175,894 research outputs found

    The gravitational field of a global monopole

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    We present an exact solution to the non-linear equation which describes a global monopole in the flat space. We re-examine the metric and the geodesics outside the global monopole. We will see that a global monopole produces a repulsive gravitational field outside the core in addition to a solid angular deficit. The lensing property of the global monopole and the global monopole-antimonopole annihilation mechanism are studied.Comment: 8 pages, no figure

    Evaluation of ASTER GDEM ver2 using GPS measurements and SRTM ver4.1 in China

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    The freely available ASTER GDEM ver2 was released by NASA and METI on October 17, 2011. As one of the most complete high resolution digital topographic data sets of the world to date, the ASTER GDEM covers land surfaces between 83°N and 83°S at a spatial resolution of 1 arc-second and will be a useful product for many applications, such as relief analysis, hydrological studies and radar interferometry. The stated improvements in the second version of ASTER GDEM benefit from finer horizontal resolution, offset adjustment and water body detection in addition to new observed ASTER scenes. This study investigates the absolute vertical accuracy of the ASTER GDEM ver2 at five study sites in China using ground control points (GCPs) from high accuracy GPS benchmarks, and also using a DEM-to-DEM comparison with the Consultative Group for International Agriculture Research Consortium for Spatial Information (CGIAR-CSI) SRTM DEM (Version 4.1). And then, the results are separated into GlobCover land cover classes to derive the spatial pattern of error. It is demonstrated that the RMSE (19m) and mean (-13m) values of ASTER GDEM ver2 against GPS-GCPs in the five study areas is lower than its first version ASTER GDEM ver1 (26m and -21m) as a result of the adjustment of the elevation offsets in the new version. It should be noted that the five study areas in this study are representative in terms of terrain types and land covers in China, and even for most of mid-latitude zones. It is believed that the ASTER GDEM offers a major alternative in accessibility to high quality elevation data

    Adiabatic passage of collective excitations in atomic ensembles

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    We describe a theoretical scheme that allows for transfer of quantum states of atomic collective excitation between two macroscopic atomic ensembles localized in two spatially-separated domains. The conception is based on the occurrence of double-exciton dark states due to the collective destructive quantum interference of the emissions from the two atomic ensembles. With an adiabatically coherence manipulation for the atom-field couplings by stimulated Ramann scattering, the dark states will extrapolate from an exciton state of an ensemble to that of another. This realizes the transport of quantum information among atomic ensembles.Comment: 7 pages, 2 figure

    Intersections of homogeneous Cantor sets and beta-expansions

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    Let Γβ,N\Gamma_{\beta,N} be the NN-part homogeneous Cantor set with β(1/(2N1),1/N)\beta\in(1/(2N-1),1/N). Any string (j)=1N(j_\ell)_{\ell=1}^\N with j{0,±1,...,±(N1)}j_\ell\in\{0,\pm 1,...,\pm(N-1)\} such that t==1Njβ1(1β)/(N1)t=\sum_{\ell=1}^\N j_\ell\beta^{\ell-1}(1-\beta)/(N-1) is called a code of tt. Let Uβ,±N\mathcal{U}_{\beta,\pm N} be the set of t[1,1]t\in[-1,1] having a unique code, and let Sβ,±N\mathcal{S}_{\beta,\pm N} be the set of tUβ,±Nt\in\mathcal{U}_{\beta,\pm N} which make the intersection Γβ,N(Γβ,N+t)\Gamma_{\beta,N}\cap(\Gamma_{\beta,N}+t) a self-similar set. We characterize the set Uβ,±N\mathcal{U}_{\beta,\pm N} in a geometrical and algebraical way, and give a sufficient and necessary condition for tSβ,±Nt\in\mathcal{S}_{\beta,\pm N}. Using techniques from beta-expansions, we show that there is a critical point βc(1/(2N1),1/N)\beta_c\in(1/(2N-1),1/N), which is a transcendental number, such that Uβ,±N\mathcal{U}_{\beta,\pm N} has positive Hausdorff dimension if β(1/(2N1),βc)\beta\in(1/(2N-1),\beta_c), and contains countably infinite many elements if β(βc,1/N)\beta\in(\beta_c,1/N). Moreover, there exists a second critical point αc=[N+1(N1)(N+3)]/2(1/(2N1),βc)\alpha_c=\big[N+1-\sqrt{(N-1)(N+3)}\,\big]/2\in(1/(2N-1),\beta_c) such that Sβ,±N\mathcal{S}_{\beta,\pm N} has positive Hausdorff dimension if β(1/(2N1),αc)\beta\in(1/(2N-1),\alpha_c), and contains countably infinite many elements if β[αc,1/N)\beta\in[\alpha_c,1/N).Comment: 23 pages, 4 figure
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