1 Hydrogen Atom The simplest system: p + e Schroedinger equation can be solved exactly Spherical symmetry Potential energy between p + e r e V 0 2 4πε −= 2 Polar Coordinates Ψ(x,y,z) → Ψ(r,θ, φ) x = ? y = ? z = r cos q Take advantage of spherical symmetry 3 Radial and Angular Part Ψn, l, m (r,θ, φ) = N × Rn, l (r) × χl, m(θ, φ) Separation of variables Rn, l (r) = radial part of the wave function, depends only on distance from a nucleus - r χl, m(θ, φ) = angular (angles) part of the wave function, depends only on direction - θ, φ N = normalisation constant In order to be ∫| Ψ |2 dV = +1 Normalisation condition - electron is definitely somewhere with probability = 1 4 Quantum Numbers Principal quantum number n, (1 to ∞) Angular momentum quantum number l, (0 to n −1) l = 0 (s), 1 (p), 2 (d), 3 (f), 4 (g), 5 (h), ........ Magnetic quantum number ml, (+ l, .....0, ..... −l) For each l there is (2l + 1) values of ml Magnetic spin quantum number ms (±½) Rn, l (r) depends on quantum numbers n and l χl, m(θ, φ) depends on quantum numbers l and ml 5 Wave Functions of H atom • solution of Schrödinger equation • complex function of coordinates x, y, z or better r, φ, θ • no physical meaning • positive and negative values • | Ψ |2 probability density of finding electron e 6 Radial Part of the Wave Function of H Atom 1 (p) 1 (p) 0 (s) l ±1 0 0 ml 2 (Z/2a0) 3/2 (1 − Zr/2a0) exp(− Zr/2a0)2 (L) 2/√3 (Z/2a0) 3/2 (Zr/2a0) exp(− Zr/2a0)2 (L) 2 (Z/a0) 3/2 exp(− Zr/a0)1 (K) Rn, l (r)n 7 Electron Energy in H-type Atoms μ = reduced mass of nucleus-electron e = elementary charge, ε0 = permitivity of vacuum Z – the higher a nucleus charge the stronger is an electron bound, the lower energy has, one-electron ions (He+, Li2+,....) n – the higher a principal number the less stable e is Corresponds to Bohr’s eq.!! 2 2 22 0 4 8 n Z h eN E A n ε μ −= 2 2 0 n Z EEn −= 8 Electron Energy in H-type Atoms E1 = −13.6 eV (13.6 eV = 1 Ry) Energy depend ONLY on n E2 = ? 2 2 22 0 4 8 n Z h eN E A n ε μ −= 9 Principal Quantum Number n Gives the levels energy Higher n has higher energy less stable n same as in the Bohr’s model Attains values 1 to ∞ For each n there is n2 of degenerate levels Σ (2l + 1) = n2 l = 0 l = n − 1 10 Orbital Angular Momentum L = Orbital angular momentum (vector) L = m × v × r = p × r ( )1+= llL h Describes movements of electrons in orbitals L 11 Angular Momentum Quantum Number l l orbital 0 s 1 p 2 d 3 f 4 g 5 h 6 i 7 j 8 k L = Orbital angular momentum L = m × v × r Type of orbital, (0 to n −1) these orbitals are not filled by electrons in atoms in ground state ( )1+= llL h 12 Magnetic Quantum Number ml l orbital ml 0 s 0 1 p 1, 0, −1 2 d 2, 1, 0, −1, −2 3 f 3, 2, 1, 0, −1, −2, −3 4 g 5 h 6 i π2 h mmL llz == h these orbitals are not filled by electrons in atoms in ground state 13 Quantization of Orbital Angular Momentum ( )1+= llL h π2 h mmL llz == h 14 1sn = 1 543210l = hgfdps 2p2sn = 2 n = 6 n = 5 n = 4 n = 3 6s 5s 4s 3s 6h6g6f6d6p 5g5f5d5p 4f4d4p 3d3p For each n there is n2 of degenerate levels 15 Magnetic Spin Quantum Number ms Stern-Gerlach experiment S = h/2π [s (s +1)]½ s = ½ SZ = ms h/2π S = spin momentum vacuum Inhomogeneous magnetic field Furnace with Ag 16 Magnetic Spin Quantum Number ms S = h/2π [s (s +1)]½ s = ½ SZ = ms h/2π ms = ±½ 17 Ψ = Wave Functions Ψ = solution of Schrödinger equation | Ψ |2 = probability density of e | Ψ |2 dV = probability density of finding electron e in volume dV = distribution of electron density 1 s 18 Probability Density Polar coordinates Rn, l (r) radial function dV = 4πr2 dr (spherical layer of thickness dr) Radial distribution function P = 4πr2 | Ψ |2 dr = 4πr2 R2 n, l (r) dr P = probability density of finding electron e in volume of spherical layer of thickness dr In a distance r 19 Wave Functions Probability density Radial distribution function Orbital Sign change Zero values 20 Orbitals Position of electrons cannot be established – Heisenberg’s principle – only probability Radial function – probability of finding e in a direction away from nucleus (to r = ∞) and number of nodes = zero values of radial distribution function Angular function = shape of orbitals (number of nodal planes) 21 s - Orbitals Rn, l (r) = Radial function, depends on r only χl, m(θ, φ) = angular function, is a constant for sorbitals (l = 0) = SPHERICAL SHAPE 22 Atomic Orbital 1s Rn, l (r) n = 1, l = 0 Wave Function 1s 23 Radial Distribution Function Rn, l (r) = Radial function of H atom 4πr2 R2 n, l (r) = Radial distribution function rmax = the most probable radius for 1s rmax = a0 Bohr’s radius 4πr2 R2 n, l (r) 24 4πr2R2 n,l(r)=Radialdistributionfunction 25 26 Nodes Number of nodes = n − l −1 • Wavefunction changes sign • Radial distribution function has zero value 27 Effect of Z Radial Function s With increasing nucleus charge the maximum of radial distribution function approaches closer to the nucleus ⎟⎟ ⎠ ⎞ ⎜⎜ ⎝ ⎛ −⎟⎟ ⎠ ⎞ ⎜⎜ ⎝ ⎛ = 0 3 0 ln, exp2(r)R a Zr a Z Radial distribution function 1s 28 4πr2 (Rnl)2 29 Angular Wave Function Angular wave function gives the shape of orbitals The same for all values of n 30 p - Orbitals x y z pz py px n = 2, l = 1, m = 1,0,−1 31 n = 2, l = 1, m = 0 n = 3, l = 1, m = 0 2p - orbitals 3p - orbitals 32 33 2p - orbitals 3p - orbitals Wave Function = Radial × Angular + − + + − − 34 Angular Wave Function of d-Orbitals 35 d - Orbitals dZ2 dX2-Y2 dXY dXZ dYZ 36 d - Orbitals x y z dZ2 x y z dYZ x y dX2-Y2 x y dXY 37 f - Orbitals 38 Nodes Spherical nodes = n − l −1 for s, p, d, f,.... Radial wave function Nodal planes Angular wave function: Orbital no. s 0 p 1 d 2 f 3 . . . . Only s-orbitals have non-zero value of wave function at the nucleus 39 Energy of H-Atom Orbitals Energetically degenerate levels n 2 2 22 0 4 8 n Z h eN E A n ε μ −= Energy depends only on n 40 Energy Levels in Many-Electron Atoms No degeneration Energies depend on n and l 41 Energy Levels in Many-Electron Atoms More stable orbital has a lower energy Madelung’s Rule (up to Ca) 1. Lower for (n + l) 2. When n + l same lower n 3p 4s 4p 3d 42 Many-Electron Atoms Penetration and Screeneing 2s and 2p penetrate 1s 2s penetrate more than 2p E(2s) < E(2p) but maxima r(2s) > r(2p) 1s 2p 2s 43 Relative Energies of s, p, d Orbitals E(3s) < E(3p) < E(3d) r(3s) > r(3p) > r(3d) 44 Slater’s Orbitals Orbitals for many-electron atoms - approximate • orbitals (wave functions) of hydrogen type • angular part: same as for H • radial part: R (r) = N r n*−1 exp(− Z* r/n*) Z* = A charge acting on an electron = Nucleus charge (Z+) – charge of other electrons n* = effective quant. number (for K, L, M = n) Ei = − N (Z*i /ni) N = 1313 kJ mol −1 45 Efective Nucleus Charge Z* = Z − σ σ = screening constant, sum for all electrons (1s)(2s,2p)(3s,3p)(3d)(4s,4p)(4d)(4f)(5s,5p)(5d)(5f)... Slater’s rules e on the right does not screen, no contribution to σ Within a group screens 0.35 (1s only 0.30) n − 1 (s,p) screens 0.85 n − 2 and lower screens 1.00 If an electron is in d or f, all on the left screens 1.00 46 Efective Nucleus Charge Z* = Efective Nucleus Charge Z* = Z − σ A charge acting on an electron = Nucleus charge (Z+) – charge of other electrons K (1s)2(2s,2p)8(3s,3p)8(3d)1 σ(3d) = 0 x (0.35) + 8 x 1.00 + 10 x 1.00 = 18 Z* = 19 − 18 = 1 K (1s)2(2s,2p)8(3s,3p)8 (4s)1 σ(4s) = 0 x (0.35) + 8 x 0.85 + 10 x 1.00 = 16.8 Z* = 19 − 16.8 = 2.2 47 0 2 4 6 8 10 12 14 16 H He Li Be Be C N O F Ne Na Mg Al Si P S Cl Ar K Ca Sc Ti V Cr Mn Fe Co Ni Cu Zn Ga Ge As Se Br Kr Efective Nucleus Charge Efective charge Z* He (1s)2 σ(1s) = 1 x (0.30) = 0.30 Z* = 2 − 0.30 = 1.70 48 Efective charge Z* 1s electrons are not screened Other electrons are screened 49 Radius of maximum electron density r(2s) > r(2p) r(3s) ~ r(3p) 50 Energies of 2s and 2p Orbitals Closer for light elements 51 Electron Configurations of Ground State Atoms Aufbau Principle: Electron levels are filled by electrons in the order of increasing energy, to maintain the lowest atom energy Pauli Principle: Two electrons cannot have all 4 quantum numbers the same Hund’s Rule: In degenerate orbitals, the state with maximum unpaired electrons is the most stable 52 53 Electron Configurations of C 54 Electron Configurations of Valence Shell (Ne) 55 Orbital energy Placing electrons in orbitals can change order of energy levels Starting at Sc, 3d orbitals have lower energy than 4s 56 4s 57 58 Electron Configurations of Valence Shell (Ar) 59 Ionisation Energies