47,579 research outputs found

    Pentaquark Θ+\Theta^+ in nuclear matter and Θ+\Theta^+ hypernuclei

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    We study the properties of the Θ+\Theta^+ in nuclear matter and Θ+\Theta^+ hypernuclei within the quark mean-field (QMF) model, which has been successfully used for the description of ordinary nuclei and Λ\Lambda hypernuclei. With the assumption that the non-strange mesons couple only to the uu and dd quarks inside baryons, a sizable attractive potential of the Θ+\Theta^+ in nuclear matter is achieved as a consequence of the cancellation between the attractive scalar potential and the repulsive vector potential. We investigate the Θ+\Theta^+ single-particle energies in light, medium, and heavy nuclei. More bound states are obtained in Θ+\Theta^+ hypernuclei in comparison with those in Λ\Lambda hypernuclei.Comment: 16 pages, 5 figure

    Gain-constrained recursive filtering with stochastic nonlinearities and probabilistic sensor delays

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    This is the post-print of the Article. The official published version can be accessed from the link below - Copyright @ 2013 IEEE.This paper is concerned with the gain-constrained recursive filtering problem for a class of time-varying nonlinear stochastic systems with probabilistic sensor delays and correlated noises. The stochastic nonlinearities are described by statistical means that cover the multiplicative stochastic disturbances as a special case. The phenomenon of probabilistic sensor delays is modeled by introducing a diagonal matrix composed of Bernoulli distributed random variables taking values of 1 or 0, which means that the sensors may experience randomly occurring delays with individual delay characteristics. The process noise is finite-step autocorrelated. The purpose of the addressed gain-constrained filtering problem is to design a filter such that, for all probabilistic sensor delays, stochastic nonlinearities, gain constraint as well as correlated noises, the cost function concerning the filtering error is minimized at each sampling instant, where the filter gain satisfies a certain equality constraint. A new recursive filtering algorithm is developed that ensures both the local optimality and the unbiasedness of the designed filter at each sampling instant which achieving the pre-specified filter gain constraint. A simulation example is provided to illustrate the effectiveness of the proposed filter design approach.This work was supported in part by the National Natural Science Foundation of China by Grants 61273156, 61028008, 60825303, 61104125, and 11271103, National 973 Project by Grant 2009CB320600, the Fok Ying Tung Education Fund by Grant 111064, the Special Fund for the Author of National Excellent Doctoral Dissertation of China by Grant 2007B4, the State Key Laboratory of Integrated Automation for the Process Industry (Northeastern University) of China, the Engineering and Physical Sciences Research Council (EPSRC) of the U.K. by Grant GR/S27658/01, the Royal Society of the U.K., and the Alexander von Humboldt Foundation of Germany

    Superfluidity of Λ\Lambda hyperons in neutron stars

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    We study the 1S0^1S_0 superfluidity of Λ\Lambda hyperons in neutron star matter and neutron stars. We use the relativistic mean field (RMF) theory to calculate the properties of neutron star matter. In the RMF approach, the meson-hyperon couplings are constrained by reasonable hyperon potentials that include the updated information from recent developments in hypernuclear physics. To examine the 1S0^1S_0 pairing gap of Λ\Lambda hyperons, we employ several ΛΛ\Lambda\Lambda interactions based on the Nijmegen models and used in double-Λ\Lambda hypernuclei studies. It is found that the maximal pairing gap obtained is a few tenths of a MeV. The magnitude and the density region of the pairing gap are dependent on the ΛΛ\Lambda\Lambda interaction and the treatment of neutron star matter. We calculate neutron star properties and find that whether the 1S0^1S_0 superfluidity of Λ\Lambda hyperons exists in the core of neutron stars mainly depends on the ΛΛ\Lambda\Lambda interaction used.Comment: 22 pages, 2 Tables, 6 Figur

    Nonlinear analysis of dynamical complex networks

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    Copyright © 2013 Zidong Wang et al. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.Complex networks are composed of a large number of highly interconnected dynamical units and therefore exhibit very complicated dynamics. Examples of such complex networks include the Internet, that is, a network of routers or domains, the World Wide Web (WWW), that is, a network of websites, the brain, that is, a network of neurons, and an organization, that is, a network of people. Since the introduction of the small-world network principle, a great deal of research has been focused on the dependence of the asymptotic behavior of interconnected oscillatory agents on the structural properties of complex networks. It has been found out that the general structure of the interaction network may play a crucial role in the emergence of synchronization phenomena in various fields such as physics, technology, and the life sciences

    Modification of nucleon properties in nuclear matter and finite nuclei

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    We present a model for the description of nuclear matter and finite nuclei, and at the same time, for the study of medium modifications of nucleon properties. The nucleons are described as nontopological solitons which interact through the self-consistent exchange of scalar and vector mesons. The model explicitly incorporates quark degrees of freedom into nuclear many-body systems and provides satisfactory results on the nuclear properties. The present model predicts a significant increase of the nucleon radius at normal nuclear matter density. It is very interesting to see the nucleon properties change from the nuclear surface to the nuclear interior.Comment: 22 pages, 10 figure

    Neutron star matter in the quark-meson coupling model in strong magnetic fields

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    The effects of strong magnetic fields on neutron star matter are investigated in the quark-meson coupling (QMC) model. The QMC model describes a nuclear many-body system as nonoverlapping MIT bags in which quarks interact through self-consistent exchange of scalar and vector mesons in the mean-field approximation. The results of the QMC model are compared with those obtained in a relativistic mean-field (RMF) model. It is found that quantitative differences exist between the QMC and RMF models, while qualitative trends of the magnetic field effects on the equation of state and composition of neutron star matter are very similar.Comment: 16 pages, 4 figure
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