2015
DOI: 10.1103/physrevb.92.024419
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Nature of antiferromagnetic order in epitaxially strained multiferroicSrMnO3thin films

Abstract: Epitaxial films of SrMnO3 and bilayers of SrMnO3 / La0.67Sr0.33MnO3 have been deposited by pulsed laser deposition on different substrates, namely LaAlO3 (001), (LaAlO3)0.3(Sr2AlTaO6)0.7 (001) and SrTiO3 (001), allowing us to perform an exhaustive study of the dependence of antiferromagnetic order and exchange bias field on epitaxial strain. The Néel temperatures (TN ) of the SrMnO3 films have been determined by low energy muon spin spectroscopy. In agreement with theoretical predictions, TN is reduced as the … Show more

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Cited by 62 publications
(53 citation statements)
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“…Ferromagnetic (FM) and G-type antiferromagnetic (AFM) phases have been observed in SrCoO 3−δ films subject to low (SrTiO 3 substrate) and large (DyScO 3 substrate) tensile epitaxial strains, respectively 10 . An increase (decrease) of Néel temperature due to compressive (tensile) biaxial strain was predicted in AFM SrTcO 3 films 11 A very strong dependence of T N on biaxial strain (≈ 50 K per 1%) has been predicted 12 and subsequently confirmed experimentally 13 for G-type AFM phase of SrMnO 3 . The ability to drive a magnetic phase transition with a large entropy change, ∆S = 9 J/kgK, by means of biaxial strain was demonstrated in La 0.7 Ca 0.3 MnO 3 film on BaTiO 3 substrate.…”
mentioning
confidence: 75%
“…Ferromagnetic (FM) and G-type antiferromagnetic (AFM) phases have been observed in SrCoO 3−δ films subject to low (SrTiO 3 substrate) and large (DyScO 3 substrate) tensile epitaxial strains, respectively 10 . An increase (decrease) of Néel temperature due to compressive (tensile) biaxial strain was predicted in AFM SrTcO 3 films 11 A very strong dependence of T N on biaxial strain (≈ 50 K per 1%) has been predicted 12 and subsequently confirmed experimentally 13 for G-type AFM phase of SrMnO 3 . The ability to drive a magnetic phase transition with a large entropy change, ∆S = 9 J/kgK, by means of biaxial strain was demonstrated in La 0.7 Ca 0.3 MnO 3 film on BaTiO 3 substrate.…”
mentioning
confidence: 75%
“…19 . Here, the oxygen-pressure dependence on the perovskite phase stabilization is the direct evidence that the formation of oxygen vacancies during thin film growth plays a central role in its stability, since perovskite SMO is only stabilized under low oxygen pressure 28,36,37 . The formation of oxygen vacancies is charge compensated by a reduction of the formal oxidation state of some Mn 4+ to Mn 3+ , resulting in a chemical expansion of the crystal lattice, relieving the strain.…”
Section: Textmentioning
confidence: 98%
“…1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35 36 37 38 39 40 41 42 43 44 45 46 47 48 49 50 51 52 53 54 55 56 57 58 59 60 8 Earlier works in ferroelectric HoMnO 3 epitaxial films pointed out the interplay between strain gradients and the presence of oxygen vacancies and the possibility to modulate the strain gradients, and thus flexoelectricity and polarization, as a function of the oxygen pressure during the film growth 19 . Here, the oxygen-pressure dependence on the perovskite phase stabilization is the direct evidence that the formation of oxygen vacancies during thin film growth plays a central role in its stability, since perovskite SMO is only stabilized under low oxygen pressure 28,36,37 . The formation of oxygen vacancies is charge compensated by a reduction of the formal oxidation state of some Mn 4+ to Mn 3+ , resulting in a chemical expansion of the crystal lattice, relieving the strain.…”
mentioning
confidence: 98%
“…However, macroscopic magnetic measurements on our present sample with strain up to 3.8% (Supplemental Material Fig. 8 [29]) shows no detectable remnant magnetization down to ∼10 K, indicating that the system retains its antiferromangetic state [34]. In order to investigate the magnetic nature of the highly strained SMO films, x-ray absorption spectroscopy (XAS) and x-ray linear dichroism (XLD) were employed to probe the antiferromagnetic state [35].…”
Section: Strain Tuning Of Antiferromagnetic Ordering and Spin-lattmentioning
confidence: 99%