Testing the itinerancy of spin dynamics in superconducting Bi2Sr2CaCu2O8+δ

A systematic neutron-scattering study of large near-optimally doped single crystals of the cuprate superconductor, Bi 2 Sr 2 CaCu 2 O 8+ δ , indicates that its magnetic properties are governed by localized magnetic moments, and not by itinerant quasiparticles, as widely expected. Much of what we kno...

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Veröffentlicht in:Nature physics 2009-09, Vol.5 (9), p.642-646
Hauptverfasser: Xu, Guangyong, Gu, G. D., Hücker, M., Fauqué, B., Perring, T. G., Regnault, L. P., Tranquada, J. M.
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Sprache:eng
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Zusammenfassung:A systematic neutron-scattering study of large near-optimally doped single crystals of the cuprate superconductor, Bi 2 Sr 2 CaCu 2 O 8+ δ , indicates that its magnetic properties are governed by localized magnetic moments, and not by itinerant quasiparticles, as widely expected. Much of what we know about the electronic states of high-temperature superconductors is due to photoemission 1 , 2 , 3 and scanning tunnelling spectroscopy 4 , 5 studies of the compound Bi 2 Sr 2 CaCu 2 O 8+ δ . The demonstration of well-defined quasiparticles in the superconducting state has encouraged many theorists to apply the conventional theory of metals, Fermi-liquid theory, to the cuprates 6 , 7 , 8 , 9 . In particular, the spin excitations observed by neutron scattering at energies below twice the superconducting gap energy are commonly believed to correspond to an excitonic state involving itinerant electrons 10 , 11 , 12 , 13 , 14 . Here, we present the first measurements of the magnetic spectral weight of optimally doped Bi 2 Sr 2 CaCu 2 O 8+ δ in absolute units. The lack of temperature dependence of the local spin susceptibility across the superconducting transition temperature, T c , is incompatible with the itinerant calculations. Alternatively, the magnetic excitations could be due to local moments, as the magnetic spectrum is similar to that in La 1.875 Ba 0.125 CuO 4 (ref.  15 ), where quasiparticles 16 and local moments 17 coexist.
ISSN:1745-2473
1745-2481
DOI:10.1038/nphys1360