Modeling X-ray Line Shapes from Asphaltenes

被引:2
|
作者
Alqahtani, H. [1 ]
Lewis, J. Courtenay [1 ]
Shirokoff, J. [2 ]
机构
[1] Mem Univ Newfoundland, Dept Phys & Phys Oceanog, St John, NF A1B 3X7, Canada
[2] Mem Univ Newfoundland, Dept Proc Engn, St John, NF A1B 3X7, Canada
来源
XXIII INTERNATIONAL CONFERENCE ON SPECTRAL LINE SHAPES | 2017年 / 810卷
关键词
D O I
10.1088/1742-6596/810/1/012049
中图分类号
O433 [光谱学];
学科分类号
0703 ; 070302 ;
摘要
Structural studies of asphaltene in crude oil have been performed by x-ray diffraction (XRD). The XRD spectra were taken with a Rigaku Dmax 2200V/PC, and builtin JadeTM software was used for initial analysis. XRD was performed with Cu-K-a radiation operating at 40 KV and 40 mA, with a scan rate of 0.001 degrees 2 theta per second. The XRD data were first fitted with Pearson VII profiles and then with pseudo-Voigt profiles, and then modeled in Mathematica(C) using a generalized Fermi function (GFF). These fits also included several different backgrounds (linear, exponential, and Lorentzian). The results are discussed in terms of their accuracy with different combinations of background and line profile.
引用
收藏
页数:4
相关论文
共 50 条
  • [1] X-RAY PHOTOEMISSION LINE-SHAPES FROM SOLIDS AND SURFACES
    CITRIN, PH
    ABSTRACTS OF PAPERS OF THE AMERICAN CHEMICAL SOCIETY, 1979, (APR): : 109 - 109
  • [2] The determination of x-ray line shapes by a double crystal spectrometer
    Smith, LP
    PHYSICAL REVIEW, 1934, 46 (05): : 0343 - 0351
  • [3] MODIFICATIONS TO X-RAY LINE SHAPES DUE TO CRYSTAL DISTORTIONS
    COOPER, EP
    PHYSICAL REVIEW, 1951, 83 (04): : 885 - 885
  • [4] Modeling of the M X-ray line structures for tungsten and L X-ray line structures for molybdenum
    Slabkowska, K.
    Polasik, M.
    Syrocki, L.
    Szymanska, E.
    Rzadkiewicz, J.
    Pereira, N. R.
    17TH INTERNATIONAL CONFERENCE ON THE PHYSICS OF HIGHLY CHARGED IONS, 2015, 583
  • [5] X-ray diffraction of subfractions of petroleum asphaltenes
    Andersen, SI
    Jensen, JO
    Speight, JG
    ENERGY & FUELS, 2005, 19 (06) : 2371 - 2377
  • [6] CONSTRAINTS ON POROSITY AND MASS LOSS IN O-STAR WINDS FROM THE MODELING OF X-RAY EMISSION LINE PROFILE SHAPES
    Leutenegger, Maurice A.
    Cohen, David H.
    Sundqvist, Jon O.
    Owocki, Stanley P.
    ASTROPHYSICAL JOURNAL, 2013, 770 (01):
  • [7] LINE SHAPES IN SOFT X-RAY ABSORPTION SPECTRA OF SOLIDIFIED RARE GASES
    HAENSEL, R
    KEITEL, G
    KUNZ, C
    SCHREIBER, P
    PHYSICAL REVIEW LETTERS, 1970, 25 (04) : 208 - +
  • [8] LINE SHAPES IN SOFT X-RAY ABSORPTION SPECTRA OF SOLIDIFIED RARE GASES
    KUNZ, C
    HAENSEL, R
    KEITEL, G
    SCHREIBE.P
    BULLETIN OF THE AMERICAN PHYSICAL SOCIETY, 1970, 15 (03): : 248 - &
  • [9] INVESTIGATION OF STRUCTURE OF PETROLEUM ASPHALTENES BY X-RAY DIFFRACTION
    YEN, TF
    ERDMAN, JG
    POLLACK, SS
    ANALYTICAL CHEMISTRY, 1961, 33 (11) : 1587 - &
  • [10] SHAPES OF X-RAY NANOSECOND PULSES
    GORBACHEV, VM
    GORBUNOV, VV
    KURYAKIN, VF
    KOROLEV, VN
    PRIBORY I TEKHNIKA EKSPERIMENTA, 1972, (03): : 232 - +