28 August 2022 to 2 September 2022
Science and Technology Campus, University of Parma
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Phase diagram of the perovskite solid solution CaCu$_3$Ti$_{(4-x)}$Ru$_{x}$O$_{12}$ elucidated with bulk $\mu^+$SR

29 Aug 2022, 17:20
1h 40m
Science and Technology Campus, University of Parma

Science and Technology Campus, University of Parma

University of Parma, Italy
Poster Strongly correlated electron systems Posters

Speaker

Elisabetta Nocerino (KTH Royal Institute of Technology)

Description

The CaCu$_3$Ti$_{(4-x)}$Ru$_{(x)}$O$_{12}$ family, synthesized under high pressure (7.7 GPa) belongs to the perovskite class of materials. The ground state of the extremes of this solid solution are antiferromagnetic insulator for the x = 0 member, and itinerant-electron system, i.e., Pauli-paramagnetic metal, for the x = 4 member respectively [1,2]. The suppression of magnetic ordering from the x = 0 to the x = 4 member of the solid solution seems to be accompanied by non-Fermi liquid (NFL) behavior since CaCu$_3$Ti$_4$O$_{12}$ manifested indications of such a behavior in heat capacity measurements [3]. These features make the solid solution CaCu$_3$Ti$_{(4-x)}$Ru$_{(x)}$O$_{12}$ a promising candidate for possessing a Doniach-type phase diagram [4]. In this work we present the results of a bulk muon spin rotation study on the intermediate members of the solid solution, showing the evolution of the magnetic ground state going from antiferromagnetic to paramagnetic. Evidence of highly dynamical ground states are also found among the members of the solid solution and a tentative phase diagram as a function of the Ru content x is proposed.

[1] A. Collomb, D. Samaras, B. Bochu, and J. C. Joubert, Physica Status Solidi (a) 41, 459 (1977)
[2] A. Ramirez, G. Lawes, D. Li, and M. Subramanian, Solid State Communications 131, 251 (2004)
[3] A. Krimmel, A. Gunther, W. Kraetschmer, H. Dekinger, N. Buttgen, A. Loidl, S. G. Ebbing-haus, E.-W. Scheidt, and W. Scherer, Phys. Rev. B 78, 165126 (2008).
[4] S. Doniach, Physica B+C 91, 231 (1977)

Primary author

Elisabetta Nocerino (KTH Royal Institute of Technology)

Co-authors

Dr Ola K. Forslund (Chalmers) Frank Elson (KTH, Royal Institute of Technology) Dr Rasmus Palm (KTH Royal Institute of Technology) Ms Ugne Miniotaite (KTH Royal Institute of Technology, Sweden) Dr Hiroya Sakurai (NIMS) Mr Konstantinos Papadopulos (Chalmers University of Technology) Prof. Yasmine Sassa (Chalmers University of Technology) Jun Sugiyama (CROSS Neutron Science and Technology Center) Prof. Martin Mansson (KTH Royal Institute of Technology)

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