Student Seminar: Classical and Quantum Integrable Systems
Student Seminar: Classical and Quantum Integrable Systems
Student Seminar: Classical and Quantum Integrable Systems
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corresponding to equal eigenvalues form a representation of su(2) with spin s = 1<br />
<strong>and</strong> the state<br />
⎛ ⎞<br />
0<br />
vs=0 hw = ⎜ −1<br />
⎟<br />
⎝ 1 ⎠<br />
}<br />
0<br />
{{ }<br />
h.w.<br />
which corresponds to 3 J is a singlet of su(2). Indeed, the generators of the global<br />
2<br />
su(2) are realized as<br />
⎛ ⎞<br />
⎛ ⎞<br />
⎛ ⎞<br />
0 1 1 0<br />
0 0 0 0<br />
1 0 0 0<br />
S + = ⎜ 0 0 0 1<br />
⎟<br />
⎝ 0 0 0 1 ⎠ , S− = ⎜ 1 0 0 0<br />
⎟<br />
⎝ 1 0 0 0 ⎠ , S3 = ⎜ 0 0 0 0<br />
⎟<br />
⎝ 0 0 0 0 ⎠ .<br />
0 0 0 0<br />
0 1 1 0<br />
0 0 0 −1<br />
The vectors vs=1 hw <strong>and</strong> vs=0 hw are the highest-weight vectors of the s = 1 <strong>and</strong> s = 0<br />
representations respectively, because they are annihilated by S + <strong>and</strong> are eigenstates<br />
of S 3 . In fact, vs=0 hw is also annihilated by S − which shows that this state has zero<br />
spin. Thus, we completely understood the structure of the Hilbert space for L = 2.<br />
In general, the Hamiltonian can be realized as 2 L × 2 L symmetric matrix which<br />
means that it has a complete orthogonal system of eigenvectors. The Hilbert space<br />
split into sum of irreducible representations of su(2). Thus, for L being finite the<br />
problem of finding the eigenvalues of H reduces to the problem of diagonalizing a<br />
symmetric 2 L ×2 L matrix. This can be easily achieved by computer provided L is sufficiently<br />
small. However, for the physically interesting regime L → ∞ corresponding<br />
to the thermodynamic limit new analytic methods are required.<br />
In what follows it is useful to introduce the following operator:<br />
P = 1 2<br />
(<br />
I ⊗ I + ∑ α<br />
) ( 1<br />
σ α ⊗ σ α = 2<br />
4 I ⊗ I + ∑ α<br />
S α ⊗ S α )<br />
which acts on C 2 ⊗ C 2 as the permutation: P (a ⊗ b) = b ⊗ a. Indeed, we have<br />
It is appropriate to call S 3 the operator of the total spin. On a state |ψ〉 with<br />
M spins down we have<br />
S 3 |ψ〉 =<br />
( 1<br />
2 (L − M) − 1 ) ( 1<br />
)<br />
2 M |ψ〉 =<br />
2 L − M |ψ〉 .<br />
Since [H, S 3 ] = 0 the Hamiltonian can be diagonalized within each subspace of the<br />
full Hilbert space with a given total spin (which is uniquely characterized by the<br />
number of spins down).<br />
Let M < L be a number of overturned spins. If M = 0 we have a unique state<br />
|F 〉 = | ↑ · · · ↑〉.<br />
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