1982
DOI: 10.1016/0001-6160(82)90039-6
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A study of interstitial atom configuration in fresh and aged iron-carbon martensite by mossbauer spectroscopy

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1983
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Cited by 45 publications
(28 citation statements)
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“…The B hf determined by MES for the η s resonance of samples ranged from 16.9 to 17.4 T, consistent with that of 17.4±0.5 T reported previously for this same alloy [19], and within the range of 16.2 [32] to 17.9 T [20] reported for η s . In [32] a distinction between ε or  was not made, but previous research suggests the resonance was due to  s [19]. The small fractions of the η s resonance necessitated the isomer shift (IS) and quadrupole splitting (QS) be fixed at 0.16 and -0.09 mm s -1 , respectively [19].…”
supporting
confidence: 90%
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“…The B hf determined by MES for the η s resonance of samples ranged from 16.9 to 17.4 T, consistent with that of 17.4±0.5 T reported previously for this same alloy [19], and within the range of 16.2 [32] to 17.9 T [20] reported for η s . In [32] a distinction between ε or  was not made, but previous research suggests the resonance was due to  s [19]. The small fractions of the η s resonance necessitated the isomer shift (IS) and quadrupole splitting (QS) be fixed at 0.16 and -0.09 mm s -1 , respectively [19].…”
supporting
confidence: 90%
“…The small fractions of the η s resonance necessitated the isomer shift (IS) and quadrupole splitting (QS) be fixed at 0.16 and -0.09 mm s -1 , respectively [19]. The B hf of the η ns resonance ranged from 25.1 to 25.6 T, falling within the range of 23.7 to 25.7 T and reported previously [19,28,32]. Similarly, the small η ns resonance necessitated that the IS and QS be fixed at 0.13 and -0.36 mm s -1 [19], respectively.…”
mentioning
confidence: 57%
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“…Upon tempering at 573 K for 1 hour (Figure 4(b)), a number of prominent peaks appeared in the diffraction patInvestigations carried out by several groups [7][8][9][10][11][12][13][14] reveal that the Mössbauer spectrum of fresh Fe-C martensite tern of the Fe-C sample. Most of the major new peaks can be indexed as that of the -Fe 3 C phase.…”
Section: A As-deposited Statementioning
confidence: 99%
“…4,10 As noted above, rather than being stoichiometric Fe 4 C, the carbon-rich regions tended to have a carbon content closer to 10 at. %, 14 a point that was highlighted by Ino et al 15 who denoted it as Fe 4 C x with x Ӷ 1. Taylor et al 4 on the basis of their original TEM and atom probe data on Fe-Ni-C martensites along with previous work including Mössbauer spectroscopy proposed that instead of ␥Ј-Fe 4 C, the carbon-rich regions could be better described as ␣Љ-Fe 16 C 2 , which is isostructural to the metastable ␣Љ-Fe 16 N 2 nitride.…”
Section: Introductionmentioning
confidence: 99%