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    25 December 2016, Volume 38 Issue 6
    Brief Introduction of Nobel Prize
    2016 Nobel Prize in Physics: Theoretical discoveries in topological phase transitions and topological phases of matter
    SHI Yu
    2016, 38(6):  414-419.  doi:10.3969/j.issn.0253-9608.2016.06.004
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    A popular accurate introduction is made for the prize-winning work and related background knowledge for 2016 Nobel Prize in Physics. The historical development leading to these theoretical discoveries and the careers of the three Nobel Laureates are also investigated. The paper is concluded with the implications of these achievements as well as the lessons we can learn.

    The tiniest machine in the world: A brief introduction to the Nobel Prize in Chemistry 2016
    GU Jun, SUN Yuren, GONG Hegui
    2016, 38(6):  420-428.  doi:10.3969/j.issn.0253-9608.2016.06.005
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    The Royal Swedish Academy of Sciences decided to award Jean-Pierre Sauvage, J. Fraser Stoddart and Bernard L. Feringa the Nobel Prize in Chemistry 2016 for the design and synthesis of the molecular machines. In this article, we mainly introduced the concept of molecular machine and the achievement of the three scientists. Finally, the current problems and the challenges for future research were presented in this new field.

    Progress
    A great eruption of Tambora mystery: Insights from the Tibetan eclogites
    LIU Yan, YUAN Tingyuan, WU Liandong
    2016, 38(6):  429-435.  doi:10.3969/j.issn.0253-9608.2016.06.006
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    Songduo eclogites within the Tibetan regions are typical products of subduction of ancient oceanic crust, and thus studied in details in this paper. Petrographic observations and thermodynamic calculation confirm that the Songduo eclogites have experienced reduction reaction during the oceanic subdution. Fe3+ and S6+ were reduced to Fe2+ and S2- , respectively, releasing the fluids enriched in CO2 and H2S in the subduction channel. The CO2 and H2S-rich fluids were subsequently transferred into the overlying mantle wedge, and partially released into the atmosphere through the arc volcanoes. Therefore, it is regarded that the currently deep subduction of India oceanic crust experienced similar reduction reactions in deep earth. The sulfur is liberated from the buried surface
    sulphates into the sulfur-bearing fluids, and released into the atmosphere through the Tambora-like volcanoes. Today, the oceanic subduction and reduction reactions continued, and then, the newly-formed sulfur-bearing fluids continuously sunk in the magma chambers beneath the island arc volcanoes. Therefore, the tambora-like volcanic eruption is a high probability event happening in the near future.

    In-situ study on the hydrothermal synthesis mechanisms for nanopowders
    ZHANG Liangmiao①, LUO Hongjie①②, GAO Yanfeng①
    2016, 38(6):  436-447.  doi:10.3969/j.issn.0253-9608.2016.06.007
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    Hydrothermal synthesis has many unique advantages in the preparation of nanopowders. But the reaction mechanisms and kinetics have not been clearly understood because the reaction was generally occurred in a sealed vessel. In-situ techniques can be used to collect information about the precursors, phase evolution, the fate of the transient intermediates and better understand the nucleation, crystallization and growth by monitoring the whole reaction process in real time. Thus the controlled synthesis of materials can be achieved. This review summarizes the in-situ techniques, in-situ reactors and their applications in understanding the hydrothermal formation mechanisms of nanopowders. These in-situ techniques include synchrotron energy dispersive X-ray diffraction (EDXRD), angular dispersive X-ray diffraction (ADXRD), X-ray absorption fine structure (XAFS), small-angle X-ray scattering (SAXS), neutron powder diffraction (NPD), small-angle neutron scattering (SANS) and several selected spectroscopic methods (UV-Vis, Raman, FTIR).

    Science Review
    Winners of sciences
    GUAN Yi
    2016, 38(6):  448-455.  doi:10.3969/j.issn.0253-9608.2016.06.008
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    Natural Forum
    Will our sun become a black hole
    ZHANG Tianrong
    2016, 38(6):  456-460.  doi:10.3969/j.issn.0253-9608.2016.06.009
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    Will our sun become a black hole? No. Stars like the Sun just are not massive enough to become black hole. Instead, in several billion years, the Sun will cast off its outer layer, and its core will form a white dwarf, a dense ball of carbon and oxygen that no longer produces nuclear energy, which still shines because it is very hot. A typical white dwarf is about as massive as the Sun, but only as big as the Earth, which is one percent of the Sun’s present diameter.

    Portraits
    Founder of modern human anatomy—Andreas Vesalius
    GU Fanji
    2016, 38(6):  461-466.  doi:10.3969/j.issn.0253-9608.2016.06.010
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