree-Fock Self-Consistent Field Method Single-electron wavefunction: ψ i (x 1 ): atomic spin orbital x 1 : electron variable m ∑ ψ 1 s ( r ) = c a N a e − Z a r / a 0 Example for 1 s : a = 1 linear combination of basis functions ψ 1 with variational parameters N-electron wavefunction: Slater determinants ψ 2 ψ 1 (x 1 ) ψ 2 (x 1 ) ψ N (x 1 )  ψ 3 ψ 1 (x 2 ) ψ 2 (x 2 ) ψ 2 (x 2 )  1 Ψ (x 1 ,...,x N ) =    N ! ψ 1 (x N ) ψ 2 (x N )  ψ N (x N )

  6. Mean-Field Approximation Many-electron Hamiltonian: N − 1 H = −  2 Ze 2 e 2 N N N ∑ ∑ ∑ ∑ ˆ ∇ i − + 2 2 m e r r i = 1 i = 1 i = 1 j = i + 1 i ij Many-electron Integrals: e 2 e 2 N N ∑ ∑ ψ 1 ψ 2  ψ j  ψ 1 ψ 2  ψ j  = ψ 1 ψ j ψ 1 ψ j r r j = 2 j = 2 1 j 1 j e 2 N ∑ ∫∫ = | ψ 1 | 2 | ψ j | 2 d τ 1 d τ 2 r A Slater determinant, j = 2 1 j product of spin orbitals e 2 | ψ j | 2 ⎧ ⎫ ⎪ ⎪ N ∑ ∫ ∫ = | ψ 1 | 2 d τ 2 d τ 1 ⎨ ⎬ ⎪ ⎪ r ⎩ ⎭ j = 2 1 j Mean-field term due to averaged distribution of all other electrons

  7. Mean-Field Approximation Hartree-Fock Mean-field Hamiltonian: H = −  2 Ze 2 N N N N + 1 ∑ ∑ ∑ ∑ ˆ ˆ ∇ i − ≡ 2 V i ( r i ) h i 2 m e r 2 i = 1 i = 1 i = 1 i = 1 i e 2 | ψ j | 2 N ∑ ∫ i ) = d τ j where V i ( r r j ≠ i ij • Single determinantal wavefunction leads naturally to the mean-field approximation • The approximation allows a factorization of the Hamiltonian into N single-electron problems • Given a basis, the theory provides a variational groundstate & optimal atomic orbitals within the single determinant approximation è mean-field, no electron correlations • N single-electron Schrodinger equations are interdependent è requires solving self-consistently via an iterative procedure

  8. Many-electron Model Hartree-Fock ˆ Y = Y (Self-consistent H E field, SCF) Method

  9. Atomic Orbitals for Many-Electron Atoms The concept of The use of “orbital” is just a orbital is exact good approximation

  10. Na Radial Distribution Function for “Valance” Orbitals r 2 R ( r ) 2 “Core” electrons: screening/shielding effect < < Penetration effect E E E of the 3s and 3p orbitals 3 s 3 p 3 d Increase screening

  11. Hund’s Rule For degenerate orbitals, electrons occupy them one at a time. Less likely p x p y p z Likely p x p y p z

  12. Hund’s Rule Smaller electrostatic repulsion? The electron-electron repulsion does not allow the two electrons getting too close to each other. However, this explanation is now obsolete. Likely p x p y p z

  13. Hund’s Rule “Exchange energy” makes the triplet configuration more stable Different spins: two electrons do not exchange p x p y p z Same spin: two electrons can exchange p x p y p z

  14. Hund’s Rule Larger electron-nucleus interaction due to less screening when two different orbitals are occupied! Less likely p x p y p z Likely p x p y p z Proven by exact QM calculations, see Levine.

  15. Atomic Energy States 2 2 2 C : 1 s 2 s 2 p “Electron configuration” along does not fully specify the “state” of a many-electron system. These three arrangements (states) have different energies when electron-electron repulsions are included! Depending on total angular momentum!

  16. Atomic Energy States -- Terms The energy of a many-electron state depends on the total orbital angular momentum and total spin angular momentum of the state. L = ˆ ˆ L 1 + ˆ L 2 + ˆ L 3 + … S = ˆ ˆ S 1 + ˆ S 2 + ˆ S 3 + … Notations: L : quantum number for total orbital angular momentum l 1 , l 2 ,…: orbital angular momentum quantum numbers for each individual electrons S : quantum number for total spin angular momentum s 1 , s 2 ,…: spin angular momentum for each electrons L & S are determined by vector addition/subtraction rules.

  17. Example: two electrons in p p 2 ( l 1 = 1, l 2 = 1): L = 2,1, 0 L = 2 = D 1 = P = 0 S = + + - - ! L l l , l l 1 , , l l 1 2 1 2 1 2 2 0

  18. Example: two electrons in p p 2 ( l 1 = 1, l 2 = 1): L = 2,1, 0 L = 2 = D 1 = P = 0 S p 2 f 1 ( l 1 = 1, l 2 = 1, l 3 = 3) L=5, 4, 3, 2, 1, …

  19. Addition of Three Angular Momenta two at a time… ¢ = + + - - L l l , l l 1 , ! , l l Adding the first two: 1 2 1 2 1 2 ¢ ¢ ¢ = + + - - L L l , L l 1 , ! , L l Then add the third one: 3 3 3 = + + L l l l z z 1 z 2 z 3 If all l are equal, the minimum is zero, if one L’ l is larger than the others, the minimum is that given by - - l l l 1 2 3 ( vector sum of all vectors ).

