MTLE-6120: Advanced Electronic Properties of Materials Atoms, many - - PowerPoint PPT Presentation

mtle 6120 advanced electronic properties of materials
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MTLE-6120: Advanced Electronic Properties of Materials Atoms, many - - PowerPoint PPT Presentation

1 MTLE-6120: Advanced Electronic Properties of Materials Atoms, many electron theories and the periodic table Contents: Hydrogen atom: quantum numbers and orbitals Many-electron systems and the density-functional (DFT) perspective


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MTLE-6120: Advanced Electronic Properties of Materials Atoms, many electron theories and the periodic table

Contents:

◮ Hydrogen atom: quantum numbers and orbitals ◮ Many-electron systems and the density-functional (DFT) perspective ◮ Electronic configuration examples

Reading:

◮ Kasap: 3.7 - 3.8

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Hydrogenic atom

◮ Single electron with a nucleus of charge +Ze, where Z is the atomic

number

◮ Z = 1 is hydrogen, Z = 2 is a He+ ion, Z = 3 is Li2+ etc. ◮ Schrodinger equation

−2∇2ψ( r) 2m − Ze2 4πǫ0rψ( r) = Eψ( r) separable in spherical coordinates resulting in eigenfunctions ψnlm( r) = Rnl(r)Ylm(θ, φ) and eigen-energies Enlm = − me4 32π2ǫ2

02 · Z2

n2 = −Z2 2n2 Eh = −Z2 n2 Ryd ≈ −Z2 n2 (13.6 eV)

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Atomic quantum numbers

◮ For the box, we has nx, ny and nz ◮ Now in spherical coordinates, so correspond to r, θ and φ ◮ Principal quantum number n = 1, 2, . . . is for the radial r direction ◮ Angular quantum number l = 0, 1, 2, . . . , n − 1 is for the θ direction ◮ Azimuthal quantum number ml = −l, −l + 1, . . . , +l is for the φ direction ◮ But energy Enlml ∝ n−2 only depends on n ◮ States of various l and ml at same n are ‘degenerate’ i.e. have same energy

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Radial wavefunctions

◮ Radial functions of the form

Rnl(r) ∝ exp −Zr na0

  • · rl · p(l)

n−l−1(r)

where a0 = 4πǫ02/(me2) ≈ 0.529 ˚ A is the Bohr radius

◮ Typical radial extent ∼ na0/Z ◮ Polynomial degree n − l − 1: first n of given l

has no nodes, next has one node etc.

◮ Remember l = 0, 1, 2, 3 denoted by s, p, d, f ◮ 1s has no nodes, 2s has 1 node etc. ◮ 2p has no nodes, 3p has 1 node etc.

1s 2s 3s 2p 3p

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Angular wavefunctions

◮ Spherical harmonics Ylml(θ, φ) = P ml l

(cos θ)eimlφ

◮ Characteristic orbital shapes used in chemistry (typically ReYlm and ImYlm) ◮ l controls number of lobes ◮ ml controls number in xy-plane ◮ All ml related by spherical symmetry

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Electronic configuration of atoms

◮ Pauli exclusion principle: one electron per state (Fermi-Dirac statistics) ◮ Spin: ms = ±1/2 (2 states) ◮ Azimuthal: m = −l, −l + 1, . . . , +l (2l + 1 states) ◮ Per n and l: 2(2l + 1) states ◮ Periodic table by orbital being filled (Z range):

1s (1-2) 2s (3-4) 2p (5-10) 3s (11-12) 3p (13-18) 4s (19-20) 3d (21-30) 4p (31-36) 5s (37-38) 4d (39-48) 5p (49-54) 6s (55-56) 4f (57-70) 5d (71-80) 7p (81-86) 7s (87-88) 5f (89-102)

