PVT equation of state of epsilon iron and its densities at inner core conditions

被引:10
|
作者
Garai, Jozsef [1 ,3 ]
Chen, Jiuhua [1 ,2 ]
Telekes, Gabor [3 ,4 ]
机构
[1] Florida Int Univ, Dept Mech & Mat Engn, Miami, FL 33174 USA
[2] Florida Int Univ, CeSMEC, Miami, FL 33199 USA
[3] Szent Istvan Univ, Ybl Miklos Fac Architecture & Civil Engn, H-1146 Budapest, Hungary
[4] Univ Debrecen, Fac Engn, H-4028 Debrecen, Hungary
关键词
Equation of state; epsilon iron; inner core density; temperature in the core; light elements in the inner core; X-RAY-DIFFRACTION; HIGH-PRESSURE; HIGH-TEMPERATURE; THERMAL EQUATION; EARTHS CORE; GPA; COMPRESSIBILITY; CONSTRAINTS; STABILITY; MANTLE;
D O I
10.2138/am.2011.3612
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
The first comprehensive PVT description of epsilon-Fe is presented by collecting the complete data set of previous experiments on epsilon iron, covering a pressure and temperature range of 6-306 GPa and 293-2255 K, respectively. A single set of equation of state parameters, which is able to cover the entire pressure and temperature range has been determined. The root mean square misfit of the residuals is 1.17 GPa for the PVT version of the Birch-Murnaghan equation of state. The equation of state uses an absolute reference frame (T = 0 K and P = 0 GPa) and follows a T = 0 (P=0)double right arrow T = T and then P = 0 (T=T)double right arrow P=P path, which eliminates the pressure effect on the volume coefficient of thermal expansion and the temperature effect on the pressure derivative of the bulk modulus. The calculated temperatures, which reproduce the PREM density, bulk modulus, and bulk seismic velocities at the inner core boundary, are 4640, 4070, and 3980 (+/-230) K, respectively, indicating that no light elements are necessary in the inner core. The calculated density deficit for the outer core at 4000-4600 K ICB temperatures is 4.4-3.5%.
引用
收藏
页码:828 / 832
页数:5
相关论文
共 50 条
  • [1] Thermodynamics of epsilon iron at core physical conditions
    Saxena, SK
    EARTH'S CORE: DYNAMICS, STRUCTURE, ROTATION, 2003, 31 : 129 - 136
  • [2] EQUATION OF STATE OF LIQUID-IRON AT EARTHS CORE CONDITIONS
    BOSCHI, E
    MULARGIA, F
    JOURNAL OF GEOPHYSICS-ZEITSCHRIFT FUR GEOPHYSIK, 1977, 43 (1-2): : 465 - 472
  • [3] EQUATION OF STATE OF ALPHA AND EPSILON PHASES OF IRON
    ANDREWS, DJ
    JOURNAL OF PHYSICS AND CHEMISTRY OF SOLIDS, 1973, 34 (05) : 825 - 840
  • [4] THEORETICAL EQUATION OF STATE FOR INNER CORE
    BUKOWINSKI, MST
    PHYSICS OF THE EARTH AND PLANETARY INTERIORS, 1977, 14 (04) : 333 - 344
  • [5] EQUATION OF STATE OF ALPHA AND EPSILON PHASES OF IRON
    ANDREWS, DJ
    TRANSACTIONS-AMERICAN GEOPHYSICAL UNION, 1970, 51 (11): : 828 - +
  • [6] Equation of state of iron under core conditions of large rocky exoplanets
    Smith, Raymond F.
    Fratanduono, Dayne E.
    Braun, David G.
    Duffy, Thomas S.
    Wicks, June K.
    Celliers, Peter M.
    Ali, Suzanne J.
    Fernandez-Panella, Amalia
    Kraus, Richard G.
    Swift, Damian C.
    Collins, Gilbert W.
    Eggert, Jon H.
    NATURE ASTRONOMY, 2018, 2 (06): : 452 - 458
  • [7] Equation of state of iron under core conditions of large rocky exoplanets
    Raymond F. Smith
    Dayne E. Fratanduono
    David G. Braun
    Thomas S. Duffy
    June K. Wicks
    Peter M. Celliers
    Suzanne J. Ali
    Amalia Fernandez-Pañella
    Richard G. Kraus
    Damian C. Swift
    Gilbert W. Collins
    Jon H. Eggert
    Nature Astronomy, 2018, 2 : 452 - 458
  • [8] Ab initio calculations of the elasticity of iron and iron alloys at inner core conditions: Evidence for a partially molten inner core?
    Vocadlo, Lidunka
    EARTH AND PLANETARY SCIENCE LETTERS, 2007, 254 (1-2) : 227 - 232
  • [9] Author Correction: Equation of state of iron under core conditions of large rocky exoplanets
    Raymond F. Smith
    Dayne E. Fratanduono
    David G. Braun
    Thomas S. Duffy
    June K. Wicks
    Peter M. Celliers
    Suzanne J. Ali
    Amalia Fernandez-Pañella
    Richard G. Kraus
    Damian C. Swift
    Gilbert W. Collins
    Jon H. Eggert
    Nature Astronomy, 2018, 2 : 591 - 591
  • [10] THE EQUATION OF STATE AT ULTRAHIGH DENSITIES AND ITS RELATIVISTIC LIMITATIONS
    ZELDOVICH, YB
    SOVIET PHYSICS JETP-USSR, 1962, 14 (05): : 1143 - 1147