15,026 research outputs found

    Mean-Field Limit for a Collision-Avoiding Flocking System and the Time-Asymptotic Flocking Dynamics for the Kinetic Equation

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    A Collision-Avoiding flocking particle system proposed in [8] is studied in this paper. The global wellposedness of its corresponding Vlasov-type kinetic equation is proved. As a corollary of the global stability result, the mean field limit of the particle system is obtained. Furthermore, the time-asymptotic flocking behavior of the solution to the kinetic equation is also derived. The technics used for local wellposedness and stability follow from similar ideas to those have been used in [3,22,14]. While in order to extend the local result globally, the main contribution here is to generate a series of new estimates for this Vlasov type equation, which imply that the growing of the characteristics can be controlled globally. Further estimates also show the long time flocking phenomena.Comment: 21 page

    Discriminating dark energy models by using the statefinder hierarchy and the growth rate of matter perturbations

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    We apply the Statefinder hierarchy and the growth rate of matter perturbations to discriminate modified Chaplygin gas (MCG), generalized Chaplygin gas (GCG), superfluid Chaplygin gas (SCG), purely kinetic k-essence (PKK), and Λ\LambdaCDM model. We plot the evolutional trajectories of these models in the statefinder plane and in the composite diagnostic plane. We find that GCG, MCG, SCG, PKK, and Λ\LambdaCDM can be distinguished well from each other at the present epoch by using the composite diagnostic {ϵ(z),S5(1)}\{\epsilon(z), S^{(1)}_{5}\}. Using other combinations, such as {S3(1),S4(1)}\{S^{(1)}_{3}, S^{(1)}_4\}, {S3(1),S5}\{S^{(1)}_{3}, S_{5}\}, {ϵ(z),S3(1)}\{\epsilon(z), S^{(1)}_{3}\}, and {ϵ(z),S4}\{\epsilon(z), S_4 \}, some of these five dark energy models cannot be distinguished.Comment: 12 pages, 9 figure

    Introduction to Holographic Superconductor Models

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    In the last years it has been shown that some properties of strongly coupled superconductors can be potentially described by classical general relativity living in one higher dimension, which is known as holographic superconductors. This paper gives a quick and introductory overview of some holographic superconductor models with s-wave, p-wave and d-wave orders in the literature from point of view of bottom-up, and summarizes some basic properties of these holographic models in various regimes. The competition and coexistence of these superconductivity orders are also studied in these superconductor models.Comment: 93 pages, 38 figures, 2 tables; v3: misprints corrected, published version. arXiv admin note: text overlap with arXiv:1309.5086, arXiv:1007.1981 by other author

    P-V criticality in the extended phase space of Gauss-Bonnet black holes in AdS space

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    We study the P−VP-V criticality and phase transition in the extended phase space of charged Gauss-Bonnet black holes in anti-de Sitter space, where the cosmological constant appears as a dynamical pressure of the system and its conjugate quantity is the thermodynamic volume of the black hole. The black holes can have a Ricci flat (k=0k=0), spherical (k=1k=1), or hyperbolic (k=−1k=-1) horizon. We find that for the Ricci flat and hyperbolic Gauss-Bonnet black holes, no P−VP-V criticality and phase transition appear, while for the black holes with a spherical horizon, even when the charge of the black hole is absent, the P−VP-V criticality and the small black hole/large black hole phase transition will appear, but it happens only in d=5d=5 dimensions; when the charge does not vanish, the P−VP-V criticality and the small black hole/large phase transition always appear in d=5d=5 dimensions; in the case of d≥6d\ge 6, to have the P−VP-V criticality and the small black hole/large black hole phase transition, there exists an upper bound for the parameter b=α~∣Q∣−2/(d−3)b=\widetilde{\alpha}|Q|^{-2/(d-3)}, where α~\tilde {\alpha} is the Gauss-Bonnet coefficient and QQ is the charge of the black hole. We calculate the critical exponents at the critical point and find that for all cases, they are the same as those in the van der Waals liquid-gas system.Comment: 23 pages,9 figure

    Petrov type I Condition and Dual Fluid Dynamics

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    Recently Lysov and Strominger [arXiv:1104.5502] showed that imposing Petrov type I condition on a (p+1)(p+1)-dimensional timelike hypersurface embedded in a (p+2)(p+2)-dimensional vacuum Einstein gravity reduces the degrees of freedom in the extrinsic curvature of the hypersurface to that of a fluid on the hypersurface, and that the leading-order Einstein constraint equations in terms of the mean curvature of the embedding give the incompressible Navier-Stokes equations of the dual fluid. In this paper we show that the non-relativistic fluid dual to vacuum Einstein gravity does not satisfy the Petrov type I condition at next order, unless additional constraint such as the irrotational condition is added. In addition, we show that this procedure can be inversed to derive the non-relativistic hydrodynamics with higher order corrections through imposing the Petrov type I condition, and that some second order transport coefficients can be extracted, but the dual "Petrov type I fluid" does not match the dual fluid constructed from the geometry of vacuum Einstein gravity in the non-relativistic limit. We discuss the procedure both on the finite cutoff surface via the non-relativistic hydrodynamic expansion and on the highly accelerated surface via the near horizon expansion.Comment: 20 pages, published version, with minor improvement

