Identical Particles ¾We would like to move from the quantum theory of hydrogen to that for the rest of the periodic table
One electron atom to multielectron atoms ¾This is complicated by the interaction of the electrons with each other and by the fact that the electrons are identical
The Schrodinger equation for the two electron atom can only be solved by using approximation methods
1 Identical Particles ¾In classical mechanics, identical particles can be identified by their positions ¾In quantum mechanics, because of the uncertainty principle, identical particles are indistinguishable
This effect is connected with the Pauli exclusion principle and is of major importance in determining the properties of atoms, nuclei, and bulk matter
2 Identical Particles
Consider two particles, then Ψ(x,t)→ Ψ(x1,x2,t) The time dependent Schrodinger equation is
() 2 2 2 2 ∂Ψ x1,x2,t ⎡ h ∂ h ∂ ⎤ ih = ⎢− 2 − 2 +V ()()x1, x2 ⎥Ψ x1,x2,t ∂t ⎣ 2m ∂x1 2m ∂x2 ⎦ The time independent Schrodinger equation is ψ 2 2 2 2 ⎡ h ∂ h ∂ ⎤ ⎢− 2 − 2 +V ()()x1, x2 ⎥ x1,x2 = Eψ x1,x2 () ⎣ 2m ∂x1 2m ∂x2 ⎦ And note here we have used labels that identify particles 1 and 2
3 Identical Particles ¾An important case is when the particles do not interact with each other
This is called the independent particle model
It’s the starting point for the He atom e.g.
Then V ()x1, x2 = V1(x1 )+V2 (x2 ) ⎡ 2 2 2 2 ⎤ h ∂ h ∂ ψ ⎢− 2 +V1()x1 − 2 +V2 ()x2 ⎥ x1 (, x2 = E )x1, x2 ( ) ⎣ 2m ∂x1 ψ2m ∂x2 ⎦ ()()()ψ This suggests we can write x1ψ, x2 = x1 x2 and E = E1 + E2 ψ Which leads to ψ 2 2 ⎡ h d ⎤ ψ ⎢− 2 +V1()x1 ⎥ x1 ()= E1 x1 () ⎣ 2m dx1 ⎦ 2 2 ψ ⎡ h d ⎤ ⎢− 2 +V2 ()x2 ⎥ x2 ()= E2ψ x2 () ⎣ 2m dx2 ⎦ 4 Identical Particles
¾ Let’s say particle 1 is in quantum state m and particle 2 is in quantum state n
ψ ()x1, x2 =ψ m (x1 )ψ n (x2 )
¾ If we interchange the two particles then
ψ ()x1, x2 =ψ m (x2 )ψ n (x1 )
¾ We get different wave functions (and probability densities) so the two particles are distinguishable
Two particles are indistinguishable if we can exchange their labels without changing a measurable quantity
Thus neither of the solutions above is satisfactory 5 Identical Particles
¾In fact thereψ are two ways to construct indistinguishableψ wave functions 1 ψ ψ = ()ψ ()()x x + x ψ ()()x s 2 m 1 ψ n 2 m 2 n 1 1 ψ ψ = ()()()x x − x ψ ()()x a 2 m 1 n 2 m 2 n 1
Ψs is a symmetric wave function under particle interchange of 1↔2
Ψs →Ψs
Ψa is a antisymmetric wave function under particle interchange of 1↔2
Ψa → -Ψa The probability density remains unchanged under particle interchange of 1↔2 6 Identical Particles ¾All particles with integer spin are called bosons
Spin 0,1,2,…
Photon, pions, Z-boson, Higgs ¾All particles with half integer spin are called fermions
Spin 1/2, 3/2, …
Electron, proton, neutron, quarks, … ¾For the next few lectures we’ll focus on the fermions (electrons)
7 Identical Particles ¾The wave function of a multi-particle system
of identical fermions is antisymmetric under interchange of any two fermions
of identical bosons is symmetric under interchange of any two bosons ¾The Pauli exclusion principle follows from these principles
No two identicalψ electrons (fermions) can occupy ψ the same quantum state 1 ψ ψ a = ()m ()()x1 n x2 − m x2 ψ ()()n x1 2 ψ for m = n (same quantumψ state) 1 ψ ψ = ()()x x ()− x ψ ()x = 0 () a 2 m 1 m 2 m 2 m 1 8 Identical Particles ¾What about 3 particles? ¾Symmetric ()ψ = ψ ()x ψ (x )ψ (x )+ψ (x )ψ (x )()ψ x +ψ (x )ψ (x )ψ (x ) s m 1 ψ n 2 o 3 o 1 m 2 n 3 n 1 o 2 m 3 ()() () () ψ s = m x1 n x2 ψ o x3 + permutations
¾Antisymmetricψ
Use the Slater determinantψ ψ ψ m (1) ψ m (2) m (3) ψ1 ψ ψ = det()ψ 1 ( )2 ψ ()3 a 3! ()n ψ (ψ n )n () ψ o 1 o 2ψ ψ o 3 ψ ψ 1 ψ ψ = (ψ ()1 2 (ψ )3 − ()1 3 ()2 () ( ) a 6 m ψn o ψ m n o ()ψ () ()ψ () () () + 2 3 1 −ψ 2 1ψ 3 m ()n ()o ()m ψ n ()o () () + m 3 n 1 o 2 − m 3 n 2 ψ o 1 ) 9 Identical Particles ¾Just a reminder, we are presently only working with the space wave functions
We’ll get to spin in a little bit ¾A consequence of identical particles is called exchange “forces”
Symmetric space wave functions behave as if the particles attract one another
Antisymmetric wave functions behave as if the particles repel one another
10 Infinite Square Well ¾Quick review. For an infinite well at x=0 and x=L 2 n x Solutions are (x) = sin ψ n L L π 2 2 π E = n2 h 2mL2
11 Identical Particles ¾Let’s return to the infinite well problem only now with two particles
Case 1 distinguishable particles ψ ()x , x =ψ (x )ψ (x ) 1 2 m ψ1 n 2 ψ Case 2 identical particles (symmetric) 1 ψ ψ ()x , x = ()()()x x + x ψ ()()x 1 2 2 ψm 1 n 2 m 2 n 1 Case 3 identical particles (antisymmetric)ψ 1 ψ ψ ()x , x = ()()x x ()− x ψ ()x () 1 2 2 m 1 n 2 m 2 n 1
