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Phys. Rev. B 72, 064437 (2005) [13 pages]

Mapping spin-wave dispersions in stripe-ordered La2−xSrxNiO4 (x=0.275, 0.333)

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Hyungje Woo1,2,*, A. T. Boothroyd3, K. Nakajima4, T. G. Perring2, C. D. Frost2, P. G. Freeman3, D. Prabhakaran3, K. Yamada5, and J. M. Tranquada1
1Physics Department, Brookhaven National Laboratory, Upton, New York 11973, USA
2ISIS Facility, Rutherford Appleton Laboratory, Chilton, Didcot, Oxon, OX11 0QX, United Kingdom
3Department of Physics, Oxford University, Oxford, OX1 3PU, United Kingdom
4Neutron Science Research Center, Japan Atomic Energy Research Institute, Tokai, Ibaraki 319-1195, Japan
5Institute for Materials Research, Tohoku University, Sendai 980-8577, Japan

Received 29 April 2005; published 18 August 2005

Using the MAPS spectrometer at the ISIS spallation source, we have measured the magnetic excitations of single-crystal samples of stripe-ordered La2−xSrxNiO4 with x=0.333 and 0.275. The full two-dimensional spin-wave dispersions were obtained using incident energies of 60 and 160 meV. To analyze the excitations, we have evaluated a spin-only Hamiltonian describing diagonal, site-centered stripes in the linear spin-wave approximation. Besides the superexchange energy J within antiferromagnetic domains, we have considered effective exchange couplings J1 and J2 across a charge stripe coupling second-neighbor Ni sites along Ni-O bond directions and along the plaquette diagonal, respectively. From least-squares fits of the model to the measurements on the x=1∕3 sample at T=10 K, we find that the dispersions are well described by a model using just J and J1, but not J and J2. Consistent with an analysis of previous measurements, we find that J is about 90% of the superexchange energy of undoped La2NiO4 and J1J≈0.5. The excitations observed for x=0.275 are surprisingly similar to those for x=1∕3, despite the differing magnetic-ordering wave vectors; the main difference is a broadening of the excitations for x=0.275. For both samples, we find that one spin-wave branch has a gap of ∼20 meV, confirming a previous observation for x=1∕3. We discuss the possible origin of this gap.

© 2005 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevB.72.064437
DOI:
10.1103/PhysRevB.72.064437
PACS:
75.30.Ds, 61.12.Ex, 75.30.Fv, 71.45.Lr

*Present address: Department of Physics & Astronomy, University of Tennessee, Knoxville, TN 37996-1200, USA.