2010
DOI: 10.1103/physrevb.81.024505
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Spin waves inJ1aJ1bJ2orthorhombic square-lattice Heisenberg models: Application to iron pnictide materials

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Cited by 38 publications
(40 citation statements)
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“…In previous observations of electronic nematic phases in different materials, there is usually a symmetry breaking field present, such as an external magnetic field, uniaxial pressure, or an orthorhombic crystalline lattice [12][13][14][15][16][17] , which is not the case here. The observation of a short-range spin nematic phase in the tetragonal state of BaFe 2 As 2 reveals the presence of strong spin-orbital coupling at temperatures above T N [17][18][19][20][21][22][23][24]29].…”
Section: Discussionmentioning
confidence: 99%
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“…In previous observations of electronic nematic phases in different materials, there is usually a symmetry breaking field present, such as an external magnetic field, uniaxial pressure, or an orthorhombic crystalline lattice [12][13][14][15][16][17] , which is not the case here. The observation of a short-range spin nematic phase in the tetragonal state of BaFe 2 As 2 reveals the presence of strong spin-orbital coupling at temperatures above T N [17][18][19][20][21][22][23][24]29].…”
Section: Discussionmentioning
confidence: 99%
“…These results provide compelling evidence for a nematic spin fluid that breaks the tetragonal C 4 symmetry of the underlying crystalline lattice and spontaneously forms without the need for uniaxial pressure. Moreover, we suggest that this spin anisotropy causes a splitting of the d xz and d yz orbital bands in the tetragonal phase [18][19][20][21][22][23][24] , which in turn leads to the orthorhombic lattice distortion and electronic anisotropy.…”
Section: Introductionmentioning
confidence: 99%
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“…Some systems are believed to possess good nesting properties [3][4][5], while some are not [6,11]. Also there have been many theories that emphasize the role of local Fe 3d electrons [12][13][14][15].…”
mentioning
confidence: 99%
“…This set of parameters corresponds to the neutron scattering observation that the spin-wave spectra is better fit with an AFM exchange along one direction and a weak FM exchange along the other. 73 The latter could arise from double exchange 57 or from the orbital geometries. 55 But, its sign or magnitude is not crucial for the phase transitions we report here.…”
Section: II Spin-orbital Modelmentioning
confidence: 99%