Muon Spin Relaxation Measurements of Na x CoO 2 · y H 2 OKanigel, A; Keren, A; Patlagan, L; Chashka, K. B; King, P. B
doi: 10.1103/PhysRevLett.92.257007pmid: 15245055
Using the transverse field muon spin relaxation technique, we measure the temperature dependence of the magnetic field penetration depth λ , in the Na x CoO 2 · y H 2 O system. We find that λ , which is determined by the superfluid density n s and the effective mass m * , is very small and on the edge of the TF- μ SR sensitivity. Nevertheless, the results indicate that this system obeys the Uemura relation. By comparing λ with the normal state electron density, we conclude that m * of the superconductivity carrier is 70 times larger than the mass of bare electrons. Finally, the order parameter in this system cannot be described by a complete gap over the entire Fermi surface.
Fluid Invasion in Porous Media: Viscous Gradient PercolationLam, Chi-Hang
doi: 10.1103/PhysRevLett.92.254503pmid: 15245015
We suggest that the dynamics of stable viscous invasion fronts in porous media depends on the volume capacitance of the media. At high volume capacitance, our network simulations provide numerical evidence of a scaling relation between the front width and its velocity. In the low volume capacitance regime, we derive a new effective scaling supported by network simulations and that is in agreement with previous experiments on imbibition in paper and collections of glass beads.
Sneutrino Condensate Source for Density Perturbations, Leptogenesis, <?format ?>and Low Reheat TemperatureMazumdar, Anupam ; Pérez-Lorenzana, Abdel
doi: 10.1103/PhysRevLett.92.251301pmid: 15244992
We bring together some known ingredients beyond the standard model physics that can explain the hot big bang model with the observed baryon asymmetry and also the fluctuations in the cosmic microwave background radiation with a minimal set of assumptions. We propose an interesting scenario where the inflaton energy density is dumped into an infinitely large extra dimension. Instead of the inflaton it is the right handed sneutrino condensate, which is acquiring a nonzero vacuum expectation value during inflation, whose fluctuations are responsible for the density perturbations seen in the cosmic microwave background radiation with a spectral index n s ≈ 1 . The decay of the condensate is explaining the reheating of the Universe with a temperature, T r h ≤ 10 9 GeV , and the baryon asymmetry of order one part in 10 10 with no baryon-isocurvature fluctuations.
External Time-Varying Fields and Electron CoherenceHsiang, Jen-Tsung ; Ford, L. H
doi: 10.1103/PhysRevLett.92.250402pmid: 15244987
The effect of time-varying electromagnetic fields on electron coherence is investigated. A sinusoidal electromagnetic field produces a time-varying Aharonov-Bohm phase. In a measurement of the interference pattern which averages over this phase, the effect is a loss of contrast. This is effectively a form of decoherence. We calculate the magnitude of this effect for various electromagnetic field configurations. The result seems to be sufficiently large to be observable.