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661por Wilson, Derrek J., Summers, Adam M., Zigo, Stefan, Davis, Brandin, Robatjazi, Seyyed-Javad, Powell, Jeffery A., Rolles, Daniel, Rudenko, Artem, Trallero-Herrero, Carlos A.“…When focused, this source can ionize gas targets, which we demonstrate here through the ionization of atomic xenon at wavelengths ranging from 5 μm to 9 μm. This opens up new opportunities for fundamental atomic and molecular physics, enabling experimental tests of strong-field ionization theories in the extreme long-wavelength, few-cycle limit and the direct excitation of vibrational transitions in organic molecules.…”
Publicado 2019
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662por Asmar, Meena, Asmar, Ali, Simonsen, Lene, Dela, Flemming, Holst, Jens Juul, Bülow, Jens“…Subcutaneous abdominal adipose tissue blood flow (ATBF) was measured by the (133)Xenon clearance technique, and microvascular blood volume was determined by contrast-enhanced ultrasound imaging. …”
Publicado 2019
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663“…Medical gases include common gases, such as oxygen, hydrogen and carbon dioxide; hydrogen sulphide and nitric oxide that have been considered toxic; volatile anesthetic gases, such as isoflurane and sevoflurane; and inert gases like helium, argon, and xenon. The neuroprotection from these medical gases has been investigated in experimental animal models of various types of brain injuries, such as traumatic brain injury, stroke, subarachnoid hemorrhage, cerebral ischemic/reperfusion injury, and neurodegenerative diseases. …”
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664por Qin, Wenjing, Hong, Mengqing, Wang, Yongqiang, Tang, Jun, Cai, Guangxu, Yin, Ran, Ruan, Xuefeng, Yang, Bing, Jiang, Changzhong, Ren, Feng“…Two kinds of composite ceramics with different grain sizes were prepared by spark plasma sintering (SPS), and their radiation damage behaviors were evaluated by helium (He) and xenon (Xe) ion irradiation. It was found that these dual-phase composite ceramics had better radiation tolerance than the pure yttria-stabilized ZrO(2) (YSZ) and MgO. …”
Publicado 2019
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665por Casini, Beatrice, Tuvo, Benedetta, Cristina, Maria Luisa, Spagnolo, Anna Maria, Totaro, Michele, Baggiani, Angelo, Privitera, Gaetano Pierpaolo“…The effect of an enhanced strategy for terminal room disinfection, applying the pulsed xenon-based ultraviolet light no-touch disinfection systems (PX-UVC) after the current standard operating protocol (SOP) was evaluated. …”
Publicado 2019
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666“…In addition, the dyed polyamide 6 fabric was pH-sensitive, despite dye degradation under xenon light, regardless of whether it was finished.…”
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667por Esteve Bosch, Raúl, Toledo Alarcón, José F., Herrero Bosch, Vicente, Simón Estévez, Ander, Monrabal Capilla, Francesc, Álvarez Puerta, Vicente, Rodríguez Samaniego, Javier, Querol Segura, Marc, Ballester Merelo, Francisco“…This article describes the event detection system of the NEXT-White detector, a 5 kg high pressure xenon TPC with electroluminescent amplification, located in the Laboratorio Subterráneo de Canfranc (LSC), Spain. …”
Publicado 2021
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668“…Consequently, a remarkable anticancer PDT effect was achieved using HA-es-ZnPP and a xenon light source, without apparent side effects. …”
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669“…TTM at 33 or 36°C and adrenaline (epinephrine) are studied most, followed by xenon, erythropoietin, and calcium antagonists. Lack of efficacy is associated with heterogeneity of patient groups and limited specificity of outcome measures. …”
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670“…Concretely, the atomic ionizations induced by mllicharged dark matter particles and millicharged neutrinos in high-purity germanium (HPGe) and liquid xenon (LXe) detectors are carefully studied in this work. …”
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671“…[Image: see text] We report the results of inelastic differential scattering experiments and full-dimensional molecular dynamics trajectory simulations for 2.76 eV H atoms colliding at a surface of solid xenon. The interaction potential is based on an effective medium theory (EMT) fit to density functional theory (DFT) energies. …”
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672“…The left eyes of Sprague–Dawley albino rats (6-weeks old, n = 6 for each wavelength) were exposed to seven narrow-band wavelengths (central wavelengths, 421, 441, 459, 501, 541, 581, and 615 nm) with bandwidths of 16 to 29 nm (half bandwidth, ±8–14.5 nm) using a xenon lamp source with bandpass filters at the retinal radiant exposures of 340 and 680 J/cm(2). …”
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673“…It is shown that the sheath characteristics, viz. the particle number densities, the electrostatic potential and the space charge density profile in the sheath all depend on the [Formula: see text] concentration that is gradually added to the argon-xenon plasma as the third positive ion species. Also, the effect of ion-neutral collisions on the sheath properties is investigated numerically. …”
