KOPRI Repository

Modeling for intercrystalline isotope diffusion

Cited 0 time in wos
Cited 0 time in scopus
Metadata Downloads
Modeling for intercrystalline isotope diffusion
Other Titles
광물간 동위원소 확산 모델링
Park, Changkun
동위원소; 모델링; 확산
Issue Date
Park, Changkun. 2017. Modeling for intercrystalline isotope diffusion. 2017년도 추계지질과학연합학술대회. 제주 컨벤션 센터. 2017.10.25~2017.10.28.
Stable isotope exchange between coexisting minerals can take place during cooling of a closed system, followed by isotopic diffusion through minerals. The result of stable isotope diffusion depends on the temperature, time, diffusion coefficients, fractionation factors, grain sizes and abundances of mineral phases. Since these factors can be determined by experiments and petrological studies, the cooling history of the system can be modeled. To model isotopic exchange between minerals and retrograde intra-crystalline diffusion in a closed system, it is assumed that 1) isotope concentration at grain boundaries is considered to be homogeneous at any points of grain boundaries, 2) mass flux of isotope is preserved (thus, net flux is zero), 3) concentration gradient at the grain surfaces leads to a solid-state isotope diffusion through individual grains, and 4) diffusion coefficients of minerals and isotopic concentrations at grain boundaries are changed with decreasing temperature (Eiler et al., 1994; Jenkin et al., 1994). This process continues until the system cools down to the diffusive closure temperatures of minerals. Results of modeling well reproduce concentration profiles observed in terrestrial rocks (e.g., Bonamici et al., 2011). The model is applied to refractory inclusions in extraterrestrial rocks to reproduce isotopic distributions in coexisting minerals, which could constrain cooling history of the inclusions in the early Solar System.
Conference Name
2017년도 추계지질과학연합학술대회
Conference Place
제주 컨벤션 센터
Conference Date
Files in This Item
General Conditions
      ROMEO Green
    Can archive pre-print and post-print or publisher's version/PDF
      ROMEO Blue
    Can archive post-print (ie final draft post-refereeing) or publisher's version/PDF
      ROMEO Yellow
    Can archive pre-print (ie pre-refereeing)
      ROMEO White
    Archiving not formally supported

    Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.