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Phys. Rev. B 76, 214512 (2007) [15 pages]

Dispersion of the odd magnetic resonant mode in near-optimally doped Bi2Sr2CaCu2O8+δ

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B. Fauqué1, Y. Sidis1, L. Capogna2,3, A. Ivanov3, K. Hradil4, C. Ulrich2, A. I. Rykov5, B. Keimer2, and P. Bourges1,*
1Laboratoire Léon Brillouin, CEA-CNRS, CE-Saclay, 91191 Gif sur Yvette, France
2Max-Plank-Institute für Festkörperforschung, Heisenbergstrasse 1, 70569 Stuttgart, Germany
3Institut Laue-Langevin, 6 Rue J. Horowitz, 38042 Grenoble cedex 9, France
4Institut für Physikalische Chemie, Universität Göttingen, Tammanstrasse 6, 37077 Göttingen, Germany
5Department of Applied Chemistry, University of Tokyo, Hongo 7-3-1, Bunkyo-ku, Tokyo 113-8656, Japan

Received 4 January 2007; revised 28 August 2007; published 26 December 2007

We report a neutron scattering study of the spin excitation spectrum in the superconducting state of the slightly overdoped Bi2Sr2CaCu2O8+δ system (Tc=87 K). We focus on the dispersion of the resonance peak in the superconducting state that is due to a S=1 collective mode. The measured spin excitation spectrum bears a strong similarity to the spectrum of the YBa2Cu3O6+x system for a similar doping level (i.e., x∼0.95−1), which can be described as intersecting upward- and downward-dispersing branches. A close comparison of the threshold of the electron-hole spin flip continuum, known from angle resolved photoemission measurements in the same system, indicates that the magnetic response in the superconducting state is confined, in both energy and momentum, below the gapped Stoner continuum. In contrast to YBa2Cu3O6+x, the spin excitation spectrum is broader than the experimental resolution. In the framework of an itinerant-electron model, we quantitatively relate this intrinsic energy width to the superconducting gap distribution observed in scanning tunneling microscopy experiments. Our study further suggests a significant in-plane anisotropy of the magnetic response.

© 2007 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevB.76.214512
DOI:
10.1103/PhysRevB.76.214512
PACS:
74.25.Ha, 25.40.Fq, 74.72.Hs

*Author to whom correspondence should be addressed: email address; bourges@llb.saclay.cea.fr