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首页> 外文期刊>Physics and Chemistry of Minerals >The high-pressure phase diagram of synthetic epsomite (MgSO4·7H2O and MgSO4·7D2O) from ultrasonic and neutron powder diffraction measurements
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The high-pressure phase diagram of synthetic epsomite (MgSO4·7H2O and MgSO4·7D2O) from ultrasonic and neutron powder diffraction measurements

机译:超声和中子粉末衍射测量合成eps石(MgSO4·7H2O和MgSO4·7D2O)的高压相图

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We present an ultrasonic and neutron powder diffraction study of crystalline MgSO4·7H2O (synthetic epsomite) and MgSO4·7D2O under pressure up to ~3 GPa near room temperature and up to ~2 GPa at lower temperatures. Both methods provide complementary data on the phase transitions and elasticity of magnesium sulphate heptahydrate, where protonated and deuterated counterparts exhibit very similar behaviour and properties. Under compression in the declared pressure intervals, we observed three different sequences of phase transitions: between 280 and 295 K, phase transitions occurred at approximately 1.4, 1.6, and 2.5 GPa; between 240 and 280 K, only a single phase transition occurred; below 240 K, there were no phase transformations. Overall, we have identified four new phase fields at high pressure, in addition to that of the room-pressure orthorhombic structure. Of these, we present neutron powder diffraction data obtained in situ in the three phase fields observed near room temperature. We present evidence that these high-pressure phase fields correspond to regions where MgSO4·7H2O decomposes to a lower hydrate by exsolving water. Upon cooling to liquid nitrogen temperatures, the ratio of shear modulus G to bulk modulus B increases and we observe elastic softening of both moduli with pressure, which may be a precursor to pressure-induced amorphization. These observations may have important consequences for modelling the interiors of icy planetary bodies in which hydrated sulphates are important rock-forming minerals, such as the large icy moons of Jupiter, influencing their internal structure, dynamics, and potential for supporting life.
机译:我们目前对晶体MgSO4·7H2O(合成次泻岩)和MgSO4·7D2O的超声和中子粉末衍射研究在室温下约〜3 GPa和在低温下约〜2 GPa的压力下进行。两种方法都提供了有关七水合硫酸镁的相变和弹性的补充数据,其中质子化和氘代的对应物表现出非常相似的行为和性质。在声明的压力间隔内压缩下,我们观察到三个不同的相变序列:在280和295K之间,相变发生在大约1.4、1.6和2.5GPa处;在240至280 K之间,仅发生了单相转变;低于240 K,则没有相变。总的来说,除了常压正交晶系结构外,我们还确定了四个新的高压相场。其中,我们提供了在室温附近观察到的三相场中原位获得的中子粉末衍射数据。我们提供的证据表明,这些高压相场对应于其中MgSO4·7H2O通过溶解水分解为较低水合物的区域。冷却至液氮温度后,剪切模量G与体积模量B的比率增加,并且我们观察到两个模量随压力的弹性软化,这可能是压力诱导非晶化的先兆。这些观察结果可能对冰质行星体内的建模具有重要的意义,其中水合硫酸盐是重要的岩石形成矿物,例如木星的大型冰质卫星,影响其内部结构,动力和维持生命的潜力。

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