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Please use this identifier to cite or link to this item: http://dspace.bits-pilani.ac.in:8080/jspui/xmlui/handle/123456789/14151
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dc.contributor.authorBandyopadhyay, Debashis-
dc.date.accessioned2024-02-09T06:35:14Z-
dc.date.available2024-02-09T06:35:14Z-
dc.date.issued1999-11-
dc.identifier.urihttps://link.springer.com/article/10.1023/A:1012678613739-
dc.identifier.urihttp://dspace.bits-pilani.ac.in:8080/jspui/xmlui/handle/123456789/14151-
dc.description.abstractThis paper reports 57Fe Mössbauer spectroscopic studies of the polycrystalline samples of the substitutionally disordered, isostructural (fcc), ternary alloy system Fe80-xNixCr20 for x = 30, 26, 19 and 14 in the temperature range of 10–295 K. The data have been analyzed in terms of the magnetic phase transitions occurring in these alloys by examining the temperature dependence of the various Mössbauer parameters like line‐width, center shift, resonance area, distribution of hyperfine field, P(H), and the average hyperfine field 〈H〉. An estimate of the magnetic transition temperature T C is made for the alloys with x = 30 and 26 and these results are compared with those previously obtained by magnetic measurements and neutron diffraction experiments. The data for the second order Doppler shift have been analyzed to estimate the Debye temperature ΘD for alloys with x = 30 and 26.en_US
dc.language.isoenen_US
dc.publisherSpringeren_US
dc.subjectPhysicsen_US
dc.subjectSpectroscopyen_US
dc.subjectMagnetic phaseen_US
dc.titleA study of the effect of annealing temperatures and time periods on the hyperfine field distributions of Fe79B16Si5 metallic glass near and below the crystallization temperature was carried out using 57Fe Mössbauer spectroscopy. The effect of crystallization during annealing as a function of annealing time on the average hyperfine magnetic field, <H>, and the relative change of the probability of hyperfine fields, P(H), with respect to that of the as-received sample are also discussed.en_US
dc.typeArticleen_US
Appears in Collections:Department of Physics

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