Paramagnetic collective electronic mode and low temperature hybrid modes in the far infrared dynamics of orthorhombic NdMnO₃

We report on the far- and mid-infrared reflectivity of NdMnO₃ from 4 to 300 K. Two main features are distinguished in the infrared spectra: active phonons in agreement with expectations for the orthorhombic D¹⁶<sub>2h</sub>-Pbnm (Z = 4) space group remaining constant down to 4 K and a we...

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Autores principales: Massa, Néstor Emilio, Campo, Leire del, De Sousa Meneses, Domingos, Echegut, Patrick, Martínez-Lope, María Jesús, Alonso, José Antonio
Formato: Articulo
Lenguaje:Inglés
Publicado: 2013
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Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/131564
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Sumario:We report on the far- and mid-infrared reflectivity of NdMnO₃ from 4 to 300 K. Two main features are distinguished in the infrared spectra: active phonons in agreement with expectations for the orthorhombic D¹⁶<sub>2h</sub>-Pbnm (Z = 4) space group remaining constant down to 4 K and a well defined collective excitation in the THz region due to e<sub>g</sub> electrons in a d-orbital fluctuating environment. We trace its origin to the NdMnO₃ high-temperature orbital disordered intermediate phase not being totally dynamically quenched at lower temperatures. This results in minute orbital misalignments that translate into randomized non-static e<sub>g</sub> electrons within orbitals yielding a room-temperature collective excitation. Below T<sub>N</sub> ∼ 78 K, electrons gradually localize, inducing long-range magnetic order as the THz band condenses into two modes that emerge pinned to the A-type antiferromagnetic order. They harden simultaneously down to 4 K, obeying power laws with T<sub>N</sub> as the critical temperature and exponents β ∼ 0.25 and β ∼ 0.53, as for a tri-critical point and Landau magnetic ordering, respectively. At 4 K they match known zone center spin wave modes. The power law dependence is concomitant with a second order transition in which spin modes modulate orbital instabilities in a magnetoelectric hybridized orbital-charge-spin-lattice scenario. We also found that phonon profiles also undergo strong changes at T<sub>N</sub> ∼ 78 K due to magnetoelasticity.