2012
DOI: 10.1103/physrevb.85.155130
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Observable NMR signal from circulating current order in YBCO

Abstract: Assuming, as suggested by recent neutron scattering experiments, that a broken symmetry state with orbital current order occurs in the pseudo-gap phase of the cuprate superconductors, we show that there must be associated equilibrium magnetic fields at various atomic sites in the unit cell, which should be detectable by NMR experiments.

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Cited by 26 publications
(38 citation statements)
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“…Our results challenge them as it remains ∼40° whatever the L value. It actually does not favour models in which θ goes to zero at L =0, such as LC models that include apical oxygens as an explanation for the tilt2324, where one would expect a L -dependent tilt. More generally, the observed temperature dependence of θ is not consistent with theories where the tilt direction is due to rigid geometrical factors.…”
Section: Discussionmentioning
confidence: 97%
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“…Our results challenge them as it remains ∼40° whatever the L value. It actually does not favour models in which θ goes to zero at L =0, such as LC models that include apical oxygens as an explanation for the tilt2324, where one would expect a L -dependent tilt. More generally, the observed temperature dependence of θ is not consistent with theories where the tilt direction is due to rigid geometrical factors.…”
Section: Discussionmentioning
confidence: 97%
“…In contrast, the correlated in-plane component develops only below T mag giving rise to an apparent tilt of the magnetic moment. Most theories that are interpretating the origin of the tilt, θ , focus on the Bragg peak L =1 (refs 24, 28, 29). Our results challenge them as it remains ∼40° whatever the L value.…”
Section: Discussionmentioning
confidence: 99%
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“…A more stringent test, if the orbital currents have the symmetry shown in Fig.1, is to examine the NMR linewidth for broadening that might reflect a small frequency splitting. Our measurements at all temperatures of the angular variation of the linewidth is less than 0.5 kHz which places a bound on orbital current fields of 0.4 G. According to Lederer and Kivelson,[19] orbital currents inferred from neutron scattering results [8,10,11] should lead to local fields of order H max ∼ 200 G oriented as indicated in Fig.1. Taken together, our measurements of the angular variations of the apical orbital shift and NMR linewidth, in-plane and out of-plane, place substantial constraints on predictions from the theory for a static orbital field to be less than 0.4 G.…”
mentioning
confidence: 83%
“…In addition, the Θ II phase (a q = 0 Fermi surface instability) faces the challenge of explaining the excitation gap in the pseudogap regime. Intense effort has been devoted to searching indirectly for orbital loop currents, using techniques such as NMR [47][48][49] and muon spin rotation, [50][51][52] but their existence in the cuprates remains inconclusive.…”
Section: Introductionmentioning
confidence: 99%