  20. Addition of Three Angular Momenta p 2 f 1 ( l 1 = 1, l 2 = 1, l 3 = 3) L' = 2, 1, 0 L = 5, 4, 3, 2, 1 L = 4, 3, 2 L = 3 Degeneracy = 2L + 1

  21. Addition of Three Angular Momenta Degeneracy 2L+1 Number of microstates: p 2 f 1 ( l 1 = 1, l 2 = 1, l 3 = 3) L = 5, 4, 3, 2, 1 2 × 5+1 = 11 2 × 4+1 = 9 2 × 3+1 = 7 2 × 2+1 = 5 2 × 1+1 = 3 35

  22. Addition of Three Angular Momenta Degeneracy 2L+1 Number of microstates: p 2 f 1 ( l 1 = 1, l 2 = 1, l 3 = 3) L = 4, 3, 2 2 × 4+1 = 9 2 × 3+1 = 7 2 × 2+1 = 5 21

  23. Addition of Three Angular Momenta Degeneracy 2L+1 Number of microstates: p 2 f 1 ( l 1 = 1 , l 2 = 1 , l 3 = 3 ) L = 5, 4, 3, 2, 1 35 L = 4, 3, 2 21 L = 3 7 63 3 × 3 × 7

  24. Total spin angular momentum S for n electrons: S = n /2, n /2–1, n /2–2,…, 0, for n even S = n /2, n /2–1, n /2–2,…., 1/2, for n odd Spin multiplicity = 2S+1 S=0, 2S+1=1, singlet, m s = 0 S=1/2, 2S+1=2, doublet, m s = ½, -½ S=1, 2S+1=3, triplet, m s = 1, 0, -1

  25. Total spin angular momentum S for n electrons: S = n /2, n /2–1, n /2–2,…, 0, for n even S = n /2, n /2–1, n /2–2,…., 1/2, for n odd 2 2 p Spin multiplicity = 2S+1 singlet, m s = 0 S=0 triplet, m s = 1, 0, -1 S=1 singlet, m s = 0 S=0

  26. Hund’s Rule of Maximum Multiplicity Hund's first rule states that the lowest energy atomic state is the one which maximizes the total multiplicity for all of the electrons in the open sub-shell. http://en.wikipedia.org/wiki/List_of_Hund%27s_rules

  27. Russell-Saunders/L-S Term Symbol Total orbital angular momentum L Total spin angular momentum S Total angular momentum J (couple L & S) 2S+1 L J J = L+S, L+S-1,…. | L-S | 2 S Double s one-half 1 / 2 Designation: L =0, 1, 2, 3, 4, 5…. S, P, D, F, G, H…. L-S Terms determine energy levels of atomic electronic states for atoms with small spin-orbital coupling (L-S coupling), i.e. not for heavy atoms.

  28. Example 1: a single electron 1s 1 2S+1 L J 2 S 1 2

  29. 2S+1 L J Hydrogen atom (single electron) Ground state vs. Excited States 2 P 2 S 3 / 2 1 / 2 2s 2p 2 P 1 / 2 spin-orbit interaction Energy 1s 2 S 1 / 2

  30. 2S+1 L J Fine structure of the sodium D line Energy

  31. Many-electron Atoms For many-electron system, one may derive the electronic states from the M L , M S , and M J values. = å ( ) = ± ± ± M m 0 , 1 , 2 ,.... L L l i i = å ( ) = ± ± ± M m 0 , 1 , 2 ,.... S S s i i = + = ± ± ± M M M 0 , 1 , 2 ,.... J J L S These magnetic quantum numbers are easy to determine from electronic configurations à we can then derive ( L , S , J ) from the intervals!

  32. Example 2 1s 2 For any filled shell, we just have the state with L = S = J = 0 1 S 0 No need to consider “closed shells”

  33. Term Symbols & Electronic Configurations To determine all term symbols in a configuration: 1. List all electronic microstates by filling orbitals with spin specified 2. Calculate M L and M S , then tabulate the number of states belonging to each (M L , M S ) 3. Divide states into separate terms based on the bounds of M L and M S (starting from largest L) 4. Determine term symbols Core shells are fully occupied and do not give rise to additional states à only open shell electrons need to be considered.

  34. 2S+1 L J Example 3 Totally 2x2 = 4 states 4 microstates! 1s 1 2s 1 3 S 1 S 1 0 1 S 0 + 3 S 1

  35. Example 4 Carbon: 1s 2 2s 2 2p 2 Number of possible arrangement is Ignored 6 ! = 15 microstates 2 ! 4 ! 2p 2 M C n Number of spin orbitals Number of electrons p 2 ( l 1 = 1, l 2 = 1): L = 2,1, 0

  36. Carbon: 2p 2

  37. Carbon: 2p 2 While M L = -2…2, M S =0 à L=2, S=0 Must have a 1 D We have identified 5 microstates, let’s remove them from the table – substrate 1 from the column M S =0.

  38. Carbon: 2p 2 While M L = -1…1, M S = -1…1 à L=1, S=1 1 2 1 Must have a 3 P

  39. Carbon: 2p 2 While M L = 0, M S = 0 à L=0, S=0 1 Must have a 1 S too!! GOTCHA!!

Download Presentation
Download Policy: The content available on the website is offered to you 'AS IS' for your personal information and use only. It cannot be commercialized, licensed, or distributed on other websites without prior consent from the author. To download a presentation, simply click this link. If you encounter any difficulties during the download process, it's possible that the publisher has removed the file from their server.

Recommend


More recommend