1996
DOI: 10.1103/physrevlett.76.1525
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Grazing Incidence Infrared Reflectivity ofLa1.85Sr0.15CuO4

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Cited by 36 publications
(18 citation statements)
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“…The grazing incidence geometry has been chosen because in this case the reflectivity is more sensitive to changes of optical conductivity due to opening of the superconducting gap. This experimental technique has been previously used to measure the s-wave gap of NbN and the d-wave gap of La 1.85 Sr 0.15 CuO 4 [10]. In addition, normal incidence spectra were collected in the same frequency range, which were qualitatively consistent with the grazing reflectance data reported in this paper.…”
supporting
confidence: 71%
“…The grazing incidence geometry has been chosen because in this case the reflectivity is more sensitive to changes of optical conductivity due to opening of the superconducting gap. This experimental technique has been previously used to measure the s-wave gap of NbN and the d-wave gap of La 1.85 Sr 0.15 CuO 4 [10]. In addition, normal incidence spectra were collected in the same frequency range, which were qualitatively consistent with the grazing reflectance data reported in this paper.…”
supporting
confidence: 71%
“…Some of the reported in-plane spectra show rich features in a far-infrared (FIR) region 13,14,15 , which are ascribed either to the LO-phonons 13 or to the excitation related to the polarons 14 . According to the variety of spectra, different values of the SC condensate were derived, ranging from 250 to 430 nm 10,11,12,13,14,15 in terms of the London penetration depth λ…”
Section: Introductionmentioning
confidence: 99%
“…The extracted T-dependence of ∆, with ∆(0) ≈ 0.75 THz (3.07 meV) and 2∆/k B T c ≈ 4.6, is shown in inset to panel b). ∆(T ) is plotted on top of TR, the transmissivity ratio T (ω, T )/T (ω, 16K), which is at each T normalized to its peak value (in a BCS SC, the transmissivity ratio peaks just above 2∆ [33]). Fig.…”
mentioning
confidence: 99%