Spin gaps and magnetic structure of NaxCoO2

ArXiv cond-mat/0510360 (2005)

Authors:

LM Helme, AT Boothroyd, R Coldea, D Prabhakaran, A Stunault, GJ McIntyre, N Kernavanois

Abstract:

We present two experiments that provide information on spin anisotropy and the magnetic structure of NaxCoO2. First, we report low-energy neutron inelastic scattering measurements of the zone-center magnetic excitations in the magnetically ordered phase of Na0.75CoO2. The energy spectra suggest the existence of two gaps, and are very well fitted by a spin-wave model with both in-plane and out-of-plane anisotropy terms. The gap energies decrease with increasing temperature and both gaps are found to have closed when the temperature exceeds the magnetic ordering temperature T_m~22 K. Secondly, we present neutron diffraction studies of Na0.85CoO2 with a magnetic field applied approximately parallel to the c axis. For fields in excess of ~8T a magnetic Bragg peak was observed at the (0,0,3) position in reciprocal space. We interpret this as a spin-flop transition of the A-type antiferromagnetic structure, and we show that the spin-flop field is consistent with the size of the anisotropy gap.

Bose-Einstein Condensation of Magnons in Cs2CuCl4

Physical Review Letters 95 (2005) 127202 4pp

Authors:

D Kovrizhin, T. Radu, H. Wilhelm, V. Yushankhai

21aXH-6 S=1/2擬2次元三角格子反強磁性体Cs_2CuBr_4の2-spinon励起(量子スピン系(二次元系),領域3(磁性,磁気共鳴))

(2005) 306

Authors:

小野 俊雄, Radu Coldea, Mechthild Enderle, Michael Marek Koza, 田中 秀数

Where is the spectral weight in magnetic neutron scattering in the cuprates?

(2005)

Authors:

J Lorenzana, G Seibold, R Coldea

Where is the spectral weight in magnetic neutron scattering in the cuprates?

ArXiv cond-mat/0507131 (2005)

Authors:

J Lorenzana, G Seibold, R Coldea

Abstract:

We present estimates in the Hubbard and Heisenberg models for the spectral weight in magnetic neutron scattering experiments on the cuprates. With the aid of spin-wave theory and the time dependent Gutzwiller approximation we discuss how the spectral weight is distributed among the different channels and between high and low energies. In addition to the well known total moment sum rule we discuss sum rules for each component of the dynamical structure factor tensor which are peculiar for spin 1/2 systems. The various factors that reduce the spectral weight at the relevant energies are singled out and analyzed like: shielding factors, weight at electronic energies, multimagnon process etc. Although about 10% ~ 15% of the naively expected weight is detected in experiments after consideration of these factors the missing weight is within the experimental uncertainties. A large fraction of the spectral weight is hard to detect with present experimental conditions.