46,275 research outputs found

    On unusual narrow transmission bands for a multi-layered periodic structure containing left-handed materials

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    A multi-layered structure consisting of alternate right-handed material (RHM) and left-handed material (LHM)is considered and the unusual narrow transmission bands are explained as the competitive results of the Bragg condition and the transparent condition. These unusual narrow transmission bands may exist regardless whether the optical length of the LHM layer cancels the optical length of the RHM layer or not. This unusual transmission property may disappear when the reflection coefficient for each interface is small and the optical length of the LHM layer does not cancel the optical length of the RHM layer. An non-ideal model when the LHM is dispersive and lossy is also employed to confirm the unusual transmission phenomenon.Comment: 9 pages, 4 figure

    Unusual behavior of sound velocity of a Bose gas in an optical superlattice at quasi-one-dimension

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    A Bose gas trapped in a one-dimensional optical superlattice has emerged as a novel superfluid characterized by tunable lattice topologies and tailored band structures. In this work, we focus on the propagation of sound in such a novel system and have found new features on sound velocity, which arises from the interplay between the two lattices with different periodicity and is not present in the case of a condensate in a monochromatic optical lattice. Particularly, this is the first time that the sound velocity is found to first increase and then decrease as the superlattice strength increases even at one dimension. Such unusual behavior can be analytically understood in terms of the competition between the decreasing compressibility and the increasing effective mass due to the increasing superlattice strength. This result suggests a new route to engineer the sound velocity by manipulating the superlattice's parameters. All the calculations based on the mean-field theory are justified by checking the exponent γ\gamma of the off-diagonal one-body density matrix that is much smaller than 1. Finally, the conditions for possible experimental realization of our scenario are also discussed.Comment: 10 pages, 5 figure

    Why are some BL Lacs detected by \fermi, but others not ?

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    By cross-correlating an archival sample of 170 BL Lacs with 2 year \fermilat AGN sample, we have compiled a sample of 100 BL Lacs with \fermi detection (FBLs), and a sample of 70 non-\fermi BL Lacs (NFBLs). We compared various parameters of FBLs with those of NFBLs, including the redshift, the low frequency radio luminosity at 408 MHz (L408MHzL_{\rm 408MHz}), the absolute magnitude of host galaxies (MhostM_{\rm host}), the polarization fraction from NVSS survey (PNVSSP_{\rm NVSS}), the observed arcsecond scale radio core flux at 5 GHz (FcoreF_{\rm core}) and jet Doppler factor; all the parameters are directly \textbf{measured} or derived from available data from literatures. We found that the Doppler factor is on average larger in FBLs than in NFBLs, and the Fermi γFermi~ \gamma-ray detection rate is higher in sources with higher Doppler factor. In contrast, there are no significant differences in terms of the intrinsic parameters of redshift, L408MHz L_{\rm 408MHz}, Mhost M_{\rm host} and PNVSS P_{\rm NVSS}. FBLs seem to have a higher probability of exhibiting measurable proper motion. These results strongly indicate a higher beaming effect in FBLs compared to NFBLs. The radio core flux is found to be strongly correlated with γ\gamma-ray flux, which remains after excluding the common dependence of the Doppler factor. At the fixed Doppler factor, FBLs have systematically larger radio core flux than NFBLs, implying lower γ\gamma-ray emission in NFBLs since the radio and γ\gamma-ray flux are significantly correlated. Our results indicate that the Doppler factor is an important parameter of γ\gamma-ray detection, the non-detection of γ\gamma-ray emission in NFBLs is likely due to low beaming effect, and/or low intrinsic γ\gamma-ray flux, and the gamma-rays are likely produced co-spatially with the arcsecond-scale radio core radiation and mainly through the SSC process.Comment: 6 pages, 6 figures, accepted by A&
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