Lattice Normal Modes and Phonons Via Quantum Mechanics

Lattice Normal Modes and Phonons Via Quantum Mechanics

Tom Ouldridge Keble College Lattice Normal Modes and Phonons via Quantum Mechanics The Hamiltonian for the 1-D monatomic chain is a sum of coupled harmonic oscillators: 2 2 X pj m! H = + 0 (x − x )2 (1) 2m 2 j+1 j j Show that the following Fourier decomposition decouples them; −1=2 X −ikja −1=2 X ikja xj = N e Xk pj = N e Pk (2) k k into the from: 2 XP−kPk m! H = + 0 (4 sin2(ka=2))X X (3) 2m 2 −k k k where N is the number of atoms in the chain and a is the equilibrium atomic spacing. P 0 Hint: use the identity j exp(i(k + k)ja) = Nδk;−k0 . What are the allowed values of k? To do this part we simply substitute in the new operators as given to us. Be careful with your indeces! i(k+l)ja 2 ! X PkPle m! H = N −1 + 0 e−ika − 1 e−ikjaX e−ila − 1 e−iklaX : (4) 2m 2 k l j;k;l If we perform the j summation first, we can use the identity provided in the hint: 2 ! X PkPl m! H = δ + 0 e−ika − 1 e−ila − 1 X X δ ; (5) 2m k;−l 2 k l k;−l k;l 2 ! X PkP−k m! =) H = + 0 e−ika − 1 eika − 1 X X ; (6) 2m 2 k −k k 2 ! X PkP−k m! =) H = + 0 (2 − 2 cos(ka)) X X ; (7) 2m 2 k −k k 2 ! X PkP−k m! =) H = + 0 4 sin2(ka=2) X X : (8) 2m 2 k −k k We are perfectly at liberty to change the dummy index k to −k, obtaining exactly the form in Eqn. 3. In defining our Fourier transforms (Eqn. 2), our k values are exactly the the values of k within 2πm the first Brillouin zone which are allowed by periodic boundary conditions: i.e., k = Na . This is to provide the correct periodicity of xj. So far we have made no assumptions about whether we are dealing with a quantum or a classical system. In the classical case, we could use this form of H to derive the same dispersion as in question 2 (don't worry about the details of how to do this - the easiest way is with Hamiltonian mechanics). In the quantum case, we need to explicitly consider the observables a operators. 1 y y 1. Show that [Xk;Pq] = i¯hδk;q, and that Xk = X−k (and similarly for Pk ). To do this you will y need to use the hermitian property of xj: xj = xj. 2. Define the operator ak by: 1=2 m!k i y ak = (Xk + Pk ); (9) 2¯h m!k y where !k = 2!0j sin(ka=2)j. Show that [ak; aq] = δk;q, and hence that the Hamiltonian simplifies to the form: X y H = ¯h!k(akak + 1=2) (10) k 1. To do the commutator, we again just substitute in. To do this, first invert Eqn. 2, which is reasonably simple. 2 3 −1=2 X ikja −1=2 X −iqla [Xk;Pq] = 4N e xj;N e pl5 ; (11) j l −1 X ikja −iqla =) [Xk;Pq] = N e e [xj; pl] : (12) j;l Now we can use the good old commutation relations of second year, [xj; pl] = i¯hδj;l, i¯h X [X ;P ] = ei(k−q)ja = i¯hδ : (13) k q N i;j j The conjugation property is not too hard to show: 0 1y y −1=2 X ikja −1=2 X −ikja y −1=2 X −ikja Xk = @N e xjA = N e xj = N e xj = X−k (14) j j j 2. We now have everything we need to evaluate the second commutator: i [a ; ay] = −(! =! )1=2[X ;P ] + (! =! )1=2[P y;Xy] = δ : (15) k q 2¯h k q k q q k k q k;q y To prove that we can rewrite the Hamiltonian, it is easiest to expandh! ¯ k(akak + 1=2): 2 y ¯hmwk y −i i y y 1 y ¯h!k ¯h!k(akak + 1=2) = XkXk + XkPk + Pk Xk + 2 Pk Pk + : 2¯h m!k m!k (m!k) 2 (16) y y We now commute Pk and Xk, and use the conjugation relation derived earlier: 2 y mwk 1 −i i ¯h ¯h!k ¯h!k(akak+1=2) = XkX−k + 2 PkP−k + XkPk + X−kP−k − + : 2 (m!k) m!k m!k m!k 2 (17) 2 y mwk 1 −i i =) ¯h!k(akak +1=2) = XkX−k + 2 PkP−k + XkPk + X−kP−k) : 2 (m!k) m!k m!k (18) If we sum over all k, the third and fourth terms will cancel each other. 2 X y X mwk 1 =) ¯h!k(akak + 1=2) = XkX−k + 2 PkP−k : (19) 2 (m!k) k k Which is the Hamiltonian! 2 We have now decoupled the system into independent quantum oscillators. What is the energy spec- trum? Explain what each of the new operators means physically. Referring to your answer, or otherwise, explain what a phonon is. P E = k ¯h!k(nk + 1=2) y ak increases the energy of the kth normal mode by ¯hwk, and ak decreases it by the same amount. These quantized excitations of the normal modes can be interpreted as bosons, which we call phonons. 3.

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