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We investigate the full counting statistics of a harmonically confined 1d short range Riesz gas consisting of N particles in equilibrium at finite temperature. The particles interact with each other through a repulsive power-law interaction with an exponent k > 1 which includes the Calogero–Moser model for k = 2. We examine the probability distribution of the number of particles in a finite domain [ − W , W ] called number distribution, denoted by N ( W , N ) . We analyze the probability distribution of N ( W , N ) and show that it exhibits a large deviation form for large N characterized by a speed N 3 k + 2 k + 2 and by a large deviation function (LDF) of the fraction c = N ( W , N ) / N of the particles inside the domain and W. We show that the density profiles that create the large deviations display interesting shape transitions as one varies c and W. This is manifested by a third-order phase transition exhibited by the LDF that has discontinuous third derivatives. Monte–Carlo simulations based on Metropolis–Hashtings (MH) algorithm show good agreement with our analytical expressions for the corresponding density profiles. We find that the typical fluctuations of N ( W , N ) , obtained from our field theoretic calculations are Gaussian distributed with a variance that scales as N ν k , with ν k = ( 2 − k ) / ( 2 + k ) . We also present some numerical findings on the mean and the variance. Furthermore, we adapt our formalism to study the index distribution (where the domain is semi-infinite ( − ∞ , W ] ) , linear statistics (the variance), thermodynamic pressure and bulk modulus.
We investigate the full counting statistics of a harmonically confined 1d short range Riesz gas consisting of N particles in equilibrium at finite temperature. The particles interact with each other through a repulsive power-law interaction with an exponent k > 1 which includes the Calogero–Moser model for k = 2. We examine the probability distribution of the number of particles in a finite domain [ − W , W ] called number distribution, denoted by N ( W , N ) . We analyze the probability distribution of N ( W , N ) and show that it exhibits a large deviation form for large N characterized by a speed N 3 k + 2 k + 2 and by a large deviation function (LDF) of the fraction c = N ( W , N ) / N of the particles inside the domain and W. We show that the density profiles that create the large deviations display interesting shape transitions as one varies c and W. This is manifested by a third-order phase transition exhibited by the LDF that has discontinuous third derivatives. Monte–Carlo simulations based on Metropolis–Hashtings (MH) algorithm show good agreement with our analytical expressions for the corresponding density profiles. We find that the typical fluctuations of N ( W , N ) , obtained from our field theoretic calculations are Gaussian distributed with a variance that scales as N ν k , with ν k = ( 2 − k ) / ( 2 + k ) . We also present some numerical findings on the mean and the variance. Furthermore, we adapt our formalism to study the index distribution (where the domain is semi-infinite ( − ∞ , W ] ) , linear statistics (the variance), thermodynamic pressure and bulk modulus.
We consider a system of NN spinless fermions, interacting with each other via a power-law interaction \epsilon/r^nϵ/rn, and trapped in an external harmonic potential V(r) = r^2/2V(r)=r2/2, in d=1,2,3d=1,2,3 dimensions. For any 0 < n < d+20<n<d+2, we obtain the ground-state energy E_NEN of the system perturbatively in \epsilonϵ, E_{N}=E_{N}^{≤ft(0)}+\epsilon E_{N}^{≤ft(1)}+O≤ft(\epsilon^{2})EN=EN≤ft(0)+ϵEN≤ft(1)+O≤ft(ϵ2). We calculate E_{N}^{≤ft(1)}EN≤ft(1) exactly, assuming that NN is such that the “outer shell” is filled. For the case of n=1n=1 (corresponding to a Coulomb interaction for d=3d=3), we extract the N \gg 1N≫1 behavior of E_{N}^{≤ft(1)}EN≤ft(1), focusing on the corrections to the exchange term with respect to the leading-order term that is predicted from the local density approximation applied to the Thomas-Fermi approximate density distribution. The leading correction contains a logarithmic divergence, and is of particular importance in the context of density functional theory. We also study the effect of the interactions on the fermions’ spatial density. Finally, we find that our result for E_{N}^{≤ft(1)}EN≤ft(1) significantly simplifies in the case where nn is even.
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