165 research outputs found

    Pair excitations and the mean field approximation of interacting Bosons, II

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    We consider a large number of Bosons with interaction potential vN(x)=N3βv(Nβx)v_N(x)=N^{3 \beta}v(N^{\beta}x). In earlier papers we considered a set of equations for the condensate ϕ\phi and pair excitation function kk and proved that they provide a Fock space approximation to the exact evolution of the condensate for β<13\beta <\frac{1}{3}. This result was extended to the case β<12\beta<\frac{1}{2} by E. Kuz, where it was also argued informally that the equations of our earlier work do not provide an approximation for β>12\beta>\frac{1}{2}. In 2013, we introduced a coupled refinement of our original equations and conjectured that they provide a Fock space approximation in the range 0≤β<10 \le \beta < 1. In the current paper we prove that this is indeed the case for β<23\beta < \frac{2}{3}, at least locally in time. In order to do that, we re-formulate the equations of \cite{GMM} in a way reminiscent of BBGKY and apply harmonic analysis techniques in the spirit of X. Chen and J. Holmer to prove the necessary estimates. In turn, these estimates provide bounds for the pair excitation function kk

    Second-order corrections to mean-field evolution of weakly interacting Bosons, II

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    We study the evolution of a N-body weakly interacting system of Bosons. Our work forms an extension of our previous paper I, in which we derived a second-order correction to a mean-field evolution law for coherent states in the presence of small interaction potential. Here, we remove the assumption of smallness of the interaction potential and prove global existence of solutions to the equation for the second-order correction. This implies an improved Fock-space estimate for our approximation of the N-body state

    Pair excitations and the mean field approximation of interacting Bosons, I

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    In our previous work \cite{GMM1},\cite{GMM2} we introduced a correction to the mean field approximation of interacting Bosons. This correction describes the evolution of pairs of particles that leave the condensate and subsequently evolve on a background formed by the condensate. In \cite{GMM2} we carried out the analysis assuming that the interactions are independent of the number of particles NN. Here we consider the case of stronger interactions. We offer a new transparent derivation for the evolution of pair excitations. Indeed, we obtain a pair of linear equations describing their evolution. Furthermore, we obtain apriory estimates independent of the number of particles and use these to compare the exact with the approximate dynamics

    Bifurcation and stability for Nonlinear Schroedinger equations with double well potential in the semiclassical limit

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    We consider the stationary solutions for a class of Schroedinger equations with a symmetric double-well potential and a nonlinear perturbation. Here, in the semiclassical limit we prove that the reduction to a finite-mode approximation give the stationary solutions, up to an exponentially small term, and that symmetry-breaking bifurcation occurs at a given value for the strength of the nonlinear term. The kind of bifurcation picture only depends on the non-linearity power. We then discuss the stability/instability properties of each branch of the stationary solutions. Finally, we consider an explicit one-dimensional toy model where the double well potential is given by means of a couple of attractive Dirac's delta pointwise interactions.Comment: 46 pages, 4 figure

    Orbital stability of periodic waves for the nonlinear Schroedinger equation

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    The nonlinear Schroedinger equation has several families of quasi-periodic travelling waves, each of which can be parametrized up to symmetries by two real numbers: the period of the modulus of the wave profile, and the variation of its phase over a period (Floquet exponent). In the defocusing case, we show that these travelling waves are orbitally stable within the class of solutions having the same period and the same Floquet exponent. This generalizes a previous work where only small amplitude solutions were considered. A similar result is obtained in the focusing case, under a non-degeneracy condition which can be checked numerically. The proof relies on the general approach to orbital stability as developed by Grillakis, Shatah, and Strauss, and requires a detailed analysis of the Hamiltonian system satisfied by the wave profile.Comment: 34 pages, 7 figure

    Pair excitations and the mean field approximation of interacting Bosons

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    Abstract. In our previous wor

    Stability and symmetry-breaking bifurcation for the ground states of a NLS with a δ′\delta^\prime interaction

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    We determine and study the ground states of a focusing Schr\"odinger equation in dimension one with a power nonlinearity ∣ψ∣2μψ|\psi|^{2\mu} \psi and a strong inhomogeneity represented by a singular point perturbation, the so-called (attractive) δ′\delta^\prime interaction, located at the origin. The time-dependent problem turns out to be globally well posed in the subcritical regime, and locally well posed in the supercritical and critical regime in the appropriate energy space. The set of the (nonlinear) ground states is completely determined. For any value of the nonlinearity power, it exhibits a symmetry breaking bifurcation structure as a function of the frequency (i.e., the nonlinear eigenvalue) ω\omega. More precisely, there exists a critical value \om^* of the nonlinear eigenvalue \om, such that: if \om_0 < \om < \om^*, then there is a single ground state and it is an odd function; if \om > \om^* then there exist two non-symmetric ground states. We prove that before bifurcation (i.e., for \om < \om^*) and for any subcritical power, every ground state is orbitally stable. After bifurcation (\om =\om^*+0), ground states are stable if μ\mu does not exceed a value μ⋆\mu^\star that lies between 2 and 2.5, and become unstable for μ>μ∗\mu > \mu^*. Finally, for μ>2\mu > 2 and \om \gg \om^*, all ground states are unstable. The branch of odd ground states for \om \om^*, obtaining a family of orbitally unstable stationary states. Existence of ground states is proved by variational techniques, and the stability properties of stationary states are investigated by means of the Grillakis-Shatah-Strauss framework, where some non standard techniques have to be used to establish the needed properties of linearization operators.Comment: 46 pages, 5 figure
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