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Title: Mapping spin-wave dispersions in stripe-ordered La{sub 2-x}Sr{sub x}NiO{sub 4} (x=0.275, 0.333)

Journal Article · · Physical Review. B, Condensed Matter and Materials Physics
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  1. Physics Department, Brookhaven National Laboratory, Upton, New York 11973 (United States)
  2. Department of Physics, Oxford University, Oxford, OX1 3PU (United Kingdom)
  3. Neutron Science Research Center, Japan Atomic Energy Research Institute, Tokai, Ibaraki 319-1195 (Japan)
  4. ISIS Facility, Rutherford Appleton Laboratory, Chilton, Didcot, Oxon, OX11 0QX (United Kingdom)
  5. Institute for Materials Research, Tohoku University, Sendai 980-8577 (Japan)

Using the MAPS spectrometer at the ISIS spallation source, we have measured the magnetic excitations of single-crystal samples of stripe-ordered La{sub 2-x}Sr{sub x}NiO{sub 4} 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 J{sub 1} and J{sub 2} 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 J{sub 1}, but not J and J{sub 2}. Consistent with an analysis of previous measurements, we find that J is about 90% of the superexchange energy of undoped La{sub 2}NiO{sub 4} and J{sub 1}/J{approx_equal}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 {approx}20 meV, confirming a previous observation for x=1/3. We discuss the possible origin of this gap.

OSTI ID:
20719317
Journal Information:
Physical Review. B, Condensed Matter and Materials Physics, Vol. 72, Issue 6; Other Information: DOI: 10.1103/PhysRevB.72.064437; (c) 2005 The American Physical Society; Country of input: International Atomic Energy Agency (IAEA); ISSN 1098-0121
Country of Publication:
United States
Language:
English