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  • 1
    Publication Date: 2016-02-20
    Description: Despite wide studies of Na 0.5 Bi 0.5 TiO 3 , structure of this material and its connection with the observed physical properties still raise numerous questions due to mutually contradicting results obtained. Here, structure and dielectric properties of poled and unpoled Na 0.5 Bi 0.5 TiO 3 -CaTiO 3 solid solutions are studied, projecting the obtained concentration dependence of structure and dielectric properties on pure Na 0.5 Bi 0.5 TiO 3 as the end member of this material group. X-ray diffraction patterns for Na 0.5 Bi 0.5 TiO 3 -CaTiO 3 solid solutions reveal dominating of an orthorhombic Pnma phase, even for the compositions approaching the end composition (Na 0.5 Bi 0.5 TiO 3 ), whereas structure of pure Na 0.5 Bi 0.5 TiO 3 can be considered, assuming coexistence of rhombohedral and orthorhombic phases. This allows one to avoid appearance of a large difference of rhombohedral distortions between the unpoled and poled Na 0.5 Bi 0.5 TiO 3 , if the rhombohedral distortion is calculated as for single R3c phase. Features of dielectric permittivity, corresponding to the observed structural phase transition, are identified. It is discussed that the rhombohedral R3c phase is responsible for appearance of the frequency-dependent shoulder of dielectric permittivity temperature dependence, characteristic for unpoled Na 0.5 Bi 0.5 TiO 3 .
    Print ISSN: 0021-8979
    Electronic ISSN: 1089-7550
    Topics: Physics
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  • 2
    Publication Date: 2010-02-12
    Description: Stars form from cold molecular interstellar gas. As this is relatively rare in the local Universe, galaxies like the Milky Way form only a few new stars per year. Typical massive galaxies in the distant Universe formed stars an order of magnitude more rapidly. Unless star formation was significantly more efficient, this difference suggests that young galaxies were much more molecular-gas rich. Molecular gas observations in the distant Universe have so far largely been restricted to very luminous, rare objects, including mergers and quasars, and accordingly we do not yet have a clear idea about the gas content of more normal (albeit massive) galaxies. Here we report the results of a survey of molecular gas in samples of typical massive-star-forming galaxies at mean redshifts 〈z〉 of about 1.2 and 2.3, when the Universe was respectively 40% and 24% of its current age. Our measurements reveal that distant star forming galaxies were indeed gas rich, and that the star formation efficiency is not strongly dependent on cosmic epoch. The average fraction of cold gas relative to total galaxy baryonic mass at z = 2.3 and z = 1.2 is respectively about 44% and 34%, three to ten times higher than in today's massive spiral galaxies. The slow decrease between z approximately 2 and z approximately 1 probably requires a mechanism of semi-continuous replenishment of fresh gas to the young galaxies.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Tacconi, L J -- Genzel, R -- Neri, R -- Cox, P -- Cooper, M C -- Shapiro, K -- Bolatto, A -- Bouche, N -- Bournaud, F -- Burkert, A -- Combes, F -- Comerford, J -- Davis, M -- Schreiber, N M Forster -- Garcia-Burillo, S -- Gracia-Carpio, J -- Lutz, D -- Naab, T -- Omont, A -- Shapley, A -- Sternberg, A -- Weiner, B -- England -- Nature. 2010 Feb 11;463(7282):781-4. doi: 10.1038/nature08773.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Max-Planck-Institut fur extraterrestrische Physik (MPE), Giessenbachstr. 1, 85748 Garching, Germany. linda@mpe.mpg.de〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/20148033" target="_blank"〉PubMed〈/a〉
    Print ISSN: 0028-0836
    Electronic ISSN: 1476-4687
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
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  • 3
    Electronic Resource
    Electronic Resource
    [S.l.] : American Institute of Physics (AIP)
    Journal of Applied Physics 76 (1994), S. 4301-4304 
    ISSN: 1089-7550
    Source: AIP Digital Archive
    Topics: Physics
    Notes: Results of measurements in situ of electrostrictive strain, dielectric polarization, dielectric constant, and crystallographic parameters as functions of applied electric field in the temperature range 20–200 °C of Pb0.97La0.02(Zr0.66Ti0.11Sn0.23)O3 composition are reported. The antiferroelectric to ferroelectric phase transition with large volume change ΔV=0.35 A(ring)3 is shown to be the dominant mechanism of the field-induced strain. The microscopic nature of the switching mechanism and the variation of the strain versus polarization squared at various temperatures are discussed.
    Type of Medium: Electronic Resource
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