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BOGOLIUBOV SPECTRUM OF INTERACTING BOSE GASES 41<br />

contains all pairs of operators (γ,α) on H such that γ is trace class, α is<br />

Hilbert-Schmidt, α T = α and<br />

� γ α<br />

α ∗ 1+JγJ ∗<br />

�<br />

≥ 0 on H⊕H ∗ .<br />

Let us denote by G0 the set of all pairs (γ,α) ∈ G which satisfy<br />

αα ∗ = γ(1+JγJ ∗ ) and γα = αJγJ ∗ . (65)<br />

The significance of G0 is that for any (γ,α) ∈ G0, there exists a unique<br />

quasi-free pure state Φ ∈ F(H) such that<br />

(γ,α) = (γΦ,αΦ).<br />

Any element in G is also associated with a unique state, but the latter is a<br />

mixed state.<br />

The one-body density matrices offer a simple way to define quadratic<br />

Hamiltonians. More precisely, let H be a self-adjoint operator on H and let<br />

K be a Hilbert-Schmidt operator on H such that K = K T and such that<br />

the following inequality holds true<br />

�<br />

A := ≥ η > 0 on H⊕H ∗ . (66)<br />

� H K<br />

K ∗ JHJ ∗<br />

We shall consider the quadratic Hamiltonian H on F(H) defined by<br />

〈H〉 Φ := q(γΦ,αΦ) = Tr[HγΦ]+ℜTr[KαΦ] (67)<br />

for every state Φ living in the truncated Fock spaces and in the domain of<br />

H:<br />

� M� n�<br />

D(H). (68)<br />

M≥0 n=0 sym<br />

It can be verified that the so-defined operator H is exactly the Bogoliubov<br />

Hamiltonian given in (12).<br />

The main properties of the quadratic Hamiltonian H are given in the<br />

following<br />

Theorem 27 (Bogoliubov Hamiltonian). Let H be defined by (67) and assume<br />

that (66) holds true. Then we have the following statements.<br />

(i) (Form domain). We have the quadratic-form inequalities<br />

C −1 dΓ(H)−C ≤ H ≤ dΓ(H +C)+C (69)<br />

As a consequence, the form domain of the Friedrichs extension of H (still<br />

denoted by H) is the same as that of dΓ(H) on F+.<br />

(ii) (Variational principle). For any (γ,α) ∈ G, we can find (γ ′ ,α ′ ) ∈ G0<br />

such that q(γ ′ ,α ′ ) ≤ q(γ,α) and the inequality is strict expect when (γ,α) ∈<br />

G0. As a consequence, the ground state energy of H is<br />

infσ(H) = inf q(γ,α) = inf q(γ,α).<br />

(γ,α)∈G (γ,α)∈G0<br />

(iii) (Ground state and ground state energy). The Hamiltonian H has a<br />

unique ground state in F(H), which is a pure quasi-free state. Moreover,<br />

we always have infσ(H) < 0 except when K = 0 in which case infσ(H) = 0<br />

with the vacuum being the corresponding ground state.

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