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Vyacheslav S. Rusakov

Publications and source records attributed to Vyacheslav S. Rusakov.

2 recordsLinked to original sources

57Fe Mössbauer study of unusual magnetic structure of multiferroic 3R-AgFeO2

We report new results of a 57Fe Mössbauer study of multiferroic 3R-AgFeO2 powder samples performed in a wide temperature range, including two points, TN1 ~ 14 K and TN2 ~ 9 K, of magnetic phase transitions. At the intermediate temperature range, TN2 < T < TN1, the 57Fe Mössbauer spectra can be described in terms of collinear spin-density-waves (SDW) with the inclusion of many high-order harmonics, indicating that the real magnetic structure of this ferrite appears to be more complicated than a pure sinusoidally modulated SDW. The spectra at low temperatures, T < TN2, consist of a Zeeman pattern with line broadenings and sizeable spectral asymmetry. It has been shown that the observed spectral shape is consistent with a transition to the elliptical cycloidal magnetic structure. An analysis of the experimental spectra was carried out under the assumption that the electric hyperfine interactions are modulated when the Fe3+ magnetic moment rotates with respect to the principal axis of the EFG tensor and emergence of the strong anisotropy of the magnetic hyperfine field Hhf at the 57Fe nuclei. The large and temperature-independent anharmonicity parameter, m ~ 0.78, of the cycloidal spin structure obtained from the experimental spectra results from easy-axis anisotropy in the plane of rotation of the iron spin. Analysis of different mechanisms of spin and hyperfine interactions in 3R-AgFeO2 and its structural analogue CuFeO2 points to a specific role played by the topology of the exchange coupling and the oxygen polarization in the delafossite structures.

cond-mat.str-el↗

Spectrophotometry of asteroids 32 Pomona, 145 Adeona, 704 Interamnia, 779 Nina, 330825, and 2012 QG42 and laboratory study of possible analog samples

Six asteroids including two NEAs, one of which is PHA, accessible for observation in September 2012 were investigated using a low-resolution spectrophotometry in the range 0.35-0.90 um with the aim to study features of their reflectance spectra. For the first time we discovered likely spectral signs (as a maximum at 0.4-0.6 um in reflectance spectra) of simultaneous sublimation activity and presence of a temporal coma on three primitive-type main-belt asteroids, Adeona, Interamnia, and Nina, being at perihelion distances or approaching to it. We suggest that such a cometary-like activity may be a common phenomenon at the highest subsolar surface temperatures for C and close type asteroids including considerable amounts of H2O and CO2 ices beneath the surface. However, excavation of fresh ice at recent impact event(s) could be an alternative explanation of the phenomenon. Similar absorption bands centered at 0.38, 0.44 and 0.67-0.71 um registered in the reflectance spectra of Adeona, Interamnia, and Nina clearly point to predominantly silicate surface matter. To specify its content, we performed laboratory investigations of ground samples of known carbonaceous chondrites (Orguel, Mighei, Murchison, and Boriskino) and seven samples of low-iron Mg serpentines as possible analogs of the asteroids. In particular, we found that the equivalent width of the band centered at 0.44 um in reflectance spectra of the low-Fe serpentine samples has a high correlation with content of Fe3+ (octahedral and tetrahedral). It means that the absorption feature can be used as an indicator of ferric iron in oxidized and hydrated low-Fe silicate compounds on asteroids (abridged).

astro-ph.EP↗