An arbitrary unknown quantum state cannot be precisely measured or perfectly
replicated. However, quantum teleportation allows faithful transfer of unknown
quantum states from one object to another over long distance, without physical
travelling of the object itself. Long-distance teleportation has been
recognized as a fundamental element in protocols such as large-scale quantum
networks and distributed quantum computation. However, the previous
teleportation experiments between distant locations were limited to a distance
on the order of 100 kilometers, due to photon loss in optical fibres or
terrestrial free-space channels. An outstanding open challenge for a
global-scale "quantum internet" is to significantly extend the range for
teleportation. A promising solution to this problem is exploiting satellite
platform and space-based link, which can conveniently connect two remote points
on the Earth with greatly reduced channel loss because most of the photons'
propagation path is in empty space. Here, we report the first quantum
teleportation of independent single-photon qubits from a ground observatory to
a low Earth orbit satellite - through an up-link channel - with a distance up
to 1400 km. To optimize the link efficiency and overcome the atmospheric
turbulence in the up-link, a series of techniques are developed, including a
compact ultra-bright source of multi-photon entanglement, narrow beam
divergence, high-bandwidth and high-accuracy acquiring, pointing, and tracking
(APT). We demonstrate successful quantum teleportation for six input states in
mutually unbiased bases with an average fidelity of 0.80+/-0.01, well above the
classical limit. This work establishes the first ground-to-satellite up-link
for faithful and ultra-long-distance quantum teleportation, an essential step
toward global-scale quantum internet.Comment: 16 pages, 3 figure
We report the surface exploration by the lunar rover Yutu that landed on the young lava flow in the northeastern part of the Mare Imbrium, which is the largest basin on the nearside of the Moon and is filled with several basalt units estimated to date from 3.5 to 2.0 Ga. The onboard lunar penetrating radar conducted a 114-m-long profile, which measured a thickness of ∼5 m of the lunar regolith layer and detected three underlying basalt units at depths of 195, 215, and 345 m. The radar measurements suggest underestimation of the global lunar regolith thickness by other methods and reveal a vast volume of the last volcano eruption. The in situ spectral reflectance and elemental analysis of the lunar soil at the landing site suggest that the young basalt could be derived from an ilmenite-rich mantle reservoir and then assimilated by 10-20% of the last residual melt of the lunar magma ocean.volcanic history | Imbrium basin | lunar rover Yutu | lunar penetrating radar | Chang'e-3 mission
During the transition period, the extent of corruption in China is higher than before. Meanwhile the forms and characters of Chinese corruption are also different in many important aspects from those of its past and of other countries. This paper explores the causes, consequences of corruption and anti-corruption campaigns of the Chinese government. The major conclusion of this paper is that further political reform toward democracy should be the direction of future anti-corruption efforts.
RNA interference (RNAi) was first literaturally reported in 1998 and has become rapidly a promising tool for therapeutic applications in gene therapy. In a typical RNAi process, small interfering RNAs (siRNA) are used to specifically downregulate the expression of the targeted gene, known as the term “gene silencing.” One key point for successful gene silencing is to employ a safe and efficient siRNA delivery system. In this context, dendrimers are emerging as potential nonviral vectors to deliver siRNA for RNAi purpose. Dendrimers have attracted intense interest since their emanating research in the 1980s and are extensively studied as efficient DNA delivery vectors in gene transfer applications, due to their unique features based on the well-defined and multivalent structures. Knowing that DNA and RNA possess a similar structure in terms of nucleic acid framework and the electronegative nature, one can also use the excellent DNA delivery properties of dendrimers to develop effective siRNA delivery systems. In this review, the development of dendrimer-based siRNA delivery vectors is summarized, focusing on the vector features (siRNA delivery efficiency, cytotoxicity, etc.) of different types of dendrimers and the related investigations on structure-activity relationship to promote safe and efficient siRNA delivery system.
Chang’E-4 landed in the South Pole-Aitken (SPA) basin, providing a unique chance to probe the composition of the lunar interior. Its landing site is located on ejecta strips in Von Kármán crater that possibly originate from the neighboring Finsen crater. A surface rock and the lunar regolith at 10 sites along the rover Yutu-2 track were measured by the onboard Visible and Near-Infrared Imaging Spectrometer in the first three lunar days of mission operations. In situ spectra of the regolith have peak band positions at 1 and 2 μm, similar to the spectral data of Finsen ejecta from the Moon Mineralogy Mapper, which confirms that the regolith's composition of the landing area is mostly similar to that of Finsen ejecta. The rock spectrum shows similar band peak positions, but stronger absorptions, suggesting relatively fresh exposure. The rock may consist of 38.1 ± 5.4% low-Ca pyroxene, 13.9 ± 5.1% olivine and 48.0 ± 3.1% plagioclase, referred to as olivine-norite. The plagioclase-abundant and olivine-poor modal composition of the rock is inconsistent with the origin of the mantle, but representative of the lunar lower crust. Alternatively, the rock crystallized from the impact-derived melt pool formed by the SPA-impact event via mixing the lunar crust and mantle materials. This scenario is consistent with fast-cooling thermal conditions of a shallow melt pool, indicated by the fine to medium-sized texture (<3 mm) of the rock and the SPA-impact melting model [Icarus 2012; 220: 730–43].
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