5,737 research outputs found

    Stability and structure of two coupled boson systems in an external field

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    The lowest adiabatic potential expressed in hyperspherical coordinates is estimated for two boson systems in an external harmonic trap. Corresponding conditions for stability are investigated and the related structures are extracted for zero-range interactions. Strong repulsion between non-identical particles leads to two new features, respectively when identical particles attract or repel each other. For repulsion new stable structures arise with displaced center of masses. For attraction the mean-field stability region is restricted due to motion of the center of masses

    Bremsstrahlung from relativistic bare heavy ions in single crystals

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    We calculate the bremsstrahlung emitted by heavy bare ions penetrating single crystals at highly relativistic energies. The main component, originating in scattering of the virtual photons of screened target nuclei on the projectile, appears with energies of, approximately, 25γ MeV for a lead ion (γ ≡ E/Mc2 where E and M denote projectile energy and mass). It shows dips in yield upon variation of the incidence angle to major crystallographic directions quite similar to those of other close-encounter processes. Incoherent interaction with single target electrons gives rise to two additional but quite different bremsstrahlung components, a moderate component distributed over the same frequencies as the main component, and a strong component confined to low energies. The channeling characteristics of the total bremsstrahlung spectrum vary substantially with photon energy

    Signatures of the superfluid to Mott insulator transition in equilibrium and in dynamical ramps

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    We investigate the equilibrium and dynamical properties of the Bose-Hubbard model and the related particle-hole symmetric spin-1 model in the vicinity of the superfluid to Mott insulator quantum phase transition. We employ the following methods: exact-diagonalization, mean field (Gutzwiller), cluster mean-field, and mean-field plus Gaussian fluctuations. In the first part of the paper we benchmark the four methods by analyzing the equilibrium problem and give numerical estimates for observables such as the density of double occupancies and their correlation function. In the second part, we study parametric ramps from the superfluid to the Mott insulator and map out the crossover from the regime of fast ramps, which is dominated by local physics, to the regime of slow ramps with a characteristic universal power law scaling, which is dominated by long wavelength excitations. We calculate values of several relevant physical observables, characteristic time scales, and an optimal protocol needed for observing universal scaling.Comment: 23 pages, 13 figure

    Near-optimal two-mode spin squeezing via feedback

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    We propose a feedback scheme for the production of two-mode spin squeezing. We determine a general expression for the optimal feedback, which is also applicable to the case of single-mode spin squeezing. The two-mode spin squeezed states obtained via this feedback are optimal for j=1/2 and are very close to optimal for j>1/2. In addition, the master equation suggests a Hamiltonian that would produce two-mode spin squeezing without feedback, and is analogous to the two-axis countertwisting Hamiltonian in the single mode case.Comment: 10 pages, 6 figures, journal versio

    Gravity vs radiation model: on the importance of scale and heterogeneity in commuting flows

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    We test the recently introduced radiation model against the gravity model for the system composed of England and Wales, both for commuting patterns and for public transportation flows. The analysis is performed both at macroscopic scales, i.e. at the national scale, and at microscopic scales, i.e. at the city level. It is shown that the thermodynamic limit assumption for the original radiation model significantly underestimates the commuting flows for large cities. We then generalize the radiation model, introducing the correct normalisation factor for finite systems. We show that even if the gravity model has a better overall performance the parameter-free radiation model gives competitive results, especially for large scales.Comment: in press Phys. Rev. E, 201
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