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The size of atoms

◮ Orbital size ∼ na0/Z ◮ Hydrogen atom Z = 1, n = 1: size ∼ a0 ≈ 0.53 ˚

A

◮ Sodium atom Z = 11, n = 3: size ∼ 3a0/11 ≈ 0.14 ˚

A

◮ Platinum atom Z = 78, n = 6: size ∼ 6a0/78 ≈ 0.04 ˚

A

◮ What’s wrong? ◮ Hydrogenic orbitals are for one electron systems only! ◮ When more than one electron, electron-electron repulsion matters ◮ Effective charge seen by outer electrons is approximately that of nucleus +

inner electrons

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Many-electron Schrodinger equation

◮ So far, we discussed wavefunction ψ(

r) satisfying − 2 2m∇2ψ + V ( r)ψ = Eψ which is strictly a one-electron theory only.

◮ For N electrons, need to keep track of all N electronic coordinates with a

wavefunction ψ( r1, r2, . . . , rN)

◮ Corresponding Schrodinger equation with e-e interactions:

− 2 2m

  • i

∇2

  • riψ
  • Kinetic

+

  • i

V ( ri)ψ

  • e-nuc

+

  • i=j

e2 4πǫ0| ri − rj|ψ

  • e-e

= Eψ which is impossible to solve exactly beyond special N = 2 cases

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Many-electron non-interacting case

◮ Without e-e interactions:

− 2 2m

  • i

∇2

  • riψ
  • Kinetic

+

  • i

V ( ri)ψ

  • e-nuc

= Eψ which is separable in each ri.

◮ Therefore solution must be consist of products

ψ( r1, r2, . . . , rN) ∼ φ1( r1)φ2( r2) · · · φN( rN)

◮ Each ‘orbital’ φi: N = 1 Schrodinger equation with orbital energy εi ◮ Total energy E = i εi ◮ Strictly, fermionic wavefunctions need to be antisymmetric

⇒ ψ = det[φi( rj)] (Slater determinant)

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Kohn-Sham density functional theory (DFT)

◮ A single-particle theory

− 2 2m∇2φi( r) + VKS( r)ψ = εiφi( r) in an effective potential VKS( r)

◮ VKS(

r) = V ( r) + contribution from electron density n( r)

◮ Total energy E = i εi + contribution from electron density n(

r)

◮ Electron density n(

r) =

i |φi(

r)|2 made self-consistent

◮ DFT works surpisingly well even for strongly interacting electrons ◮ When DFT does not work, material called ‘strongly-correlated’!

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Atoms revisited

◮ Orbital energies are those from effective potential (not hydrogenic) ◮ For spherical atoms, still degenerate in m and ms, but not in l ◮ At same n, energy increases with l ◮ In particular, energy of (n + 1)s < (n − 1)f < nd < (n + 1)p ⇒

1s (1-2) 2s (3-4) 2p (5-10) 3s (11-12) 3p (13-18) 4s (19-20) 3d (21-30) 4p (31-36) 5s (37-38) 4d (39-48) 5p (49-54) 6s (55-56) 4f (57-70) 5d (71-80) 7p (81-86) 7s (87-88) 5f (89-102)

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Electronic configuration example: Sc

Z = 21, Configuration: 1s2 2s2 2p6 3s2 3p6 4s2 3d1

1s 2s 2p 3s 3p 4s 3d

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Electronic configuration example: V

Z = 23, Configuration: 1s2 2s2 2p6 3s2 3p6 4s2 3d3

1s 2s 2p 3s 3p 4s 3d

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Electronic configuration example: Cr

Z = 24, Configuration: 1s2 2s2 2p6 3s2 3p6 3d5 4s1

1s 2s 2p 3s 3p 4s 3d 3d

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Electronic configuration example: Ni

Z = 28, Configuration: 1s2 2s2 2p6 3s2 3p6 3d8 4s2

1s 2s 2p 3s 3p 4s 3d

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Electronic configuration example: Cu

Z = 29, Configuration: 1s2 2s2 2p6 3s2 3p6 3d10 4s1

1s 2s 2p 3s 3p 3d 4s

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