5,447 research outputs found

    Scalar Gravity and Higgs Mechanism

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    The role that the auxiliary scalar field Ï•\phi played in Brans-Dicke cosmology is discussed. If a constant vacuum energy is assumed to be the origin of dark energy, then the corresponding density parameter would be a quantity varying with Ï•\phi; and almost all of the fundamental components of our universe can be unified into the dynamical equation for Ï•\phi. As a generalization of Brans-Dicke theory, we propose a new gravity theory with a complex scalar field Ï•\phi which is coupled to the cosmological curvature scalar. Through such a coupling, the Higgs mechanism is naturally incorporated into the evolution of the universe, and a running density of the field vacuum energy is obtained which may release the particle standard model from the rigorous cosmological constant problem in some sense. Our model predicts a running mass scale of the fundamental particles in which the gauge symmetry breaks spontaneously. The running speed of the mass scale in our case could survive all existing experiments.Comment: 6 page

    Matter Power Spectra in Viable f(R)f(R) Gravity Models with Massive Neutrinos

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    We investigate the matter power spectra in the power law and exponential types of viable f(R)f(R) theories along with massive neutrinos. The enhancement of the matter power spectrum is found to be a generic feature in these models. In particular, we show that in the former type, such as the Starobinsky model, the spectrum is magnified much larger than the latter one, such as the exponential model. A greater scale of the total neutrino mass, Σmν\Sigma m_{\nu}, is allowed in the viable f(R)f(R) models than that in the Λ\LambdaCDM one. We obtain the constraints on the neutrino masses by using the CosmoMC package with the modified MGCAMB. Explicitly, we get $\Sigma m_{\nu} < 0.451 \ (0.214)\ \mathrm{eV}at95thecorrespondingoneforthe at 95% C.L. in the Starobinsky (exponential) model, while the corresponding one for the \LambdaCDMmodelisCDM model is \Sigma m_{\nu} < 0.200\ \mathrm{eV}.Furthermore,bytreatingtheeffectivenumberofneutrinospecies. Furthermore, by treating the effective number of neutrino species N_{\mathrm{eff}}asafreeparameteralongwith as a free parameter along with \Sigma m_{\nu},wefindthat, we find that N_{\mathrm{eff}} = 3.78^{+0.64}_{-0.84} (3.47^{+0.74}_{-0.60})and and \Sigma m_{\nu} = 0.533^{+0.254}_{-0.411}( (< 0.386) \ \mathrm{eV}$ at 95% C.L. in the Starobinsky (exponential) model.Comment: 15 pages, 5 figures, updated version accepted by PL

    Taiwanese newspaper use of government press releases before and after martial law

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    Learning Unmanned Aerial Vehicle Control for Autonomous Target Following

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    While deep reinforcement learning (RL) methods have achieved unprecedented successes in a range of challenging problems, their applicability has been mainly limited to simulation or game domains due to the high sample complexity of the trial-and-error learning process. However, real-world robotic applications often need a data-efficient learning process with safety-critical constraints. In this paper, we consider the challenging problem of learning unmanned aerial vehicle (UAV) control for tracking a moving target. To acquire a strategy that combines perception and control, we represent the policy by a convolutional neural network. We develop a hierarchical approach that combines a model-free policy gradient method with a conventional feedback proportional-integral-derivative (PID) controller to enable stable learning without catastrophic failure. The neural network is trained by a combination of supervised learning from raw images and reinforcement learning from games of self-play. We show that the proposed approach can learn a target following policy in a simulator efficiently and the learned behavior can be successfully transferred to the DJI quadrotor platform for real-world UAV control
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