93 research outputs found

    Cosmic constraint on the unified model of dark sectors with or without a cosmic string fluid in the varying gravitational constant theory

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    Observations indicate that most of the universal matter are invisible and the gravitational constant G(t)G(t) maybe depends on the time. A theory of the variational GG (VG) is explored in this paper, with naturally producing the useful dark components in universe. We utilize the observational data: lookback time data, model-independent gamma ray bursts, growth function of matter linear perturbations, type Ia supernovae data with systematic errors, CMB and BAO to restrict the unified model (UM) of dark components in VG theory. Using the best-fit values of parameters with the covariance matrix, constraints on the variation of GG are (GG0)z=3.5≃1.0015βˆ’0.0075+0.0071(\frac{G}{G_{0}})_{z=3.5}\simeq 1.0015^{+0.0071}_{-0.0075} and (GΛ™G)todayβ‰ƒβˆ’0.7252βˆ’2.3645+2.3645Γ—10βˆ’13yrβˆ’1(\frac{\dot{G}}{G})_{today}\simeq -0.7252^{+2.3645}_{-2.3645}\times 10^{-13} yr^{-1}, the small uncertainties around constants. Limit on the equation of state of dark matter is w0dm=0.0072βˆ’0.0170+0.0170w_{0dm}=0.0072^{+0.0170}_{-0.0170} with assuming w0de=βˆ’1w_{0de}=-1 in unified model, and dark energy is w0de=βˆ’0.9986βˆ’0.0011+0.0011w_{0de}=-0.9986^{+0.0011}_{-0.0011} with assuming w0dm=0w_{0dm}=0 at prior. Restriction on UM parameters are Bs=0.7442βˆ’0.0132βˆ’0.0292+0.0137+0.0262B_{s}=0.7442^{+0.0137+0.0262}_{-0.0132-0.0292} and Ξ±=0.0002βˆ’0.0209βˆ’0.0422+0.0206+0.0441\alpha=0.0002^{+0.0206+0.0441}_{-0.0209-0.0422} with 1Οƒ1\sigma and 2Οƒ2\sigma confidence level. In addition, the effect of a cosmic string fluid on unified model in VG theory are investigated. In this case it is found that the Ξ›\LambdaCDM (Ξ©s=0\Omega_{s}=0, Ξ²=0\beta=0 and Ξ±=0\alpha=0) is included in this VG-UM model at 1Οƒ1\sigma confidence level, and the larger errors are given: Ξ©s=βˆ’0.0106βˆ’0.0305βˆ’0.0509+0.0312+0.0582\Omega_{s}=-0.0106^{+0.0312+0.0582}_{-0.0305-0.0509} (dimensionless energy density of cosmic string), (GG0)z=3.5≃1.0008βˆ’0.0584+0.0620(\frac{G}{G_{0}})_{z=3.5}\simeq 1.0008^{+0.0620}_{-0.0584} and (GΛ™G)todayβ‰ƒβˆ’0.3496βˆ’26.3135+26.3135Γ—10βˆ’13yrβˆ’1(\frac{\dot{G}}{G})_{today}\simeq -0.3496^{+26.3135}_{-26.3135}\times 10^{-13}yr^{-1}.Comment: 17 pages,4 figure

    Chinese Firms in the Belt and Road Initiative: A Cross-Sectoral Study of BRI Activities in Kenya

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    The long-time development of the Belt and Road Initiative (BRI) has sparked debates between scholars who emphasize a state-led approach and those who see decentralized project operations initiated by profit motives. This study bridges this divide by examining the practices of Chinese firms within the BRI, shedding light on state-business relations. Focusing on Kenya, a pivotal maritime BRI location, it explores Chinese state-firm relational dynamics in infrastructure, trade, and manufacturing BRI projects. The findings reveal that Chinese firms in Kenya, private or state-owned, play a partial strategic role. The Chinese state selects activities crucial for establishing a mutually beneficial narrative and guides firms through official visits and awards to build positive reputations. However, firms remain commercially oriented and seek state assistance based on business needs. Private and state- owned Chinese firms in Kenya share a certain level of similarity in accessing state support, both financial and operational

    Investigate the interaction between dark matter and dark energy

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    In this paper we investigate the interaction between dark matter and dark energy by considering two different interacting scenarios, i.e. the cases of constant interaction function and variable interaction function. By fitting the current observational data to constrain the interacting models, it is found that the interacting strength is non-vanishing, but weak for the case of constant interaction function, and the interaction is not obvious for the case of variable interaction function. In addition, for seeing the influence from interaction we also investigate the evolutions of interaction function, effective state parameter for dark energy and energy density of dark matter. At last some geometrical quantities in the interacting scenarios are discussed.Comment: 14 pages, 6 figure

    UAV-assisted data dissemination based on network coding in vehicular networks

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    Efficient and emergency data dissemination service in vehicular networks (VN) is very important in some situations, such as earthquakes, maritime rescue, and serious traffic accidents. Data loss frequently occurs in the data transition due to the unreliability of the wireless channel and there are no enough available UAVs providing data dissemination service for the large disaster areas. UAV with an adjustable active antenna can be used in light of the situation. However, data dissemination assisted by UAV with the adjustable active antenna needs corresponding effective data dissemination framework. A UAV-assisted data dissemination method based on network coding is proposed. First, the graph theory to model the state of the data loss of the vehicles is used; the data dissemination problem is transformed as the maximum clique problem of the graph. With the coverage of the directional antenna being limited, a parallel method to find the maximum clique based on the region division is proposed. Lastly, the method\u27s effectiveness is demonstrated by the simulation; the results show that the solution proposed can accelerate the solving process of finding the maximum clique and reduce the number of UAV broadcasts. This manuscript designs a novel scheme for the UAV-assisted data dissemination in vehicular networks based on network coding. The graph theory is used to model the state of the data loss of the vehicles. With the coverage of the directional antenna being limited, then a parallel method is proposed to find the maximum clique of the graph based on the region division. The effectiveness of the method is demonstrated by the simulation
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