40 research outputs found

    Pressure dependence of the superconducting transition temperature in C6_6Yb and C6_6Ca

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    We have studied the evolution, with hydrostatic pressure, of the recently discovered superconductivity in the graphite intercalation compounds C6_6Yb and C6_6Ca. We present pressure-temperature phase diagrams, for both superconductors, established by electrical transport and magnetization measurements. In the range 0-1.2 GPa the superconducting transition temperature increases linearly with pressure in both materials with dTc/dP=+0.39K/GPadT_c/dP = +0.39 K/GPa and dTc/dP=+0.50K/GPadT_c/dP = +0.50 K/GPa for C6_6Yb and C6_6Ca respectively. The transition temperature in C6_6Yb, which has beenmeasured up to 2.3 GPa, reaches a peak at around 1.8 GPa and then starts to drop. We also discuss how this pressure dependence may be explained within a plasmon pairing mechanism.Comment: 4 pages, 3 figure

    Muon spin rotation study of the intercalated graphite superconductor CaC6 at low temperatures

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    Muon spin rotation (muSR) experiments were performed on the intercalated graphite CaC6 in the normal and superconducting state down to 20 mK. In addition, AC magnetization measurements were carried out resulting in an anisotropic upper critical field Hc2, from which the coherence lengths xi_ab(0)=36.3(1.5) nm and xi_c(0)=4.3(7) nm were estimated. The anisotropy parameter gamma_H= H_c2_ab/H_c2_c increases monotonically with decreasing temperature. A single isotropic s-wave description of superconductivity cannot account for this behaviour. From magnetic field dependent muSR experiments the absolute value of the in-plane magnetic penetretion depth lambda_ab=78(3) nm was determined. The temperature dependence of the superfluid density rho_s(T) is slightly better described by a two-gap than a single-gap model

    The Galactic Environment of the Sun: Interstellar Material Inside and Outside of the Heliosphere

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