156,588 research outputs found

    The effect of spatial transverse coherence property of a thermal source on Ghost imaging and Ghost imaging via compressive sampling

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    Both ghost imaging (GI) and ghost imaging via compressive sampling (GICS) can nonlocally image an object. We report the influence of spatial transverse coherence property of a thermal source on GI and GICS and show that, using the same acquisition numbers, the signal-to-noise ratio (SNR) of images recovered by GI will be reduced while the quality of reconstructed images will be enhanced for GICS as the spatial transverse coherence lengths located on the object plane are decreased. Differences between GI and GICS, methods to further improve the quality and image extraction efficiency of GICS, and its potential applications are also discussed.Comment: 7 pages, 5 figure

    The general property of dynamical quintessence field

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    We discuss the general dynamical behaviors of quintessence field, in particular, the general conditions for tracking and thawing solutions are discussed. We explain what the tracking solutions mean and in what sense the results depend on the initial conditions. Based on the definition of tracking solution, we give a simple explanation on the existence of a general relation between wϕw_\phi and Ωϕ\Omega_\phi which is independent of the initial conditions for the tracking solution. A more general tracker theorem which requires large initial values of the roll parameter is then proposed. To get thawing solutions, the initial value of the roll parameter needs to be small. The power-law and pseudo-Nambu Goldstone boson potentials are used to discuss the tracking and thawing solutions. A more general wϕ−Ωϕw_\phi-\Omega_\phi relation is derived for the thawing solutions. Based on the asymptotical behavior of the wϕ−Ωϕw_\phi-\Omega_\phi relation, the flow parameter is used to give an upper limit on wϕ′w_\phi' for the thawing solutions. If we use the observational constraint wϕ0<−0.8w_{\phi 0}<-0.8 and 0.2<Ωm0<0.40.2<\Omega_{m0}<0.4, then we require n≲1n\lesssim 1 for the inverse power-law potential V(ϕ)=V0(ϕ/mpl)−nV(\phi)=V_0(\phi/m_{pl})^{-n} with tracking solutions and the initial value of the roll parameter ∣λi∣<1.3|\lambda_i|<1.3 for the potentials with the thawing solutions.Comment: 11 figures, corrected some typos and presentation improved, PLB in pres
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