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674“…The photocatalytic performance was determines by the degradation of bisphenol A (BPA) under xenon lamp illumination. The Bi(7)O(9)I(3) catalyst exhibited superior photocatalytic performance and the first-order kinetic rate constant of Bi(7)O(9)I(3) was about 4.2 times greater than that of BiOI. …”
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675por Alshammari, Basheer A., Alothman, Othman Y., Alhamidi, Abdullah, Jawaid, Mohammad, Shaikh, Hamid M.“…These biocomposites were then subjected to UV exposure (Xenon arch source) for accelerated weathering for 250 and 500 h according to a standard method. …”
Publicado 2022
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676“…Interestingly, the CsPbX(3)/ZnO heterostructure as a photocatalyst has a homogeneous geometry and possesses an excellent degradation efficiency of over 50% under xenon UV-Visible light. The CsPbX(3)/ZnO catalyst carries superior oxidation/reduction properties and ionic conductivity due to the synergistic photogenerated charge carrier and interaction between CsPbX(3) and ZnO. …”
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677por Huang, Shiyong, Ng, Zhi Kai, Li, Hongling, Chaturvedi, Apoorva, Lim, Jian Wei Mark, Tay, Roland Yingjie, Teo, Edwin Hang Tong, Xu, Shuyan, Ostrikov, Kostya (Ken), Tsang, Siu Hon“…The resistance of BNNS to high-energy ions was tested by immersing the samples into the plasma plume at the anode of a 150 W Hall Effect Thruster with BNNS films facing Xenon ions, revealing that the etching rate of BNNS is 20 times less than for a single-crystalline silicon wafer. …”
Publicado 2022
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678por Bagnaschi, E., Sakurai, K., Borsato, M., Buchmueller, O., Citron, M., Costa, J.C., De Roeck, A., Dolan, M.J., Ellis, J.R., Flächer, H., Heinemeyer, S., Lucio, M., Martínez Santos, D., Olive, K.A., Richards, A., Spanos, V.C., Suárez Fernández, I., Weiglein, G.“…We use MasterCode to perform a frequentist analysis of the constraints on a phenomenological MSSM model with 11 parameters, the pMSSM11, including constraints from $\sim 36$ /fb of LHC data at 13 TeV and PICO, XENON1T and PandaX-II searches for dark matter scattering, as well as previous accelerator and astrophysical measurements, presenting fits both with and without the $(g-2)_\mu $ constraint. …”
Publicado 2017
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679por Aprile, E., Abe, K., Agostini, F., Ahmed Maouloud, S., Alfonsi, M., Althueser, L., Angelino, E., Angevaare, J. R., Antochi, V. C., Antón Martin, D., Arneodo, F., Baudis, L., Baxter, A. L., Bellagamba, L., Biondi, R., Bismark, A., Brown, A., Bruenner, S., Bruno, G., Budnik, R., Capelli, C., Cardoso, J. M. R., Cichon, D., Cimmino, B., Clark, M., Colijn, A. P., Conrad, J., Cuenca-García, J. J., Cussonneau, J. P., D’Andrea, V., Decowski, M. P., Gangi, P. Di, Pede, S. Di, Giovanni, A. Di, Stefano, R. Di, Diglio, S., Elykov, A., Farrell, S., Ferella, A. D., Fischer, H., Fulgione, W., Gaemers, P., Gaior, R., Galloway, M., Gao, F., Glade-Beucke, R., Grandi, L., Grigat, J., Higuera, A., Hils, C., Hiraide, K., Hoetzsch, L., Howlett, J., Iacovacci, M., Itow, Y., Jakob, J., Joerg, F., Kato, N., Kavrigin, P., Kazama, S., Kobayashi, M., Koltman, G., Kopec, A., Landsman, H., Lang, R. F., Levinson, L., Li, I., Liang, S., Lindemann, S., Lindner, M., Liu, K., Lombardi, F., Long, J., Lopes, J. A. M., Ma, Y., Macolino, C., Mahlstedt, J., Mancuso, A., Manenti, L., Manfredini, A., Marignetti, F., Marrodán Undagoitia, T., Martens, K., Masbou, J., Masson, D., Masson, E., Mastroianni, S., Messina, M., Miuchi, K., Mizukoshi, K., Molinario, A., Moriyama, S., Morå, K., Mosbacher, Y., Murra, M., Ni, K., Oberlack, U., Palacio, J., Peres, R., Pienaar, J., Pierre, M., Pizzella, V., Plante, G., Qi, J., Qin, J., Ramírez García, D., Reichard, S., Rocchetti, A., Rupp, N., Sanchez, L., dos Santos, J. M. F., Sartorelli, G., Schreiner, J., Schulte, D., Schulze Eißing, H., Schumann, M., Lavina, L. Scotto, Selvi, M., Semeria, F., Shagin, P., Shockley, E., Silva, M., Simgen, H., Takeda, A., Tan, P. L., Terliuk, A., Therreau, C., Thers, D., Toschi, F., Trinchero, G., Tunnell, C., Tönnies, F., Valerius, K., Volta, G., Wei, Y., Weinheimer, C., Weiss, M., Wenz, D., Westermann, J., Wittweg, C., Wolf, T., Xu, Z., Yamashita, M., Yang, L., Ye, J., Yuan, L., Zavattini, G., Zhang, Y., Zhong, M., Zhu, T., Zopounidis, J. P., Laubenstein, M., Nisi, S.“…Screening results, used as inputs for a XENONnT Monte Carlo simulation, predict a reduction of materials background ([Formula: see text] 17%) with respect to its predecessor XENON1T. Through radon emanation measurements, the expected [Formula: see text] Rn activity concentration in XENONnT is determined to be 4.2 ([Formula: see text]) [Formula: see text] Bq/kg, a factor three lower with respect to XENON1T. …”
Publicado 2022
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680por Cwetanski, Peter“…The argon-based acceptance gas mixture as well as two xenon-based operating gases are examined for its properties. …”
Publicado 2006
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