1994
DOI: 10.1016/0016-7037(94)90199-6
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X-ray photoelectron spectroscopic study of a pristine pyrite surface reacted with water vapour and air

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Cited by 317 publications
(184 citation statements)
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“…However, when the pyrrhotite is treated with conditioning under the nitrogen atmosphere for 20 min, the Fe species and their relative contents are similar to that of untreated pyrrhotite. Fe2p with those from references, the peaks A, B, C, D, and E are attributed to Fe2(Sx)3, FeOOH, Fe2O3, FeS, and Fe2(SO4)3, respectively [23][24][25]. As can be seen from Figure 10 and According to Figure 11 [24,25,27].…”
Section: Resultsmentioning
confidence: 62%
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“…However, when the pyrrhotite is treated with conditioning under the nitrogen atmosphere for 20 min, the Fe species and their relative contents are similar to that of untreated pyrrhotite. Fe2p with those from references, the peaks A, B, C, D, and E are attributed to Fe2(Sx)3, FeOOH, Fe2O3, FeS, and Fe2(SO4)3, respectively [23][24][25]. As can be seen from Figure 10 and According to Figure 11 [24,25,27].…”
Section: Resultsmentioning
confidence: 62%
“…As shown in Figure 10 of Fe2p with those from references, the peaks A, B, C, D, and E are attributed to Fe 2 (S x ) 3 , FeOOH, Fe 2 O 3 , FeS, and Fe 2 (SO 4 ) 3, respectively [23][24][25]. As can be seen from Figure 10 and Table 2, the Fe species of the untreated pyrrhotite surfaces mainly consist of Fe 2 (S x ) 3 , FeOOH, Fe 2 O 3 , and FeS, the relative contents of which are 45.83%, 21.95%, 15.78%, and 16.44%, respectively.…”
Section: Resultsmentioning
confidence: 68%
“…The Fe 2p spectra show a narrow peak at 707.2 eV which is recognized as a Fe 2p 3/2 signal from low-spin Fe(II) in the pyrite lattice. A second Fe 2p 3/2 contribution found at a higher binding energy (BE) is mainly due to a multiplet structure (four maxima plus satellite) with a highest intensity at ∼709.8 eV from surface Fe(III) oxyhydroxides [17][18][19][20][21][22]. The presence of this Fe 2p feature is in agreement with the O 1 s spectra containing an O 2− contribution (530.4 eV), which reduces in spectra taken with increasing excitation energy and, therefore, probing depth.…”
Section: Haxpesmentioning
confidence: 99%
“…Additional minor lines are ascribed to monosulfide (161.8 eV), and polysulfide (163.5 eV) and satellite at about 164.5 eV [17][18][19][20][21][22][23][24] and slightly vary with the excitation photon energy. The VB spectra are dominated by non-bonding Fe 3d 6 orbital states in the vicinity of 2 eV below the Fermi level [5][6][7].…”
Section: Haxpesmentioning
confidence: 99%
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