12 Identical Particles ¾What is the probability that both particles will be on the left side of the well?
LL/ 2 / 2 2 P = ψ ()x , x dx dx ∫∫ 1 2 1 2 ψ 0 0 ¾Case 1 ψ L / 2 2 L / 2 2 P = ()x dx ()x dx ∫ m 1 1 π∫ n 2 2 0 0 2 2 L / 2 sin 2 m x L / 2 sin 2 nπx P = ∫ dx ∫ dx L L 0 L 0 L 4 L L 1 P = 2 = L 4 4 4 13 Identical Particles
ψ¾ Case 2 and 3 L / 2 ψ 1 P = []2 ()x 2 x ()+ 2 x ()2 x ± 2ψ ()x ψ x ψ ()()x ψ x dx dx ()() ∫ m 1 n ψ 2 m 2 n 1 m 1 n 2 m 2 n 1 1 2 2 0 ψ 1 ⎡1 1 LL/ 2 / 2 ⎤ P = + ±ψ ()x x ()dx x ()x dx () ⎢ ∫∫m ψ1 n 1 1 m 2 n 2 2 ⎥ 2 ⎣4 4 0 0 ⎦ 2 ψ 1 ⎛ L / 2ψ ⎞ ψ P = ± ⎜ ()()x ψ x dx ⎟ ⎜ ∫ m 2 n 2 2 ⎟ 4 ⎝ 0 ⎠ 1 P = ± K where K > 0 4 ¾ For a symmetric wave function (+) the particles are more likely on the same side (attracted) ¾ For the antisymmetric wave function (-) the particles are more likely on opposite sides (repel) 14 Identical Particles ¾The wave function of a multi-particle system
of identical fermions is antisymmetric under interchange of any two fermions
of identical bosons is symmetric under interchange of any two bosons ¾The Pauli exclusion principle follows from these principles
No two identicalψ electrons (fermions) can occupy ψ the same quantum state 1 ψ ψ a = ()m ()()x1 n x2 − m x2 ψ ()()n x1 2 ψ for m = n (same quantumψ state) 1 ψ ψ = ()()x x ()− x ψ ()x = 0 () a 2 m 1 m 2 m 2 m 1 15 Periodic Table ¾The Pauli exclusion principle is the basis of the periodic table
This is why all the electron’s don’t simply fall into the ground state – because they are fermions
Recall there were 4 quantum numbers that specified the complete hydrogen wave
function: n, l, ml, and ms No two electrons in the same atom can have these same quantum numbers
16 Periodic Table ¾Building the periodic table
Principle quantum number n forms shells
Orbital angular momentum quantum number l forms subshells l=0,1,2,3,… are called s,p,d,f,…
Each ml can hold two electrons, one spin up (ms=1/2) and one spin down (ms=-1/2) The electrons tend to occupy the lowest energy level possible
Electrons obey the Pauli exclusion principle
17 Periodic Table ¾Energy levels Note for multielectron atoms, states of the same n and different l are no longer degenerate This is because of screening effects Referring back to the radial probability distributions, because the s states have non-zero probability of being close to the nucleus, their Coulomb potential energy is lower
18 Ionization Potential
19 Periodic Table ¾Hydrogen (H) 1 1s ¾Helium (He) 2 1s – closed shell and chemically inert ¾Lithium (Li) 2 1s 2s – valence +1, low I, partially screened, chemically very active ¾Beryllium (Be) 2 2 1s 2s – Closed subshell but the 2s electrons can extend far from the nucleus
20 Periodic Table ¾Boron (B) 2 2 1 1s 2s 2p – Smaller I than Be because of screening ¾Carbon (C) 2 2 2 1s 2s 2p – I actually increases because the electrons can spread out in 2/3 l state lobes The valence is +4 since an energetically favorable configuration is 1s22s12p3 ¾Nitrogen (N) 2 2 3 1s 2s 2p – See comments for C. Electrons spread out in 3/3 l state lobes ¾Oxygen (O) 2 2 4 1s 2s 2p – Two of the l state electrons are “paired” Electron-electron repulsion lowers I 21 Periodic Table ¾Fluorine (F) 2 2 5 1s 2s 2p – Very chemically active because it can accept an electron to become a closed shell ¾Neon (Ne) 2 2 6 1s 2s 2p –Like He
22 Periodic Table
23 Periodic Table ¾Periodic table is arranged into groups and periods ¾Groups Have similar shell structure hence have similar chemical and physical properties Examples are alkalis, alkali earths, halogens, inert gases ¾Periods Correspond to filling d and f subshells Examples are transition metals (3d,4d,5d), lanthanide (4f), and actinide (5f) series Because there are many unpaired electrons, spin is important for these elements and there are
large magnetic effects 24