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Добірка наукової літератури з теми "Polarised-nuclei"

Автор: Grafiati

Опубліковано: 11 березня 2023

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Статті в журналах з теми "Polarised-nuclei"

1

Kudryavtsev, I. N., and A. P. Soznik. "Elastic intermediate-energy proton scattering by polarised nuclei." Journal of Physics G: Nuclear and Particle Physics 15, no. 9 (1989): 1377–95. http://dx.doi.org/10.1088/0954-3899/15/9/008.

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2

Glättli, Hans. "Polarised nuclei for neutron science: recent applications and perspectives." Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 529, no. 1-3 (2004): 194–98. http://dx.doi.org/10.1016/j.nima.2004.04.156.

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3

Lampard, GJ, HH Bolotin, AE Stuchbery, CE Doran, and AP Byrne. "Systematics of Gyromagnetic Ratios of the 21+ States in Even Ge Isotopes." Australian Journal of Physics 40, no. 2 (1987): 117. http://dx.doi.org/10.1071/ph870117.

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The relative gyromagnetic ratios of the 2t states in 70,72,74,76Ge were measured simultaneously by me ns of the thin-foil, perturbed y-r yngular distribution technique utilising the transient hyperfine field manifest t nuclei of Ge ions rapidly traversing polarised Fe. The states of interest were Coulomb excited using 75-MeV 34S projectiles incident upon natural element l Ge t rget. The present results re comp red with previously reported measurements and collective model expectations.

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4

Court, G. R., and W. G. Heyes. "The polarisation of 14N and 15N nuclei in polarised proton targets using irradiated ammonia." Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 243, no. 1 (1986): 37–40. http://dx.doi.org/10.1016/0168-9002(86)90818-1.

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5

O’Connor, Eoin G. P., Andrew Shearer, Christian Gouiffes, and Philippe Laurent. "High Time Resolution Astronomical Polarimetry with GASP." Proceedings of the International Astronomical Union 13, S337 (2017): 384–85. http://dx.doi.org/10.1017/s1743921317010626.

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AbstractThe Galway Astronomical Stokes Polarimeter (GASP) is a high time resolution, full-Stokes imaging polarimeter which utilises a Fresnel rhomb prism as a beam-splitter and quarter wave retarder. The ability to perform optical photometry and polarimetry at high frame rates enables more detailed studies of a multitude of compact objects including; optical pulsars, magnetars and Active Galactic Nuclei (AGN). We present a brief discussion of the instruments’ current capabilities and hardware design. GASP is currently configured with two Electron Multiplying Charge-Coupled Devices (EMCCDs), wh

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6

Shehu, D., G. Marsicano, J. E. Fléchon, and C. Galli. "Developmentally regulated markers of in vitro-produced preimplantation bovine embroys." Zygote 4, no. 2 (1996): 109–21. http://dx.doi.org/10.1017/s0967199400002987.

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SummaryExpression of various developmentally regulated markers was screened throughout the preimplantation stages of in vitro-derived bovine embryos. This was done by investigating the distribution of several nuclear, cytoplasmic and extracellular proteins by means of immunofluorescence microscopy. While lamin B appeared as a constitutive component of nuclei of all preimplantation stages, lamins A/C had a stage-related distribution. The early cleavage stage nuclei contained lamins A/C which generally disappeared in the following stages, with the possible exception of a few positive nuclei in t

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7

KISELEV, J. F., A. F. PRUDKOGLYAD, A. S. SHUMOVSKY, and V. I. YUKALOV. "DISCOVERY OF DICKE SUPERRADIATION BY SYSTEM OF NUCLEAR MAGNETIC MOMENTS." Modern Physics Letters B 01, no. 11n12 (1988): 409–16. http://dx.doi.org/10.1142/s021798498800148x.

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Spontaneous generation of the Dicke superradiation (SR) state has been found in the system of inversely polarised proton spins with “frozen” polarisation. SR is observed at the moment when the Larmor frequency crosses the resonance frequency of the passive oscillatory circuit. SR arises from incoherent maser generation of spins. The frequency of a SR generator can be retuned from several hundreds of kilohertz to hundreds of megahertz at very low temperatures. Dependence of incoherent and coherent radiation on the initial polarisation has been investigated. A radio frequency analogue of the opt

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8

Adebahr, B., M. Brienza, and R. Morganti. "Polarised structures in the radio lobes of B2 0258+35." Astronomy & Astrophysics 622 (February 2019): A209. http://dx.doi.org/10.1051/0004-6361/201833988.

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Context. The contribution of active galactic nuclei to the magnetisation of the Universe can be constrained by knowing their duty cycles, jet and magnetic field morphologies, and the physical processes dominating their interaction with the surrounding environment. Aims. The magnetic field morphology and strength of radio lobes of AGN has an influence on the mechanisms for the propagation of cosmic rays into intergalactic space. Using the source B2 0258+35 we want to investigate the interaction of its radio lobes with the surrounding environment and examine the underlying physical effects. Meth

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9

Catoira, R., A. C. Timmers, F. Maillet, et al. "The HCL gene of Medicago truncatula controls Rhizobium-induced root hair curling." Development 128, no. 9 (2001): 1507–18. http://dx.doi.org/10.1242/dev.128.9.1507.

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The symbiotic infection of the model legume Medicago truncatula by Sinorhizobium meliloti involves marked root hair curling, a stage where entrapment of the microsymbiont occurs in a chamber from which infection thread formation is initiated within the root hair. We have genetically dissected these early symbiotic interactions using both plant and rhizobial mutants and have identified a M. truncatula gene, HCL, which controls root hair curling. S. meliloti Nod factors, which are required for the infection process, induced wild-type epidermal nodulin gene expression and root hair deformation in

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10

Pisano, G., A. Ritacco, A. Monfardini, et al. "Development and application of metamaterial-based half-wave plates for the NIKA and NIKA2 polarimeters." Astronomy & Astrophysics 658 (January 27, 2022): A24. http://dx.doi.org/10.1051/0004-6361/202038643.

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Context. Large field-of-view imaging and polarimetry instruments operating at millimetre and sub-millimetre wavelengths are fundamental tools to understand the role of magnetic fields in channelling filament material into prestellar cores, providing unique insight in the physics of galactic star-forming regions. Among other topics, at extra-galactic scales, polarisation observations of Active Galactic Nuclei (AGNs) will allow us to constrain the possible physical conditions of the emitting plasma from the jets and/or explore the physics of dust inside supernova remnants. The kilo-pixel New IRA

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