Abstract
We present Raman scattering studies of the structural and magnetic phases that accompany temperature- and field-dependent melting of charge- and orbital-order (COO) in and . Our results show that thermal and field-induced COO melting in exhibits three stages in a heterogeneous melting process: At low temperatures and fields we observe a long-range, strongly Jahn-Teller (JT) distorted-COO phase; at intermediate temperatures and/or fields, we find a coexistence regime comprising both strongly JT distorted-COO and weakly JT distorted/ferromagnetic metal (FMM) phases; and at high temperatures and/or high fields, we observe a weakly JT distorted homogeneous paramagnetic (PM) or ferromagnetic (FM) phase. In the high field-high temperature regime of and , we identify a clear structural change to a weakly JT distorted phase that is associated with either a Imma or Pnma structure. We are able to provide a complete structural phase diagram of for the temperature and field ranges and . Significantly, we provide evidence that the field-induced melting transition of is first-order, and resembles a crystallization transition of an “electronic solid.” We also investigate thermal and field-induced melting in to elucidate the role of disorder in melting of COO. We find that while thermal melting of COO in is quite similar to that in , field-induced melting of COO in the two systems is quite different in several respects: The field-induced transition from the COO phase to the weakly JT-distorted-FM phase in is very abrupt, and occurs at significantly lower fields ( at ) than in ( at ); the intermediate coexistence regime is much narrower in than in ; and the critical field increases with increasing temperature in , in contrast to the decrease in observed with increasing temperature in . To explain these differences, we propose that field-induced melting of COO in is best described as the field-induced percolation of FM domains, and we suggest that Griffiths phase physics may be an appropriate theoretical model for describing the unusual temperature- and field-dependent transitions observed in .
1 More- Received 30 September 2007
DOI:https://doi.org/10.1103/PhysRevB.77.134411
©2008 American Physical Society