The ground state of helium

7.2 The ground state of helium

Our task: To calculate the ground–state energy by using the Variational Principle experimental ev 975 . 78 − = g E Theoretically reproduce the value : Figure 7.2:the helium atom 2 r 1 2 r r − e − e − 2 r 2e + The Hamiltonian for the helium atom system ignoring fine structure and small correction is 2 2 2 2 1 2 1 2 1 2 2 2 1 2 4 e H m r r r r πε = − ∇ + ∇ − + − − 2 1 2 1 4 e e e V r r π ε = − Let 1 2 2 1 2 100 1 100 2 3 8 , r r a r r r r e a π − + Ψ ≡ Ψ Ψ = Consequently ,the energy that goes with this simplified If we ignore the electron-electron repulsion is, the ground-state wave function is just ee V where is hydrogen-like wave function with . 100 Ψ 2 = Z picture is see Chapter 5 . 1 8 109 ev E = − 1 8 ee H E V Ψ = + Ψ In the following we will apply the variational principle , using the as the trial wave function. The eigenfunction of Hamiltonian is: Ψ Thus 1 8 ee H E V = + where 1 2 2 4 2 3 3 1 2 3 1 2 8 4 r r a ee e e V d r d r a r r πε π − + = − To get the above integral value conveniently, we do the 2 r integral first and orient the coordinate system so that the polar axis lies along see Figure 7.3. 1 r 2 r By the law of cosines, 2 2 1 2 1 2 1 2 2 2 cos r r r r r r θ − = + − and hence 2 2 4 4 3 2 2 2 2 2 2 2 2 2 2 1 2 1 2 1 2 2 sin 2 cos r a r a e e I d r r dr d d r r r r r r θ θ φ θ − − ≡ = − + − The integral is trivial ;the integral is: 2 φ 1 φ π 2 Figure 7.3: choice of coordinate for the integral 2 r 2 2 2 2 1 2 1 2 2 sin 2 cos d r r r r π θ θ θ + − 2 2 1 2 1 2 2 1 2 2 cos r r r r r r θ + − = π 2 2 2 2 1 2 1 2 1 2 1 2 1 2 1 2 1 2 1 2 1 2 2 1 r r rr r r rr rr r r r r rr = + + − + − = + − − { 1 2 1 2 2 1 2 , if 2 , if r r r r r r = Thus 1 2 2 1 4 4 2 2 2 2 2 2 1 3 1 4 r r a r a r I e r dr e r dr r π π ∞ − − = + 1 3 4 1 1 2 1 1 8 r a r a e r a π − = − + It follows that is equal to ee V 1 1 2 4 4 1 1 1 1 1 1 3 2 8 1 1 sin 4 r a r a r e e e r dr d d a a θ θ φ πε π − − − + 2 2 4 8 2 5 128 r a r a r a re r e dr a ∞ − − − + = 2 1 5 5 34 4 4 2 ee e V E ev a πε = = − = Finally , then, The angular integals are easy ,and the integal becomes π 4 1 r 4 4 2 a πε 109 34 75 H ev ev ev = − + = − And therefore Not bad , but we can do better Can we think of a more realistic trial function than Ψ ?? We try the product function 1 2 3 1 1 2 3 , Z r r a Z r r e a π − + Ψ ≡ and treat Z as a variable rather than setting it equal to 2. The idea is that as each electron shields the nuclear charge seen by the other ,the effective Z is less than 2. In the following, we will treat Z as a variational parameter, picking the value that minimizes . H Rewrite in the following form: H 2 2 2 2 2 1 2 1 2 1 2 1 2 2 2 1 2 4 4 Z Z e Z Z e H m r r r r r r πε πε − − = − ∇ + ∇ − + + + + − The expectation value of is evidently H 2 1 e 2 2 1 1 2 2 2 4 ee e H Z E Z V r πε = + − + r 1 1 r Here is the expectation value of in the one-particle hydrogenic ground state but with nuclear charge Z. 100 Ψ And according to Chapter 6, we know 1 a r Z = The expection value of is the same as before ,except that instead of ,we now want arbitrary Z—so we multiply by : 2 = Z Z a ee V multiply by : 2 Z a 2 1 5 5 8 4 4 ee Z e Z V E a πε = = − Putting all this together, we find 2 2 1 1 2 4 2 5 4 2 27 4 H Z Z Z Z E Z Z E = − − = − + The lowest upper bound occurs when is minimized: H 1 4 27 4 d H Z E dZ = − + = from which it follows that 2 7 1 .6 9 Z = = 1 .6 9 1 6 Z = = Putting in this value for Z, we find 6 1 1 3 77.5 2 2 H E ev = = − Much nearer to experimental value

7.3 The hydrogen molecule ion