2013
DOI: 10.1016/j.nuclphysb.2012.09.008
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The exactly solvable spin Sutherland model of type and its related spin chain

Abstract: We compute the spectrum of the su(m) spin Sutherland model of B N type, including the exact degeneracy of all energy levels. By studying the large coupling constant limit of this model and of its scalar counterpart, we evaluate the partition function of their associated spin chain of Haldane-Shastry type in closed form. With the help of the formula for the partition function thus obtained we study the chain's spectrum, showing that it cannot be obtained as a limiting case of its BC N counterpart. The structure… Show more

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Cited by 11 publications
(19 citation statements)
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“…A well-known property shared by all spin chains of HS type is the fact that their level density becomes asymptotically Gaussian when the number of spins is large enough. This property has been rigorously established for all HS chains of type A N−1 [38], and there is strong numerical evidence that it also holds for other root systems and in the supersymmetric case [43][44][45][46][47][48][49]. Since the Haldane-Shastry chain is the k → 0 limit of Inozemtsev's chain, it is natural to investigate whether the level density of the latter chain is also approximately Gaussian when N 1.…”
Section: Level Densitymentioning
confidence: 99%
“…A well-known property shared by all spin chains of HS type is the fact that their level density becomes asymptotically Gaussian when the number of spins is large enough. This property has been rigorously established for all HS chains of type A N−1 [38], and there is strong numerical evidence that it also holds for other root systems and in the supersymmetric case [43][44][45][46][47][48][49]. Since the Haldane-Shastry chain is the k → 0 limit of Inozemtsev's chain, it is natural to investigate whether the level density of the latter chain is also approximately Gaussian when N 1.…”
Section: Level Densitymentioning
confidence: 99%
“…A characteristic property of all spin chains of Haldane-Shastry type is the fact that their level density approaches a Gaussian distribution as the number of spins tends to infinity. This property has been rigorously proved for the chains of A N −1 type and their related one-dimensional vertex models [51,52], and has been numerically checked for the B N , BC N and D N type chains with standard spin reversal operators [37][38][39]41]. More recently, it has been established that the level density of the BC N -type PF chain with PSRO shows a similar behavior [1].…”
Section: Statistical Properties Of the Spectrummentioning
confidence: 90%
“…In the spin chains studied in Refs. [35][36][37][38][39][40][41], the operators S i are represented by spin reversal operators P i (acting on the Hilbert space of the i-th particle), but this is by no means the only possible choice. As a matter of fact, in the novel version of the spin Calogero model of BC N type and its corresponding (PF) chain introduced in Ref.…”
Section: Introductionmentioning
confidence: 99%
“…Nor is it clearly associated with the A N root system like, e.g., the original HS chain and its rational [35,53], hyperbolic [54] and elliptic [47] counterparts, due to the presence of the operators S i in the Hamiltonian. Thus the chain Hamiltonian (2.1) is not directly associated with an extended root system, unlike most chains of HS type considered so far in the literature (see, e.g., [40,42,43,55] for other instances of HS-like chains of BC N , B N and D N types). For each k = 1, .…”
Section: The Modelsmentioning
confidence: 96%
“…The main idea in this respect is to replace the A N −1 root system associated with the interaction potential of the spin Sutherland model, which yields the original HS chain, by other (extended) root systems like, e.g., BC N , B N and D N . The spin Sutherland models associated with all of these root systems have in fact been studied in the literature, and used to construct spin chains of HS type by taking their strong coupling limits [40][41][42][43]. In particular, the exact partition function of each of these chains has been computed in closed form applying the freezing trick to their parent spin dynamical models.…”
Section: Introductionmentioning
confidence: 99%