1,881 research outputs found

    Polycation-siRNA nanoparticles can disassemble at the kidney glomerular basement membrane

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    Despite being engineered to avoid renal clearance, many cationic polymer (polycation)-based siRNA nanoparticles that are used for systemic delivery are rapidly eliminated from the circulation. Here, we show that a component of the renal filtration barrier—the glomerular basement membrane (GBM)—can disassemble cationic cyclodextrin-containing polymer (CDP)-based siRNA nanoparticles and, thereby, facilitate their rapid elimination from circulation. Using confocal and electron microscopies, positron emission tomography, and compartment modeling, we demonstrate that siRNA nanoparticles, but not free siRNA, accumulate and disassemble in the GBM. We also confirm that the siRNA nanoparticles do not disassemble in blood plasma in vitro and in vivo. This clearance mechanism may affect any nanoparticles that assemble primarily by electrostatic interactions between cationic delivery components and anionic nucleic acids (or other therapeutic entities)

    Fast Purcell-enhanced single photon source in 1,550-nm telecom band from a resonant quantum dot-cavity coupling

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    High-bit-rate nanocavity-based single photon sources in the 1,550-nm telecom band are challenges facing the development of fibre-based long-haul quantum communication networks. Here we report a very fast single photon source in the 1,550-nm telecom band, which is achieved by a large Purcell enhancement that results from the coupling of a single InAs quantum dot and an InP photonic crystal nanocavity. At a resonance, the spontaneous emission rate was enhanced by a factor of 5 resulting a record fast emission lifetime of 0.2 ns at 1,550 nm. We also demonstrate that this emission exhibits an enhanced anti-bunching dip. This is the first realization of nanocavity-enhanced single photon emitters in the 1,550-nm telecom band. This coupled quantum dot cavity system in the telecom band thus provides a bright high-bit-rate non-classical single photon source that offers appealing novel opportunities for the development of a long-haul quantum telecommunication system via optical fibres.Comment: 16 pages, 4 figure

    Measurement of the double-\beta decay half-life of ^{136}Xe with the KamLAND-Zen experiment

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    We present results from the KamLAND-Zen double-beta decay experiment based on an exposure of 77.6 days with 129 kg of 136^{136}Xe. The measured two-neutrino double-beta decay half-life of 136^{136}Xe is T1/22ν=2.38±0.02(stat)±0.14(syst)×1021T_{1/2}^{2\nu} = 2.38 \pm 0.02(stat) \pm 0.14(syst) \times 10^{21} yr, consistent with a recent measurement by EXO-200. We also obtain a lower limit for the neutrinoless double-beta decay half-life, T1/20ν>5.7×1024T_{1/2}^{0\nu} > 5.7 \times 10^{24} yr at 90% confidence level (C.L.), which corresponds to almost a five-fold improvement over previous limits.Comment: 6 pages, 4 figures. Version as published in PR

    Study of electron anti-neutrinos associated with gamma-ray bursts using KamLAND

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    We search for electron anti-neutrinos (ν‾e\overline{\nu}_e) from long and short-duration gamma-ray bursts~(GRBs) using data taken by the KamLAND detector from August 2002 to June 2013. No statistically significant excess over the background level is found. We place the tightest upper limits on ν‾e\overline{\nu}_e fluence from GRBs below 7 MeV and place first constraints on the relation between ν‾e\overline{\nu}_e luminosity and effective temperature.Comment: 16 pages and 5 figure

    A compact ultra-clean system for deploying radioactive sources inside the KamLAND detector

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    We describe a compact, ultra-clean device used to deploy radioactive sources along the vertical axis of the KamLAND liquid-scintillator neutrino detector for purposes of calibration. The device worked by paying out and reeling in precise lengths of a hanging, small-gauge wire rope (cable); an assortment of interchangeable radioactive sources could be attached to a weight at the end of the cable. All components exposed to the radiopure liquid scintillator were made of chemically compatible UHV-cleaned materials, primarily stainless steel, in order to avoid contaminating or degrading the scintillator. To prevent radon intrusion, the apparatus was enclosed in a hermetically sealed housing inside a glove box, and both volumes were regularly flushed with purified nitrogen gas. An infrared camera attached to the side of the housing permitted real-time visual monitoring of the cable's motion, and the system was controlled via a graphical user interface.Comment: Revised author affiliations, corrected typos, made minor improvements to text, and revised reference

    Search for extraterrestrial antineutrino sources with the KamLAND detector

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    We present the results of a search for extraterrestrial electron antineutrinos (νˉe\bar{\nu}_{e}'s) in the energy range 8.3MeV<Eνˉe<31.8MeV8.3 MeV < E_{\bar{\nu}_{e}} < 31.8 MeV using the KamLAND detector. In an exposure of 4.53 kton-year, we identify 25 candidate events. All of the candidate events can be attributed to background, most importantly neutral current atmospheric neutrino interactions, setting an upper limit on the probability of 8^{8}B solar νe\nu_{e}'s converting into νˉe\bar{\nu}_{e}'s at 5.3×10−55.3 \times 10^{-5} (90% C.L.), if we assume an undistorted νˉe\bar{\nu}_{e} shape. This limit corresponds to a solar νˉe\bar{\nu}_{e} flux of 93cm−2s−193 cm^{-2} s^{-1} or an event rate of 1.6events(kton−year)−11.6 events (kton-year)^{-1} above the energy threshold (Eνˉe>8.3MeV)(E_{\bar{\nu}_{e}} > 8.3 MeV). The present data also allows us to set more stringent limits on the diffuse supernova neutrino flux and on the annihilation rates for light dark matter particles.Comment: 22 pages, 6 figure
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