Mg3Al2Si3O12火山岩的状态方程:对石榴石后转变和地幔动力学的影响

IF 2.4 3区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS
Anna M. Dymshits , Peter I. Dorogokupets , Igor S. Sharygin , Anton F. Shatskiy
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引用次数: 0

摘要

地幔对流是热物质上涌和冷板块俯冲的主导过程。这些过程具有密度依赖性,并受地幔过渡带(MTZ)/下地幔(LM)中尖晶石和石榴石后转变的影响。这些转换的克拉珀龙斜率的知识用于表达地幔块体的动力学,对于了解地球深部是必要的。本文通过对实验测得的等压热容、体积模量、热膨胀、压力(P)、单胞体积(V)、温度(T)数据的联合分析,给出了Mg3Al2Si3O12 (Prp)的Kunc-Einstein状态方程(EoS)。基于我们的模型,体积模量及其压力导数为K0,T0 = 168.5 GPa, K ' 0,T = 4.77, V0 = 1501.7 Å。优化后的参数包括两个爱因斯坦温度θ1 = 331和θ2 = 1093 K,环境条件下的gr neisen参数γ0 = 1.77,无限压缩γ∞= 0,β = 1.12,固有非谐性参数a0 = -20。计算得到热膨胀系数为α = 2.33·10−5 K−1,热力学grisen参数为γth = 1.42。得到的Prp的相态图和初步拟合的al - motoite (Al-Aki)的相态图,结合桥菱石(Bdm)和刚玉(Crn)的文献数据,在LM条件下计算了75 mol% MgSiO3 + 25 mol% Al2O3体系的相图。在24 GPa和1570 K条件下,Prp向Bdm + Crn转变,Clapeyron斜率略为正(dP/dT = 2.1 MPa/K)。在T = 1250 ~ 1570 K, P = 23 ~ 27 GPa时检测Al-Aki的稳定场。当P值高于24 ~ 27 GPa时,Al-Aki转变为Bdm + Crn组合,具有高度负的Clapeyron斜率。对所研究相的声速计算表明,从Prp到Bdm + Crn的转变使Vp和Vs分别增加了9%和20%。声速的如此大的跳跃表明,后石榴石转变比后aki转变更适合于在MTZ底部产生双重不连续,并结合环伍德石向Bdm +铁长石组合的转变。与Al-Aki的形成和溶解有关的声速的增加不太可能对MTZ敏感。在660-720 km深度附近,后石榴石、后尖晶石和后aki转变的组合可能抑制了上涌的热地幔和俯冲的冷板块。MTZ底部停滞的热LM物质加热了俯冲过程中堆积的辉钼矿和榴辉钼矿层。加热的MTZ可能参与了进一步的上升流。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Equation of state for Mg3Al2Si3O12 pyrope: Implications for post-garnet transitions and mantle dynamics

Equation of state for Mg3Al2Si3O12 pyrope: Implications for post-garnet transitions and mantle dynamics

Mantle convection is the dominant process driving the upwelling of hot materials and subduction of cold slabs. These processes are density-dependent and influenced by post-spinel and post-garnet transitions in the mantle transition zone (MTZ)/ lower mantle (LM). Knowledge of the Clapeyron slope of these transformations is used to express the dynamics of mantle blocks and is necessary for understanding the deep Earth. Here, we provide the Kunc-Einstein equation of state (EoS) for the pyrope Mg3Al2Si3O12 (Prp) calculated from a joint analysis of the experimentally measured isobaric heat capacity, bulk moduli, thermal expansion, pressure (P), unit cell volume (V), temperature (T) data. Based on our model, the bulk modulus and its pressure derivatives were K0,T0 = 168.5 GPa, K′0,T = 4.77, and V0 = 1501.7 Å. The optimised parameters include two Einstein temperatures, i.e., θ1 = 331 and θ2 = 1093 K, Grüneisen parameter at ambient condition γ0 = 1.77, infinite compression γ = 0 with β = 1.12 and an intrinsic anharmonicity parameter a0 = –20. The value for the thermal expansion coefficient was calculated to be α = 2.33·10−5 K−1, and the thermodynamic Grüneisen parameter was estimated as γth = 1.42. The obtained EoS for Prp and the preliminarily fitted EoS for Al-bearing akimotoite (Al-Aki), in combination with literature data on bridgmanite (Bdm) and corundum (Crn), allowed the calculation of the phase diagram of the system with 75 mol% MgSiO3 + 25 mol% Al2O3 under LM conditions. The transformation from Prp to Bdm + Crn was computed at 24 GPa and 1570 K and exhibited a slightly positive Clapeyron slope (dP/dT = 2.1 MPa/K). The stability field of Al-Aki was detected at T = 1250–1570 K and P = 23–27 GPa. At P values higher than 24–27 GPa, the Al-Aki transforms into a Bdm + Crn assemblage with a highly negative Clapeyron slope. Calculations of sound velocities for the studied phases showed that the transformation from Prp to Bdm + Crn increased Vp and Vs by up to 9 and 20%, respectively. Such a big jump in the sound velocities indicates that the post-garnet transition is a better candidate than the post-Aki transition for producing a double discontinuity at the base of the MTZ, in combination with the transformation of ringwoodite into the Bdm + ferropericlase assemblage. The increase in sound velocities associated with the formation and dissolution of Al-Aki is unlikely to be sensitive to the MTZ. The combination of post-garnet, post-spinel, and post-Aki transitions near 660–720 km depths may have sluggished both the upwelling hot mantle and the subducted cold plates. The stagnant, hot LM material at the base of MTZ warmed the harzburgite and eclogite layers stacked during subduction. The heated MTZ may have been involved in further upwelling.

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来源期刊
Physics of the Earth and Planetary Interiors
Physics of the Earth and Planetary Interiors 地学天文-地球化学与地球物理
CiteScore
5.00
自引率
4.30%
发文量
78
审稿时长
18.5 weeks
期刊介绍: Launched in 1968 to fill the need for an international journal in the field of planetary physics, geodesy and geophysics, Physics of the Earth and Planetary Interiors has now grown to become important reading matter for all geophysicists. It is the only journal to be entirely devoted to the physical and chemical processes of planetary interiors. Original research papers, review articles, short communications and book reviews are all published on a regular basis; and from time to time special issues of the journal are devoted to the publication of the proceedings of symposia and congresses which the editors feel will be of particular interest to the reader.
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