Emptiness and Depletion Formation Probability in spin models with inverse square interaction

Details Emptiness and Depletion Formation Probability in spin models with inverse square interaction Emptiness and Depletion Formation Probability in spin models with inverse square interaction

2009-08-19

arxiv.org/abs/0908.2652v2

Nucl.Phys.B825:320-340,2010

Physics

Condensed Matter

Strongly Correlated Electrons

26 pages, no figures

Scientific paper

10.1016/j.nuclphysb.2009.09.005

We calculate the Emptiness Formation Probability (EFP) in the spin-Calogero Model (sCM) and Haldane-Shastry Model (HSM) using their hydrodynamic description. The EFP is the probability that a region of space is completely void of particles in the ground state of a quantum many body system. We calculate this probability in an instanton approach, by considering the more general problem of an arbitrary depletion of particles (DFP). In the limit of large size of depletion region the probability is dominated by a classical configuration in imaginary time that satisfies a set of boundary conditions and the action calculated on such solution gives the EFP/DFP with exponential accuracy. We show that the calculation for sCM can be elegantly performed by representing the gradientless hydrodynamics of spin particles as a sum of two spin-less Calogero collective field theories in auxiliary variables. Interestingly, the result we find for the EFP can be casted in a form reminiscing of spin-charge separation, which should be violated for a non-linear effect such as this. We also highlight the connections between sCM, HSM and $\lambda=2$ spin-less Calogero model from a EFP/DFP perspective.

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