    The evolution of the power law k-essence cosmology

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    We investigate the evolution of the power law k-essence field in FRWL spacetime. The autonomous dynamical system and critical points are obtained. The corresponding cosmological parameters, such as Ωϕ\Omega _{\phi } and wϕw_{\phi }, are calculated at these critical points. We find it is possible to achieve an equation of state crossing through −1-1 for k-essence field. The results we obtained indicate that the power law k-essence dark energy model can be compatible with observations.Comment: 9 pages, 4 figures, some comments are adde

    On the minimal affinizations over the quantum affine algebras of type CnC_n

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    In this paper, we study the minimal affinizations over the quantum affine algebras of type CnC_n by using the theory of cluster algebras. We show that the qq-characters of a large family of minimal affinizations of type CnC_n satisfy some systems of equations. These equations correspond to mutation equations of some cluster algebras. Furthermore, we show that the minimal affinizations in these equations correspond to cluster variables in these cluster algebras.Comment: arXiv admin note: substantial text overlap with arXiv:1501.00146, arXiv:1502.0242

    Ground state of three qubits coupled to a harmonic oscillator with ultrastrong coupling

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    We study the Rabi model composed of three qubits coupled to a harmonic oscillator without involving the rotating-wave approximation. We show that the ground state of the three-qubit Rabi model can be analytically treated by using the transformation method, and the transformed ground state agrees well with the exactly numerical simulation under a wide range of qubit-oscillator coupling strengths for different detunings. We use the pairwise entanglement to characterize the ground-state entanglement between any two qubits and show that it has an approximately quadratic dependence on the qubit-oscillator coupling strength. Interestingly, we find that there is no qubit-qubit entanglement for the ground state if the qubit-oscillator coupling strength is large enough.Comment: 5 pages, 2 figures, Physical Review A 88, 045803 (2013

    A Disease Diagnosis and Treatment Recommendation System Based on Big Data Mining and Cloud Computing

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    It is crucial to provide compatible treatment schemes for a disease according to various symptoms at different stages. However, most classification methods might be ineffective in accurately classifying a disease that holds the characteristics of multiple treatment stages, various symptoms, and multi-pathogenesis. Moreover, there are limited exchanges and cooperative actions in disease diagnoses and treatments between different departments and hospitals. Thus, when new diseases occur with atypical symptoms, inexperienced doctors might have difficulty in identifying them promptly and accurately. Therefore, to maximize the utilization of the advanced medical technology of developed hospitals and the rich medical knowledge of experienced doctors, a Disease Diagnosis and Treatment Recommendation System (DDTRS) is proposed in this paper. First, to effectively identify disease symptoms more accurately, a Density-Peaked Clustering Analysis (DPCA) algorithm is introduced for disease-symptom clustering. In addition, association analyses on Disease-Diagnosis (D-D) rules and Disease-Treatment (D-T) rules are conducted by the Apriori algorithm separately. The appropriate diagnosis and treatment schemes are recommended for patients and inexperienced doctors, even if they are in a limited therapeutic environment. Moreover, to reach the goals of high performance and low latency response, we implement a parallel solution for DDTRS using the Apache Spark cloud platform. Extensive experimental results demonstrate that the proposed DDTRS realizes disease-symptom clustering effectively and derives disease treatment recommendations intelligently and accurately

    Enhanced entanglement of two optical modes in optomechanical systems via an optical parametric amplifier

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    We investigate the effect of a degenerate optical parametric amplifier (OPA) placed inside an optomechanical cavity on the steady-state entanglement of two cavity modes, which jointly interact with a mechanical resonator. Two cavity modes are respectively driven at the red and blue sideband associated with the mechanical resonator, which generates entanglement between them in the limit of resolved sideband. The OPA gives rise to single-mode squeezing of the cavity fields, which results in significant improvement of the two-mode entanglement. It is found that an optimal nonlinear gain of the OPA exists, depending on the system temperatures, which yields the maximum entanglement. The improvement is particularly remarkable for the system at cryogenic temperatures.Comment: 14 pages, 5 figures, to appear in J. Phys.
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