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441por Badziak, Marcin, Delgado, Antonio, Olechowski, Marek, Pokorski, Stefan, Sakurai, Kazuki“…The second general conclusion is that the bound $\Omega_\chi h^2\leq 0.12$ together with the LUX (XENON1T) limits for the neutralino spin independent scattering cross sections constrain the electroweakino spectrum so that the mass differences between the NLSP and the LSP are smaller than 40 (10) GeV, respectively, with important implications for the collider searches. …”
Publicado 2015
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442por Glorieux, Maximilien, Evans, Adrian, Lange, Thomas, In, A-Duong, Alexandrescu, Dan, Boatella-Polo, Cesar, Garcia Alía, Rubén, Tali, Maris, Urbina Ortega, Carlos, Kastriotou, Maria, Fernández-Martínez, Pablo, Ferlet-Cavrois, Véronique“…Additionally, irradiation with a ultra high energy xenon beam shows similar upset sensitivity.…”
Publicado 2018
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443“…More specifically, the performances of the headlights containing halogen, xenon, and LED light sources in dark and foggy weather conditions are examined and the performance of each headlight is evaluated separately. …”
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444“…In the case of a high-power signal input, as xenon-gas breakdown occurred, the transmitted signal was close to zero, and most of the high-power signal was reflected with a blocking efficiency of 40.55 dB. …”
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445“…Similar to Tc-99m-DTPA and unlike Xenon-133, Tc-99m-HDP allowed direct comparison of all 8 ventilation-perfusion images. …”
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446“…We report on the aromatic noble-gas hydride, C(6)H(5)CCXeH, identified in a xenon matrix using infrared spectroscopy and extensive quantum chemical calculations. …”
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447por Poodproh, Rattawan, Kaewmeechai, Supavadee, Leelawatwattana, Ladda, Prapunpoj, Porntip“…The binding dissociation constant (K (d)) values of pigC/huTTR, xenoN/pigC/huTTR and pigC/crocTTR were 3.20 ± 0.35, 1.53 ± 0.38 and 0.31 ± 0.04 μm, respectively, and the K (d) values of human and C. porosus TTR were 4.92 ± 0.68 and 1.42 ± 0.45 μm, respectively. …”
Publicado 2017
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448“…Compared to xenon, Argon, as a noble gas, is abundant, cheap and widely applicable, and has been also demonstrated to be neuroprotective in many research studies. …”
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449“…This article combines theory and experiment to highlight the importance of non-covalent NgBs in the solid state of several xenon fluorides [XeF(n)](m+) were the central oxidation state of Xe varies from +2 to +6 and the number of fluorine atoms varies from n = 2 to 6. …”
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450por Austin, Dane R., Johnson, Allan S., McGrath, Felicity, Wood, David, Miseikis, Lukas, Siegel, Thomas, Hawkins, Peter, Harvey, Alex, Mašín, Zdeněk, Patchkovskii, Serguei, Vacher, Morgane, Malhado, João Pedro, Ivanov, Misha Y., Smirnova, Olga, Marangos, Jon P.“…The method is applied to xenon atoms and to benzene molecules, the latter exhibiting significant fast nuclear dynamics following ionization. …”
Publicado 2021
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451por Zhang, Jiongshan, Liu, Wei, Bi, Mingmin, Xu, Jinwen, Yang, Hongzhi, Zhang, Yaxing“…Mechanistically, besides the competitive inhibition of N-methyl-D-aspartate (NMDA) receptor in nervous system by xenon, the key and common mechanisms of noble gases are involved in modulation of cell death and inflammatory or immune signals. …”
Publicado 2022
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452por Pitt, Michael“…Therefore, the work has been divided into detector development activities towards applications at the future International Linear Collider (ILC) as well as to data analysis related to two front-edge topics: the search for the Higgs boson (within CERN-ATLAS detector) and for Dark matter (within XENON100).…”
Publicado 2015
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453por Collective“…The objective of the Light Detection in Noble Elements (LIDINE) 2015 conference is to promote discussion between the members of the particle and nuclear physics communities about light and charge collection in detectors based on liquid or gaseous noble elements, xenon and argon being the most common, but neon and helium also in use, and represented at this conference. …”
Publicado 2016
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454“…A recent global fit to the CMSSM incorporating current constraints on supersymmetry, including missing transverse energy searches at the LHC, BR(B_s to mu+ mu-) and the direct XENON100 search for dark matter, favours points towards the end of the stau-neutralino (stau_1- chi) coannihilation strip with relatively large m_1/2 and 10 < tan beta < 40 and points in the H/A rapid-annihilation funnel with tan beta ~ 50. …”
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455“…We find that future LHC searches for generic missing $E_T$, charginos and stops will be able to constrain the different GUT models in complementary ways, as will the Xenon 1 ton and Darwin dark matter scattering experiments and future FERMI or CTA $\gamma$-ray searches.…”
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456por Krasnopevtsev, Dimitriy“…The performance of the TRT, operating with different gas mixtures (Xenon-based and Argon-based) and for high track multiplicities is presented. …”
Publicado 2016
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457por Mohanty, Subhendra“…Cosmology and astroparticle physics have seen an avalanche of discoveries in the past decade (IceCube - high energy neutrinos, LIGO - gravitational waves, Fermi- gamma-ray telescope, Xenon-1T - dark matter detection, PLANCK- cosmic microwave radiation, EHT picture of black hole, SDSS -galaxy surveys), all of which require a multidisciplinary background for analyzing the phenomena. …”
Publicado 2020
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458por Borschensky, Christoph“…Detailed phenomenological studies illustrate the complementary reach of collider searches for Dark Matter and the direct detection experiments CRESST and XENON. In the case of cancellation effects in the tree-level contributions, one-loop corrections can have a particularly large impact on exclusion limits in the case of combined $s + t$-channel models.…”
Publicado 2021
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459“…The results are compared with other experimental data known in light odd-mass xenon isotopes and with calculations performed in the frame of the multi-shell interacting boson-fermion model.…”
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460por Hardy, J C“…Overall, the 'gross theory' beta -strength functions are remarkably reliable, although some systematic deviations are observed in the xenon and tellurium isotopes. (30 refs).…”
Publicado 1981
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